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TTU Math2450 Calculus3 Sec 13.3

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    MAGDALENA TODA: Welcome
    to our review of 13.1.
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    How many of you didn't
    get your exams back?
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    I have your exam, and yours.
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    And you have to wait.
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    I don't have it with me.
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    I have it in my office.
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    If you have questions
    about the score,
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    why don't you go ahead and
    email me right after class.
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    Chapter 13 is a very
    physical chapter.
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    It has a lot to do with
    mechanical engineering,
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    with mechanics,
    physics, electricity.
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    You're going to see things,
    weird things like work.
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    You've already seen work.
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    Do you remember the definition?
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    So we define the work
    as a path integral
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    along the regular curve.
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    And by regular curve-- I'm
    sorry if I'm repeating myself,
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    but this is part of the
    deal-- R is the position
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    vector in R3 that is class C1.
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    That means differentiable and
    derivatives are continuous.
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    Plus you are not
    allowed to stop.
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    So no matter how drunk,
    the bug has to keep flying,
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    and not even for a
    fraction of a second is he
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    or she allowed to
    have velocity 0.
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    At no point I want
    to have velocity 0.
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    And that's the position vector.
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    And then you have some force
    field acting on you-- no,
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    acting on the particle
    at every moment.
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    So you have an F that is
    acting at location xy.
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    Maybe if you are in space,
    let's talk about the xyz,
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    where x is a function of
    t, y is a functional of t,
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    z is a function of t,
    which is the same as saying
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    that R of t, which is the given
    position vector, is x of t
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    y of t.
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    Let me put angular bracket,
    although I hate them,
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    because you like angular
    brackets for vectors.
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    F is also a nice function.
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    How nice?
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    We discussed a
    little bit last time.
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    It really doesn't
    have to be continuous.
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    The book assumes it continues.
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    It has to be
    integrable, so maybe it
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    could be piecewise continuous.
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    So I had nice enough, was
    it continues piecewise.
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    And we define the work as
    being the path integral over c.
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    I keep repeating, because
    that's going to be on the final
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    as well.
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    So all the notions
    that are important
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    should be given enough
    attention in this class.
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    Hi.
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    So do you guys remember
    how we denoted F?
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    F was, in general, three
    components in our F1, F2, F3.
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    They are functions of
    the position vector,
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    or the position xyz.
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    And the position is
    a function of time.
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    So all in all, after
    you do all the work,
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    keep in mind that when you
    multiply with a dot product,
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    the integral will give you what?
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    A time integral?
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    From a time T0 to a time
    T1, you are here at time T0
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    and you are here at time T1.
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    Maybe your curve is
    piecewise, differentiable,
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    you don't know what it is.
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    But let's assume just a
    very nice, smooth arc here.
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    Of what?
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    Of F1 times what is that?
    x prime of t plus F2 times
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    y prime of t, plus F3
    times z prime of t dt.
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    So keep in mind that
    Mr. dR is your friend.
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    And he was-- what was he?
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    Was defined as the
    velocity vector multiplied
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    by the infinitesimal element dt.
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    Say again, the
    velocity vector prime
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    was a vector in F3 quantified
    by the infinitesimal element dt.
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    So we reduce this Calc
    3 notion path integral
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    to a Calc 1 notion, which was a
    simple integral from t0 to t1.
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    And we've done a
    lot of applications.
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    What else have we done?
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    We've done some
    integral of this type
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    over another curve, script c.
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    I'm repeating mostly for Alex.
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    You're caught in the process.
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    And there are two or three
    people who need an update.
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    Maybe I have another
    function of g and ds.
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    And this is an integral that
    in the end will depend on s.
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    But s itself depends on t.
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    So if I were to re-express
    this in terms of d,
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    how would I re-express
    the whole thing?
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    g of s, of t, whatever that
    is, then Mr. ds was what?
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    STUDENT: s prime of t.
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    MAGDALENA TODA: Right.
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    So this was the-- that s
    prime of t was the speed.
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    The speed of the arc of a curve.
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    So you have an R of
    t and R3, a vector.
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    And the speed was,
    by definition,
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    arc length element was
    by definition integral
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    from 2t0 to t.
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    Of the speed R prime
    magnitude d tau.
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    I'll have you put tau
    because I'm Greek,
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    and it's all Greek to me.
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    So the tau, some people call
    the tau the dummy variable.
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    I don't like to call it dumb.
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    It's a very smart variable.
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    It goes from t0 to t, so what
    you have is a function of t.
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    This guy is speed.
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    So when you do that
    here, ds becomes speed,
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    R prime of t times dt.
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    This was your old friend ds.
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    And let me put it on top
    of this guy with speed.
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    Because he was so
    important to you,
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    you cannot forget about him.
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    So that was review of--
    reviewing of 13.1 and 13.2
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    There were some things in
    13.3 that I pointed out
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    to you are important.
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    13.3 was independence of path.
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    Everybody write, magic-- no.
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    Magic section.
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    No, have to be serious.
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    So that's independence of path
    of certain type of integrals,
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    of some integrals.
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    And an integral like
    that, a path integral
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    is independent of path.
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    When would such an animal--
    look at this pink animal,
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    inside-- when would
    this not depend
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    on the path you are taking
    between two given points?
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    So I can move on another
    arc and another arc
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    and another regular arc, and
    all sorts of regular arcs.
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    It doesn't matter
    which path I'm taking--
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    STUDENT: If that
    force is conservative.
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    MAGDALENA TODA: If the
    force is conservative.
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    Excellent, Alex.
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    And what did it mean for a
    force to be conservative?
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    How many of you
    know-- it's no shame.
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    Just raise hands.
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    If you forgot what it is,
    don't raise your hand.
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    But if you remember what it
    means for a force F force
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    field-- may the force be
    with you-- be conservative,
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    then what do you do?
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    Say F is conservative
    by definition.
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    When, if and only, F
    there is a so-called--
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    STUDENT: Scalar.
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    MAGDALENA TODA: --potential.
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    Scalar potential, thank you.
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    I'll fix that.
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    A scalar potential function f.
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    Instead of there is, I
    didn't want to put this.
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    Because a few
    people told me they
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    got scared about
    the symbolistics.
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    This means "there exists."
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    OK, smooth potential
    such that-- at least
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    is differential [INAUDIBLE]
    1 such that the nabla of f--
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    what the heck is that?
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    The gradient of this little
    f will be the given F.
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    And we saw all sorts of wizards
    here, like, Harry Potter,
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    [INAUDIBLE] well,
    there are many,
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    Alex, Erin, many,
    many-- Matthew.
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    So what did they do?
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    They guessed the
    scalar potential.
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    I had to stop because
    there are 10 of them.
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    It's a whole school
    of Harry Potter.
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    How do they find the little f?
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    Through witchcraft.
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    No.
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    Normally you should--
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    STUDENT: I've actually
    done it through witchcraft.
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    Tell you that?
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    MAGDALENA TODA: You did.
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    I think you can do it
    through witchcraft.
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    But practically everybody
    has the ability to guess.
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    Why do we have the ability
    to guess and check?
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    Because our brain does
    the integration for you.
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    Whether you tell your
    brain to stop or not,
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    when your brain, for example,
    sees is kind of function--
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    and now I'm gonna
    test your magic skills
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    on a little harder one.
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    I didn't want to do an
    R2 value vector function.
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    Let me go to R3.
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    But I know that you have
    your witchcraft handy.
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    So let's say somebody
    gave you a force field
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    that is yz i plus xzj plus xyk.
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    And you're going to jump and
    say this is a piece of cake.
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    I can see the scalar potential
    and just wave my magic wand,
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    and I get it.
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    STUDENT: [INAUDIBLE]
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    MAGDALENA TODA: Oh my god, yes.
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    Guys, you saw it fast.
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    OK, I should be proud of you.
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    And I am proud of you.
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    I've had made classes
    where the students couldn't
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    see any of the scalar
    potentials that I gave them,
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    that I asked them to guess.
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    How did you deal with it?
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    You integrate this
    with respect to F?
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    In the back of
    your mind you did.
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    And then you guessed
    one, and then you
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    said, OK so should be xyz.
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    Does it verify my
    other two conditions?
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    And you say, oh yeah, it does.
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    Because of I prime with respect
    to y, I have exactly xz.
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    If I prime with respect to c I
    have exactly xy, so I got it.
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    And even if somebody
    said xyz plus 7,
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    they would still be right.
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    In the end you can have
    any xyz plus a constant.
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    In general it's not
    so easy to guess.
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    But there are lots of examples
    of conservative forces where
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    you simply cannot see the scalar
    potential or cannot deduce it
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    like in a few seconds.
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    Expect something easy,
    though, like that,
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    something that you can see.
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    Let's see an example.
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    Assume this is your force field
    acting on a particle that's
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    moving on a curving space.
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    And it's stubborn and it
    decides to move on a helix,
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    because it's a-- I don't
    know what kind of particle
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    would move on a
    helix, but suppose
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    a lot of particles, just a
    little train or a drunken bug
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    or something.
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    And you were moving
    on another helix.
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    Now suppose that helix will
    be R of t equals cosine t
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    sine t and t where you
    have t as 0 to start with.
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    What do I have at 0?
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    The point 1, 0, 0.
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    That's the point,
    let's call it A.
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    And let's call this B. I
    don't know what I want to do.
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    I'll just do a
    complete rotation,
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    just to make my life easier.
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    And this is B. And that
    will be A at t equals 0
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    and B equals 2 pi.
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    So what will this be at B?
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    STUDENT: 1, 0, 2 pi.
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    MAGDALENA TODA: 1, 0, and 2 pi.
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    So you perform a complete
    rotation and come back.
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    Now, if your force is
    conservative, you are lucky.
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    Because you know the theorem
    that says in that case
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    the work integral will
    be independent of path.
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    And due to the theorem in-- what
    section was that again-- 13.3,
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    independence of path,
    you know that this
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    is going to be-- let me rewrite
    it one more time with gradient
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    of f instead of big F.
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    And this will become what,
    f of the q-- not the q.
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    In the book it's f of q minus
    f of q. f of B minus f of A,
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    right?
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    What does this mean?
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    You have to measure
    the-- to evaluate
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    the coordinates of
    this function xyz
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    where t equals 2 pi minus
    xyz where t equals what?
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    0.
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    And now I have to be
    careful, because I
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    have to evaluate them.
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    So when t is 0 I have x
    is 1, y is 0, and t is 0.
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    In the end it doesn't matter.
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    I can get 0-- I
    can get 0 for this
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    and get 0 for that as well.
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    So when this is 2 pi I get
    x equals 1, y equals 0,
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    and t equals 2 pi.
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    So in the end, both products
    are 0 and I got a 0.
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    So although the [INAUDIBLE]
    works very hard-- I mean,
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    works hard in our perception
    to get from a point
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    to another-- the work is 0.
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    Why?
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    Because it's a vector
    value thing inside.
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    And there are some
    annihilations going on.
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    So that reminds me
    of another example.
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    So we are done
    with this example.
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    Let's go back to our washer.
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    I was just doing
    laundry last night
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    and I was thinking of
    the washer example.
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    And I thought of a small
    variation of the washer
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    example, just assuming that
    I would give you a pop quiz.
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    And I'm not giving you
    a pop quiz right now.
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    But if I gave you
    a pop quiz now,
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    I would ask you example
    two, the washer.
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    It is performing
    a circular motion,
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    and I want to know
    the work performed
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    by the centrifugal force
    between various points.
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    So have the circular motion,
    the centrifugal force.
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    This is the
    centrifugal, I'm sorry.
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    I'll take the centrifugal force.
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    And that was last
    time we discussed
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    that, that was extending
    the radius of the initial--
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    the vector value position.
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    So you have that in
    every point, xi plus yj.
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    And you want F to
    be able xi plus yj.
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    But it points outside
    from the point
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    on the circular trajectory.
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    And I asked you, find
    out what you performed
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    by F in one full rotation.
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    We gave the equation of motion,
    being cosine t y sine t,
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    if you remember from last time.
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    And then W2, let's
    say, is performed by F
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    from t equals 0 to t equals pi.
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    I want that as well.
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    And W2 performed by F from
    t-- that makes t0 to t
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    equals pi-- t equals 0
    to t equals pi over 4.
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    These are all very
    easy questions,
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    and you should be able to
    answer them in no time.
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    Now, let me tell you something.
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    We are in plane, not in space.
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    But it doesn't matter.
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    It's like the third quadrant
    would be 0, piece of cake.
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    Your eye should be so
    well-trained that when
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    you look at the force
    field like that,
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    and people talk about what
    you should ask yourself,
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    is it conservative?
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    And it is conservative.
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    And that means little f is what?
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    Nitish said that yesterday.
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    Why did you go there?
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    You want to sleep today?
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    I'm just teasing you.
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    I got so comfortable with
    you sitting in the front row.
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    STUDENT: I took his spot.
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    STUDENT: She doesn't like
    you sitting over here.
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    MAGDALENA TODA: It's OK.
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    It's fine.
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    I still give him credit
    for what he said last time.
  • 19:17 - 19:20
    So do you guys remember,
    he gave us this answer?
  • 19:20 - 19:23
    x squared plus y squared over
    2, and he found the scalar
  • 19:23 - 19:27
    potential through witchcraft
    in about a second and a half?
  • 19:27 - 19:28
    OK.
  • 19:28 - 19:31
    We are gonna conclude something.
  • 19:31 - 19:36
    Do you remember that I found the
    answer by find the explanation?
  • 19:36 - 19:39
    I got W to be 0.
  • 19:39 - 19:45
    But if I were to find another
    explanation why the work would
  • 19:45 - 19:50
    be 0 in this case, it
    would have been 0 anyway
  • 19:50 - 19:53
    for any force field.
  • 19:53 - 19:58
    Even if I took the F
    to be something else.
  • 19:58 - 20:03
    Assume that F would be
    G. Really wild, crazy,
  • 20:03 - 20:07
    but still differentiable
    vector value function.
  • 20:07 - 20:09
    G differential.
  • 20:09 - 20:15
    Would the work that we
    want be the same for G?
  • 20:15 - 20:16
    STUDENT: Yeah.
  • 20:16 - 20:17
    MAGDALENA TODA: Why?
  • 20:17 - 20:18
    STUDENT: Because of
    displacement scenario.
  • 20:18 - 20:21
    MAGDALENA TODA: Since
    it's conservative,
  • 20:21 - 20:23
    you have a closed loop.
  • 20:23 - 20:26
    So the closed loop
    will say, thick F
  • 20:26 - 20:30
    at that terminal point minus
    thick F at the initial point.
  • 20:30 - 20:34
    But if a loop motion,
    your terminal point
  • 20:34 - 20:35
    is the initial point.
  • 20:35 - 20:36
    Duh.
  • 20:36 - 20:41
    So you have the
    same point, the P
  • 20:41 - 20:44
    equals qe if it's
    a closed curve.
  • 20:44 - 20:48
    So for a closed curve--
    we also call that a loop.
  • 20:48 - 20:50
    With a basketball, it
    would have been too easy
  • 20:50 - 20:55
    and you would have gotten a
    dollar for free like that.
  • 20:55 - 20:58
    So any closed curve
    is called a loop.
  • 20:58 - 21:02
    If your force field is
    conservative-- attention,
  • 21:02 - 21:05
    you might have examples
    like that in the exams--
  • 21:05 - 21:09
    then it doesn't matter
    who little f is,
  • 21:09 - 21:13
    if p equals q you get 0 anyway.
  • 21:13 - 21:16
    But the reason why I
    said you would get 0
  • 21:16 - 21:21
    on the example of last time
    was a slightly different one.
  • 21:21 - 21:24
    What does the engineer
    say to himself?
  • 21:24 - 21:26
    STUDENT: Force is perpendicular.
  • 21:26 - 21:26
    MAGDALENA TODA: Yeah.
  • 21:26 - 21:27
    Very good.
  • 21:27 - 21:29
    Whenever the force
    is perpendicular
  • 21:29 - 21:33
    to the trajectory, I'm going
    to get 0 for the force.
  • 21:33 - 21:37
    Because at every
    moment the dot product
  • 21:37 - 21:41
    between the force and the
    displacement direction,
  • 21:41 - 21:45
    which would be like dR, the
    tangent to the displacement,
  • 21:45 - 21:47
    would be [INAUDIBLE].
  • 21:47 - 21:50
    And cosine of [INAUDIBLE] is 0.
  • 21:50 - 21:51
    Duh.
  • 21:51 - 21:53
    So that's another reason.
  • 21:53 - 22:00
    Reason of last time
    was F perpendicular
  • 22:00 - 22:05
    to the R prime
    direction, R prime
  • 22:05 - 22:11
    being the velocity-- look,
    when I'm moving in a circle,
  • 22:11 - 22:13
    this is the force.
  • 22:13 - 22:15
    And I'm moving.
  • 22:15 - 22:18
    This is my velocity, is
    the tangent to the circle.
  • 22:18 - 22:22
    And the velocity and the normal
    are always perpendicular,
  • 22:22 - 22:23
    at every point.
  • 22:23 - 22:24
    That's why I have 0.
  • 22:24 - 22:27
  • 22:27 - 22:32
    So note that even if I
    didn't take a close look,
  • 22:32 - 22:36
    why would the answer
    be from 0 to pi?
  • 22:36 - 22:39
    Still?
  • 22:39 - 22:43
    0 because of that.
  • 22:43 - 22:44
    0.
  • 22:44 - 22:47
    How about from 0 to pi over 4?
  • 22:47 - 22:50
    Still 0.
  • 22:50 - 22:52
    And of course if somebody
    would not believe them,
  • 22:52 - 22:55
    if somebody would not
    understand the theory,
  • 22:55 - 22:58
    they would do the work and
    they would get to the answer
  • 22:58 - 23:01
    and say, oh my
    god, yeah, I got 0.
  • 23:01 - 23:03
    All right?
  • 23:03 - 23:04
    OK.
  • 23:04 - 23:10
    Now, what if somebody--
    and I want to spray this.
  • 23:10 - 23:12
    Can I go ahead and
    erase the board
  • 23:12 - 23:15
    and move onto example
    three or whatever?
  • 23:15 - 23:16
    Yes?
  • 23:16 - 23:17
    OK.
  • 23:17 - 23:19
    All right.
  • 23:19 - 23:22
    STUDENT: Could you say
    non-conservative force?
  • 23:22 - 23:24
    MAGDALENA TODA: Yeah,
    that's what I-- exactly.
  • 23:24 - 23:26
    You are a mind reader.
  • 23:26 - 23:32
    You are gonna guess my mind.
  • 23:32 - 23:44
  • 23:44 - 23:47
    And I'm going to
    pick a nasty one.
  • 23:47 - 23:50
    And since I'm doing
    review anyway,
  • 23:50 - 23:51
    you may have one like that.
  • 23:51 - 23:55
    And you may have both one that
    involves a conservative force
  • 23:55 - 24:00
    field and one that does not
    involve a conservative force
  • 24:00 - 24:01
    field.
  • 24:01 - 24:07
    And we can ask you, find us the
    work belong to different path.
  • 24:07 - 24:12
    And I've done this
    type of example before.
  • 24:12 - 24:15
    Let's take F of
    x and y in plane.
  • 24:15 - 24:29
    In our two I take xyi
    plus x squared y of j.
  • 24:29 - 24:35
    And the problem would
    involve my favorite picture,
  • 24:35 - 24:39
    y equals x squared and y
    equals x, our two paths.
  • 24:39 - 24:41
    One is the straight path.
  • 24:41 - 24:44
    One is the [INAUDIBLE] path.
  • 24:44 - 24:46
    They go from 0,
    0 to 1, 1 anyway.
  • 24:46 - 24:49
  • 24:49 - 24:58
    And I'm asking you to
    find W1 along path one
  • 24:58 - 25:01
    and W2 along path two.
  • 25:01 - 25:06
    And of course,
    example three, if this
  • 25:06 - 25:10
    were conservative
    you would say, oh,
  • 25:10 - 25:12
    it doesn't matter
    what path I'm taking,
  • 25:12 - 25:15
    I'm still getting
    the same answer.
  • 25:15 - 25:17
    But is this conservative?
  • 25:17 - 25:18
    STUDENT: No.
  • 25:18 - 25:20
    Because you said it wasn't.
  • 25:20 - 25:21
    MAGDALENA TODA: Very good.
  • 25:21 - 25:23
    So how do you know?
  • 25:23 - 25:26
    That's one test
    when you are in two.
  • 25:26 - 25:31
    There is the magic test that
    says-- let's say this is M,
  • 25:31 - 25:37
    and let's say this is N. You
    would have to check if M sub--
  • 25:37 - 25:37
    STUDENT: y.
  • 25:37 - 25:38
    MAGDALENA TODA: y.
  • 25:38 - 25:39
    Very good.
  • 25:39 - 25:40
    I'm proud of you.
  • 25:40 - 25:42
    You're ready for
    3350, by the way.
  • 25:42 - 25:44
    Is equal to N sub x.
  • 25:44 - 25:47
    M sub y is x.
  • 25:47 - 25:49
    N sub x is 2xy.
  • 25:49 - 25:52
    They are not equal.
  • 25:52 - 25:55
    So that's me crying that I have
    to do the work twice and get--
  • 25:55 - 25:58
    probably I'll get two
    different examples.
  • 25:58 - 26:01
  • 26:01 - 26:04
    If you read the book--
    I'm afraid to ask
  • 26:04 - 26:09
    how many of you opened the
    book at section 13.2, 13.3.
  • 26:09 - 26:12
    But did you read
    it, any of them?
  • 26:12 - 26:13
    STUDENT: Nitish read it.
  • 26:13 - 26:15
    MAGDALENA TODA: Oh, good.
  • 26:15 - 26:20
    There is another criteria for
    a force to be conservative.
  • 26:20 - 26:22
    If you are, it's piece of cake.
  • 26:22 - 26:23
    You do that, right?
  • 26:23 - 26:24
    MAGDALENA TODA: Yes, sir?
  • 26:24 - 26:26
    STUDENT: Curl has frequency 0.
  • 26:26 - 26:27
    MAGDALENA TODA: The curl
    criteria, excellent.
  • 26:27 - 26:29
    The curl has to be zero.
  • 26:29 - 26:39
    So if F in R 3 is
    conservative, then you'll
  • 26:39 - 26:40
    get different order curve.
  • 26:40 - 26:42
    Curl F is 0.
  • 26:42 - 26:45
    Now let's check what
    the heck was curl.
  • 26:45 - 26:48
    You see, mathematics
    is not a bunch
  • 26:48 - 26:52
    of these joint discussions
    like other sciences.
  • 26:52 - 26:55
    In mathematics, if you don't
    know a section or you skipped
  • 26:55 - 26:58
    it, you are sick, you
    have a date that day,
  • 26:58 - 27:03
    you didn't study, then it's
    all over because you cannot
  • 27:03 - 27:07
    understand how to work out the
    problems and materials if you
  • 27:07 - 27:08
    skip the section.
  • 27:08 - 27:12
    Curl was the one
    where we learned
  • 27:12 - 27:16
    that we used the determinant.
  • 27:16 - 27:17
    That's the easiest story.
  • 27:17 - 27:21
    It came with a t-shirt,
    but that t-shirt really
  • 27:21 - 27:26
    doesn't help because
    it's easier to,
  • 27:26 - 27:28
    instead of memorizing
    the formula,
  • 27:28 - 27:31
    you set out the determinant.
  • 27:31 - 27:34
    So you have the operator
    derivative with respect
  • 27:34 - 27:41
    to x, y z followed by what?
  • 27:41 - 27:43
    F1, F2, F3.
  • 27:43 - 27:47
    Now in your case, I'm
    asking you if you did it
  • 27:47 - 27:52
    for this F, what is
    the third component?
  • 27:52 - 27:53
    STUDENT: The 0.
  • 27:53 - 27:55
    MAGDALENA TODA: The
    0, so this guy is 0.
  • 27:55 - 28:00
    This guy is X squared
    Y, and this guy is xy.
  • 28:00 - 28:02
    And it should be
    a piece of cake,
  • 28:02 - 28:04
    but I want to do
    it one more time.
  • 28:04 - 28:09
    I times the minor derivative
    of 0 with respect to y
  • 28:09 - 28:12
    is 0 minus derivative
    of x squared
  • 28:12 - 28:15
    y respect to 0, all
    right, plus j minus
  • 28:15 - 28:18
    j because I'm alternating.
  • 28:18 - 28:20
    You've known enough
    in your algebra
  • 28:20 - 28:23
    to know why I'm expanding
    along the first row.
  • 28:23 - 28:26
    I have a minus, all
    right, then the x
  • 28:26 - 28:34
    of 0, 0 derivative of xy
    respect to the 0 plus k times
  • 28:34 - 28:38
    the minor corresponding
    to k derivative 2xy.
  • 28:38 - 28:45
  • 28:45 - 28:46
    Oh, and the derivative--
  • 28:46 - 28:49
  • 28:49 - 28:53
    STUDENT: Yeah, this
    is the n equals 0.
  • 28:53 - 28:54
    MAGDALENA TODA: Oh,
    yeah, that's the one
  • 28:54 - 28:59
    where it's not a because
    that's not conservative.
  • 28:59 - 29:00
    So what do you get.
  • 29:00 - 29:05
    You get 2xy minus x, right?
  • 29:05 - 29:07
    But I don't know how to
    write it better than that.
  • 29:07 - 29:08
    Well, it doesn't matter.
  • 29:08 - 29:10
    Leave it like that.
  • 29:10 - 29:18
    So this would be 0 if it only
    if x would be 0, but otherwise y
  • 29:18 - 29:19
    was 1/2.
  • 29:19 - 29:23
    But in general, it
    is not a 0, good.
  • 29:23 - 29:30
    So F is not
    conservative, and then we
  • 29:30 - 29:32
    can say goodbye
    to the whole thing
  • 29:32 - 29:40
    here and move on to
    computing the works.
  • 29:40 - 29:42
    What is the only
    way we can do that?
  • 29:42 - 29:46
    By parameterizing
    the first path,
  • 29:46 - 29:49
    but I didn't say which
    one is the first path.
  • 29:49 - 29:53
    This is the first path, so
    x of t equals t, and y of t
  • 29:53 - 29:55
    equals t is your
    parameterization.
  • 29:55 - 30:04
    The simplest one, and then
    W1 will be integral of-- I'm
  • 30:04 - 30:10
    too lazy to write down x of t,
    y of t, but this is what it is.
  • 30:10 - 30:15
    Times x prime of
    t plus x squared
  • 30:15 - 30:22
    y times y prime of t dt where--
  • 30:22 - 30:31
    STUDENT: Isn't that just
    xy dx y-- never mind.
  • 30:31 - 30:34
    MAGDALENA TODA: This is F2.
  • 30:34 - 30:37
    And this is x prime,
    and this is y prime
  • 30:37 - 30:40
    because this thing is
    just-- I have no idea.
  • 30:40 - 30:42
    STUDENT: Right,
    but what I'm asking
  • 30:42 - 30:47
    is that not the same as just
    F1 dx because we're going
  • 30:47 - 30:50
    to do a chain rule anyway.
  • 30:50 - 30:54
    MAGDALENA TODA: If I put
    the x, I cannot put this.
  • 30:54 - 30:57
    OK, this times that is dx.
  • 30:57 - 31:00
    This guy times this guy is dx.
  • 31:00 - 31:01
    STUDENT: But then
    you can't use your
  • 31:01 - 31:04
    MAGDALENA TODA: Then I
    cannot use the t's then.
  • 31:04 - 31:06
    STUDENT: All right, there we go.
  • 31:06 - 31:11
    MAGDALENA TODA: All right, so
    I have integral from 0 to 1 t,
  • 31:11 - 31:15
    t times 1 t squared.
  • 31:15 - 31:18
    If I make a mistake, that would
    be a silly algebra mistake
  • 31:18 - 31:19
    [INAUDIBLE].
  • 31:19 - 31:22
  • 31:22 - 31:24
    All right, class.
  • 31:24 - 31:34
    t cubed times 1dt,
    how much is this?
  • 31:34 - 31:38
    t cubed over 3 plus t
    to the fourth over 4.
  • 31:38 - 31:39
    STUDENT: It's just 2-- oh, no.
  • 31:39 - 31:45
  • 31:45 - 31:48
    MAGDALENA TODA: Very good.
  • 31:48 - 31:52
    Do not expect that we kill you
    with computations on the exams,
  • 31:52 - 31:55
    but that's not what we want.
  • 31:55 - 31:58
    We want to test if you have
    the basic understanding of what
  • 31:58 - 32:03
    this is all about, not to
    kill you with, OK, that.
  • 32:03 - 32:05
    I'm not going to say that
    in front of the cameras,
  • 32:05 - 32:07
    but everybody knows that.
  • 32:07 - 32:08
    There are professors
    who would like
  • 32:08 - 32:10
    to kill you with computations.
  • 32:10 - 32:12
    Now, we're living in
    a different world.
  • 32:12 - 32:16
    If I gave you a long
    polynomial sausage here
  • 32:16 - 32:18
    and I ask you to
    work with it, that
  • 32:18 - 32:21
    doesn't mean that I'm smart
    because MATLAB can do it.
  • 32:21 - 32:25
    Mathematica, you get some
    very nice simplifications
  • 32:25 - 32:28
    over there, so I'm
    just trying to see
  • 32:28 - 32:36
    if rather than being able
    to compute with no error,
  • 32:36 - 32:41
    you are having the basic
    understanding of the concept.
  • 32:41 - 32:45
    And the rest can been done
    by the mathematical software,
  • 32:45 - 32:50
    which, nowadays, most
    mathematicians are using.
  • 32:50 - 32:53
    If you asked me 15
    years ago, I think
  • 32:53 - 32:58
    I knew colleagues at all the
    ranks in academia who would not
  • 32:58 - 33:02
    touch Mathematica or
    MATLAB or Maple say
  • 33:02 - 33:05
    that's like tool from
    evil or something,
  • 33:05 - 33:08
    but now everybody uses.
  • 33:08 - 33:11
    Engineers use mostly
    MATLAB as I told you.
  • 33:11 - 33:16
    Mathematicians use both
    MATLAB and Mathematica.
  • 33:16 - 33:19
    Some of them use Maple,
    especially the ones who
  • 33:19 - 33:23
    have demos for K-12
    level teachers,
  • 33:23 - 33:26
    but MATLAB is a wonderful
    tool, very pretty powerful
  • 33:26 - 33:28
    in many ways.
  • 33:28 - 33:31
    If you are doing any kind
    of linear algebra project--
  • 33:31 - 33:34
    I noticed three or four of you
    are taking linear algebra-- you
  • 33:34 - 33:39
    can always rely on MATLAB being
    the best of all of the above.
  • 33:39 - 33:40
    OK, W2.
  • 33:40 - 33:43
  • 33:43 - 33:50
    For W2, I have a parabola, and
    it's, again, a piece of cake.
  • 33:50 - 33:55
    X prime will be 1,
    y prime will be 2t.
  • 33:55 - 33:56
    When I write down
    the whole thing,
  • 33:56 - 33:59
    I have to pay a little
    bit of attention
  • 33:59 - 34:02
    when I substitute
    especially when I'm
  • 34:02 - 34:05
    taking an exam under pressure.
  • 34:05 - 34:09
  • 34:09 - 34:14
    x squared is t
    squared, y is t squared
  • 34:14 - 34:17
    times y prime, which is 2t.
  • 34:17 - 34:20
    So now this is x prime.
  • 34:20 - 34:21
    This is y prime.
  • 34:21 - 34:25
    Let me change colors.
  • 34:25 - 34:27
    All politicians change colors.
  • 34:27 - 34:29
    But I'm not a
    politician, but I'm
  • 34:29 - 34:34
    thinking it's useful for you
    to see who everybody was.
  • 34:34 - 34:39
    This is the F1 in terms of t.
  • 34:39 - 34:46
    That's the idea of what that
    is, and this is F2 in terms of t
  • 34:46 - 34:48
    as well.
  • 34:48 - 34:50
    Oh, my God, another answer?
  • 34:50 - 34:54
    Absolutely, I'm going to
    get an another answer.
  • 34:54 - 34:57
    Is it obviously to everybody
    I'm going to get another answer?
  • 34:57 - 34:58
    STUDENT: Yeah.
  • 34:58 - 35:01
    MAGDALENA TODA: So I don't
    have to put the t's here,
  • 35:01 - 35:04
    but I thought it was
    sort of neat to see
  • 35:04 - 35:06
    that t goes from 0 to 1.
  • 35:06 - 35:09
    And what do I get?
  • 35:09 - 35:16
    This whole lot of them is t
    cubed plus 2 t to the fifth.
  • 35:16 - 35:19
  • 35:19 - 35:26
    So when I do the integration,
    I get t to the 4 over 4 plus--
  • 35:26 - 35:27
    shut up, Magdalena, get people--
  • 35:27 - 35:30
  • 35:30 - 35:31
    STUDENT: [INAUDIBLE].
  • 35:31 - 35:32
    MAGDALENA TODA: Very good.
  • 35:32 - 35:36
    Yeah, he's done
    the simplification.
  • 35:36 - 35:38
    STUDENT: You get
    the same values.
  • 35:38 - 35:40
  • 35:40 - 35:45
    Plug in 1, you get 7/12 again.
  • 35:45 - 35:48
    MAGDALENA TODA: So I'm
    asking you-- OK, what was it?
  • 35:48 - 35:57
    Solve 0, 1-- so I'm
    asking why do you
  • 35:57 - 36:01
    think we get the same value?
  • 36:01 - 36:03
    Because the force
    is not conservative,
  • 36:03 - 36:07
    and I went on another path.
  • 36:07 - 36:10
    I went on one path, and
    I went on another path.
  • 36:10 - 36:16
    And look, obviously my
    expression was different.
  • 36:16 - 36:19
    It's like one of those
    math games or UIL games.
  • 36:19 - 36:21
    And look at the algebra.
  • 36:21 - 36:24
    The polynomials are different.
  • 36:24 - 36:26
    What was my luck here?
  • 36:26 - 36:27
    I took 1.
  • 36:27 - 36:28
    STUDENT: Yeah.
  • 36:28 - 36:29
    MAGDALENA TODA: I
    could have taken 2.
  • 36:29 - 36:36
    So if instead of 1, I would
    have taken another number,
  • 36:36 - 36:38
    then the higher the power,
    the bigger the number
  • 36:38 - 36:39
    would have been.
  • 36:39 - 36:40
    I could have taken 2--
  • 36:40 - 36:42
    STUDENT: You could
    have taken negative 1,
  • 36:42 - 36:44
    and you still wouldn't
    have got the same answer.
  • 36:44 - 36:49
    MAGDALENA TODA: Yeah, there
    are many reasons why that is.
  • 36:49 - 36:54
    But anyway, know that when you
    take 1, 1 to every power is 1.
  • 36:54 - 36:55
    And yeah, you were lucky.
  • 36:55 - 36:58
    But in general, keep in
    mind that if the force is
  • 36:58 - 37:02
    conservative, in
    general, in most examples
  • 37:02 - 37:05
    you're not going to get the
    same answer for the work
  • 37:05 - 37:11
    because it does depend on
    the path you want to take.
  • 37:11 - 37:18
    I think I have reviewed quite
    everything that I wanted.
  • 37:18 - 37:27
  • 37:27 - 37:30
    So I should be ready
    to move forward.
  • 37:30 - 37:33
  • 37:33 - 37:42
    So I'm saying we are done
    with sections 13.1, 13.2,
  • 37:42 - 37:49
    and 13.3, which was my
    favorite because it's not
  • 37:49 - 37:51
    just the integral of
    the path that I like,
  • 37:51 - 37:55
    but it's the so-called
    fundamental theorem of calculus
  • 37:55 - 38:05
    3, which says, fundamental
    theorem of the path integral
  • 38:05 - 38:12
    saying that you have f of the
    endpoint minus f of the origin,
  • 38:12 - 38:14
    where little f is
    that scalar potential
  • 38:14 - 38:17
    as the linear function
    was concerned.
  • 38:17 - 38:24
    I'm going to call it the
    fundamental theorem of path
  • 38:24 - 38:26
    integral.
  • 38:26 - 38:29
    Last time I told you the
    fundamental theorem of calculus
  • 38:29 - 38:32
    is Federal Trade Commission.
  • 38:32 - 38:35
    We refer to that in Calc 1.
  • 38:35 - 38:39
    But this one is the fundamental
    theorem of path integral.
  • 38:39 - 38:43
    Remember it because at
    least one problem out of 15
  • 38:43 - 38:45
    or something on the
    final, and there are not
  • 38:45 - 38:46
    going to be very many.
  • 38:46 - 38:49
    It's going to ask you to
    know that result. This is
  • 38:49 - 38:52
    an important theorem.
  • 38:52 - 38:56
    And another important theorem
    that is starting right now
  • 38:56 - 38:58
    is Green's theorem.
  • 38:58 - 39:03
    Green's theorem is
    a magic result. I
  • 39:03 - 39:05
    have a t-shirt with it.
  • 39:05 - 39:06
    I didn't bring it today.
  • 39:06 - 39:08
    Maybe I'm going to bring
    it next time First,
  • 39:08 - 39:12
    I want you to see
    the result, and then
  • 39:12 - 39:15
    I'll bring the t-shirt
    to the exam, so OK.
  • 39:15 - 39:18
  • 39:18 - 39:25
    Assume that you have a
    soup called Jordan curve.
  • 39:25 - 39:28
  • 39:28 - 39:32
    You see, mathematicians don't
    follow mathematical objects
  • 39:32 - 39:34
    by their names.
  • 39:34 - 39:37
    We are crazy people, but
    we don't have a big ego.
  • 39:37 - 39:42
    We would not say a theorem
    of myself or whatever.
  • 39:42 - 39:45
    We never give our names to that.
  • 39:45 - 39:51
    But all through calculus you
    saw all sorts of results.
  • 39:51 - 39:57
    Like you see the Jordan
    curve is a terminology,
  • 39:57 - 40:00
    but then you see
    everywhere the Linus rule.
  • 40:00 - 40:02
    Did Linus get to
    call it his own rule?
  • 40:02 - 40:06
    No, but Euler's
    number, these are
  • 40:06 - 40:09
    things that were
    discovered, and in honor
  • 40:09 - 40:12
    of that particular
    mathematician,
  • 40:12 - 40:13
    we call them names.
  • 40:13 - 40:16
    We call them the name
    of the mathematician.
  • 40:16 - 40:18
  • 40:18 - 40:23
    Out of curiosity for
    0.5 extra credit points,
  • 40:23 - 40:25
    find out who Jordan was.
  • 40:25 - 40:33
    Jordan curve is a closed
    curve that, in general,
  • 40:33 - 40:35
    could be piecewise continuous.
  • 40:35 - 40:41
  • 40:41 - 40:43
    So you have a closed
    loop over here.
  • 40:43 - 40:50
    So in general, I could
    have something like that
  • 40:50 - 40:54
    that does not enclose.
  • 40:54 - 40:57
    That encloses a
    domain without holes.
  • 40:57 - 41:04
  • 41:04 - 41:08
    Holes are functions
    of the same thing.
  • 41:08 - 41:10
    STUDENT: So doesn't it
    need to be continuous?
  • 41:10 - 41:12
    MAGDALENA TODA:
    No, I said it is.
  • 41:12 - 41:14
    STUDENT: You said, piecewise.
  • 41:14 - 41:15
    MAGDALENA TODA: Ah, piecewise.
  • 41:15 - 41:16
    This is piecewise.
  • 41:16 - 41:18
    STUDENT: Oh, so it's piecewise.
  • 41:18 - 41:18
    OK.
  • 41:18 - 41:20
    MAGDALENA TODA: So you
    have a bunch of arcs.
  • 41:20 - 41:23
    Finitely many, let's
    say, in your case.
  • 41:23 - 41:26
    Finitely many arcs,
    they have corners,
  • 41:26 - 41:30
    but you can see define the
    integral along such a path.
  • 41:30 - 41:34
  • 41:34 - 41:38
    Oh, and also for another
    0.5 extra credit,
  • 41:38 - 41:40
    find out who Mr.
    Green was because he
  • 41:40 - 41:43
    has several theorems that
    are through mathematics
  • 41:43 - 41:46
    and free mechanics and
    variation calculus.
  • 41:46 - 41:51
    There are several identities
    that are called Greens.
  • 41:51 - 41:52
    There is this famous
    Green's theorem,
  • 41:52 - 41:55
    but there are Green's
    first identity,
  • 41:55 - 41:58
    Green's second identity,
    and all sorts of things.
  • 41:58 - 42:02
    And find out who Mr.
    Green was, and as a total,
  • 42:02 - 42:04
    you have 1 point extra credit.
  • 42:04 - 42:09
    And you can turn in a regular
    essay like a two-page thing.
  • 42:09 - 42:13
    You want biography of these
    mathematicians if you want,
  • 42:13 - 42:16
    just a few paragraphs.
  • 42:16 - 42:19
    So what does Green's theorem do?
  • 42:19 - 42:26
    Green's theorem is
    a remarkable result
  • 42:26 - 42:31
    which links the path integral
    to the double integral.
  • 42:31 - 42:38
    It's a remarkable
    and famous result.
  • 42:38 - 42:48
    And that links the path
    integral on the closed
  • 42:48 - 43:07
    curve to a double integral
    over the domain enclosed.
  • 43:07 - 43:10
    I can see the domain
    inside, but you
  • 43:10 - 43:15
    have to understand it's
    enclosed by the curve.
  • 43:15 - 43:21
  • 43:21 - 43:24
    All right, and assume
    that you have--
  • 43:24 - 43:36
    M and N are C1 functions of
    x and y, what does it mean?
  • 43:36 - 43:38
    M is a function of xy.
  • 43:38 - 43:40
    N is a function of xy in plane.
  • 43:40 - 43:43
    Both of them are differentiable
    with continuous derivative.
  • 43:43 - 43:47
  • 43:47 - 43:48
    They are differentiable.
  • 43:48 - 43:50
    You can take the
    partial derivatives,
  • 43:50 - 43:52
    and all the partial
    derivatives are continuous.
  • 43:52 - 43:55
    That's what we mean
    by being C1 functions.
  • 43:55 - 43:59
    And there the magic
    happens, so let me show you
  • 43:59 - 44:02
    where the magic happens.
  • 44:02 - 44:06
    This in the box,
    the path integral
  • 44:06 - 44:21
    over c of M dx plus Ndy is
    equal to the double integral
  • 44:21 - 44:22
    over the domain enclosed.
  • 44:22 - 44:24
    OK, this is the c.
  • 44:24 - 44:27
    On the boundary you
    go counterclockwise
  • 44:27 - 44:29
    like any respectable
    mathematician
  • 44:29 - 44:34
    would go in a trigonometric
    sense, just counterclockwise.
  • 44:34 - 44:37
    And this is the domain
    being closed by c.
  • 44:37 - 44:40
  • 44:40 - 44:44
    And you put here the
    integral, which is magic.
  • 44:44 - 44:46
    This is easy to
    remember for you.
  • 44:46 - 44:48
    This is not easy to
    remember unless I
  • 44:48 - 44:50
    take the t-shirt to
    the exam, and you
  • 44:50 - 44:52
    cheat by looking at my t-shirt.
  • 44:52 - 44:55
    No, by the time of the
    exam, I promised you
  • 44:55 - 44:59
    you are going to have at least
    one week, seven days or more,
  • 44:59 - 45:03
    10-day period in which
    we will study samples,
  • 45:03 - 45:06
    various samples of old finals.
  • 45:06 - 45:08
    I'm going to go ahead and
    send you some by email.
  • 45:08 - 45:11
    Do you mind?
  • 45:11 - 45:14
    In the next week
    after this week, we
  • 45:14 - 45:15
    are going to start reviewing.
  • 45:15 - 45:20
    And by dA I mean dxdy, the
    usual area limit in Cartesian
  • 45:20 - 45:24
    coordinates the way you
    are used to it the most.
  • 45:24 - 45:27
  • 45:27 - 45:30
    And then, Alex is looking
    at it and said, well,
  • 45:30 - 45:32
    then I tell her that
    the most elegant way
  • 45:32 - 45:35
    is to put it with dxdy.
  • 45:35 - 45:38
    This is what we call a
    one form in mathematics.
  • 45:38 - 45:40
    What is a one form.
  • 45:40 - 45:44
    It is a linear combination of
    this infinitesimal elements
  • 45:44 - 45:47
    dxdy in plane with some
    scalar functions of x
  • 45:47 - 45:49
    and y in front of her.
  • 45:49 - 45:51
    OK, so what do we do?
  • 45:51 - 45:53
    We integrate the one form.
  • 45:53 - 45:57
    The book doesn't talk about one
    forms because the is actually
  • 45:57 - 46:01
    written for the average
    student, the average freshman
  • 46:01 - 46:05
    or the average
    sophomore, but I think
  • 46:05 - 46:08
    we have an exposure to
    the notion of one form,
  • 46:08 - 46:11
    so I can get a little bit
    more elegant and more rigorous
  • 46:11 - 46:12
    in my speech.
  • 46:12 - 46:16
    If you are a graduate
    student, you most likely
  • 46:16 - 46:18
    would know this is a one form.
  • 46:18 - 46:22
    That's actually the
    definition of a one form.
  • 46:22 - 46:23
    And you'll say, what is this?
  • 46:23 - 46:27
    This is actually two
    form, but you are
  • 46:27 - 46:28
    going to say, wait a minute.
  • 46:28 - 46:31
    I have a scalar
    function, whatever
  • 46:31 - 46:34
    that is, from the integration
    in front of the dxdy
  • 46:34 - 46:40
    you want but you never said
    that dxdy is a two form.
  • 46:40 - 46:45
    Actually, I did, and I
    didn't call it a two form.
  • 46:45 - 46:47
    Do you remember that
    I introduced to you
  • 46:47 - 46:50
    some magic wedge product?
  • 46:50 - 46:54
  • 46:54 - 46:58
    And we said, this is
    a tiny displacement.
  • 46:58 - 47:00
    Dx infinitesimal is small.
  • 47:00 - 47:02
    Imagine how much the
    video we'll there
  • 47:02 - 47:05
    is an infinitesimal
    displacement dx
  • 47:05 - 47:08
    and an infinitesimal
    displacement dy,
  • 47:08 - 47:11
    and you have some
    sort of a sign area.
  • 47:11 - 47:15
    So we said, we don't
    just take dxdy,
  • 47:15 - 47:19
    but we take a product
    between dxdy with a wedge,
  • 47:19 - 47:22
    meaning that if I
    change the order,
  • 47:22 - 47:24
    I'm going to have minus dy here.
  • 47:24 - 47:29
    This is typical exterior
    derivative theory-- exterior
  • 47:29 - 47:31
    derivative theory.
  • 47:31 - 47:35
    And it's a theory that
    starts more or less
  • 47:35 - 47:36
    at the graduate level.
  • 47:36 - 47:40
    And many people get their
    master's degree in math
  • 47:40 - 47:43
    and never get to see it, and
    I pity them, but this life.
  • 47:43 - 47:47
    On the other hand, when
    you have dx, which dx--
  • 47:47 - 47:51
    the area between dx and dx is 0.
  • 47:51 - 47:53
    So we're all very happy
    I get rid of those.
  • 47:53 - 47:56
    When I have the sign
    between the displacement,
  • 47:56 - 47:58
    dy and itself is 0.
  • 47:58 - 48:00
    So these are the
    basic properties
  • 48:00 - 48:05
    that we started
    about the sign area.
  • 48:05 - 48:08
    I want to show you what happens.
  • 48:08 - 48:16
    I'm going to-- yeah,
    I'm going to erase here.
  • 48:16 - 48:23
  • 48:23 - 48:26
    I'm going to show
    you later I'm going
  • 48:26 - 48:33
    to prove this theorem to you
    later using these tricks that I
  • 48:33 - 48:35
    just showed you here.
  • 48:35 - 48:54
    I will provide proof
    to this formula, OK?
  • 48:54 - 48:58
    And let's take a look at
    that, and we say, well,
  • 48:58 - 49:00
    can I memorize that by
    the time of the final?
  • 49:00 - 49:02
    Yes, you can.
  • 49:02 - 49:13
    What is beautiful about
    this, it can actually
  • 49:13 - 49:19
    help you solve problems that you
    didn't think would be possible.
  • 49:19 - 49:21
    For example, example
    1, and I say,
  • 49:21 - 49:26
    that would be one of
    the most basic ones.
  • 49:26 - 49:39
    Find the geometric meaning of
    the integral over a c where
  • 49:39 - 49:40
    c is a closed loop.
  • 49:40 - 49:42
    OK, c is a loop.
  • 49:42 - 49:47
    Piecewise define Jordan
    curve-- Jordan curve.
  • 49:47 - 49:50
    And I integrate out
    of something weird.
  • 49:50 - 49:51
    And you say, oh, my God.
  • 49:51 - 49:52
    Look at her.
  • 49:52 - 49:59
    She picked some weird function
    where the path from the dx
  • 49:59 - 50:06
    is M, and the path in front of
    dy is N, the M and N functions.
  • 50:06 - 50:08
    Why would pick like that?
  • 50:08 - 50:11
    You wouldn't know yet, but
    if you apply Green's theorem,
  • 50:11 - 50:14
    assuming you believe
    it's true, you
  • 50:14 - 50:18
    have double integral over the
    domain enclosed by this loop.
  • 50:18 - 50:25
    The loop is enclosing
    this domain of what?
  • 50:25 - 50:32
    Now, I'm trying to shut up,
    and I'm want you to talk.
  • 50:32 - 50:36
    What am I going to
    write over here?
  • 50:36 - 50:37
    STUDENT: 1 plus 1.
  • 50:37 - 50:41
    MAGDALENA TODA: 1 plus
    1, how fun is that?
  • 50:41 - 50:46
    Y minus 1, 1 plus 1 equals
    2 last time I checked,
  • 50:46 - 50:49
    and this is dA.
  • 50:49 - 50:53
    And what do you think
    this animal would be?
  • 50:53 - 50:56
    The cast of 2 always can escape.
  • 50:56 - 51:01
    So if we don't want
    it, just kick it out.
  • 51:01 - 51:04
    What is the remaining
    double integral for d of DA?
  • 51:04 - 51:07
    You have seen this guy all
    through the Calculus 3 course.
  • 51:07 - 51:10
    You're tired of it.
  • 51:10 - 51:14
    You said, I cannot wait for
    this semester to be over
  • 51:14 - 51:19
    because this is the double
    integral of 1dA over d.
  • 51:19 - 51:22
    What in the world is that?
  • 51:22 - 51:24
    That is the--
  • 51:24 - 51:25
    STUDENT: --area.
  • 51:25 - 51:27
    MAGDALENA TODA: Area, very good.
  • 51:27 - 51:31
    This is the area of the
    domain d inside the curve.
  • 51:31 - 51:35
    The shaded area is this.
  • 51:35 - 51:39
    So you have discovered
    something beautiful
  • 51:39 - 51:47
    that the area of the domain
    enclosed by a Jordan curve
  • 51:47 - 51:51
    equals 1/2 because you pull
    the two out in front here,
  • 51:51 - 51:56
    it's going to be 1/2 of the path
    integrals over the boundary.
  • 51:56 - 51:59
    This is called
    boundary of a domain.
  • 51:59 - 52:00
    c is the boundary of the domain.
  • 52:00 - 52:05
  • 52:05 - 52:07
    Some mathematicians--
    I don't know
  • 52:07 - 52:11
    how far you want to go with your
    education, but in a few years
  • 52:11 - 52:13
    you might become
    graduate students.
  • 52:13 - 52:19
    And even some engineers use this
    notation boundary of d, del d.
  • 52:19 - 52:22
    That means the boundaries,
    the frontier of a domain.
  • 52:22 - 52:24
    The fence of a ranch.
  • 52:24 - 52:27
    That is the del d, but
    don't tell the rancher
  • 52:27 - 52:31
    because he will take his gun
    out and shoot you thinking
  • 52:31 - 52:34
    that you are off the hook or
    you are after something weird.
  • 52:34 - 52:38
    So that's the boundary
    of the domain.
  • 52:38 - 52:42
    And then you have
    minus ydx plus xdy.
  • 52:42 - 52:46
  • 52:46 - 52:48
    MAGDALENA TODA: We discover
    something beautiful.
  • 52:48 - 52:50
    Something important.
  • 52:50 - 52:53
    And now I'm asking,
    with this exercise--
  • 52:53 - 52:59
    one which I could even--
    I could even call a lemma.
  • 52:59 - 53:04
    Lemma is not quite a
    theorem, because it's based--
  • 53:04 - 53:05
    could be based on a theorem.
  • 53:05 - 53:09
    It's a little result that can
    be proved in just a few lines
  • 53:09 - 53:12
    without being something
    sophisticated based
  • 53:12 - 53:16
    on something you
    knew from before.
  • 53:16 - 53:20
    So this is called a lemma.
  • 53:20 - 53:26
    When you have a sophisticated
    area to compute--
  • 53:26 - 53:30
    or even can you prove-- if you
    believe in Green's theorem,
  • 53:30 - 53:33
    can you prove that the
    area inside the circle
  • 53:33 - 53:35
    is pi r squared?
  • 53:35 - 53:40
    Can you prove that the
    area inside of an ellipse
  • 53:40 - 53:41
    is-- I don't know what.
  • 53:41 - 53:44
    Do you know the area
    inside of an ellipse?
  • 53:44 - 53:48
    Nobody taught me in school.
  • 53:48 - 53:51
    I don't know why
    it's so beautiful.
  • 53:51 - 53:55
    I learned what an ellipse
    was in eleventh grade
  • 53:55 - 53:59
    in high school and again
    a review as a freshman
  • 53:59 - 54:01
    analytic geometry.
  • 54:01 - 54:03
    So we've seen conics again--
  • 54:03 - 54:05
    STUDENT: I think we did
    conics in 10th grade.
  • 54:05 - 54:07
    We might have seen it.
  • 54:07 - 54:08
    MAGDALENA TODA:
    But nobody told me
  • 54:08 - 54:10
    like-- I give you an ellipse.
  • 54:10 - 54:12
    Compute the area inside.
  • 54:12 - 54:13
    I had no idea.
  • 54:13 - 54:15
    And I didn't know
    the formula until I
  • 54:15 - 54:18
    became an assistant professor.
  • 54:18 - 54:19
    I was already in my thirties.
  • 54:19 - 54:24
    That's a shame to see that
    thing for the first time OK.
  • 54:24 - 54:28
    So let's see if we believe
    this lemma, and the Green's
  • 54:28 - 54:29
    theorem of course.
  • 54:29 - 54:32
    But let's apply the
    lemma, primarily
  • 54:32 - 54:33
    from the Green's theorem.
  • 54:33 - 54:37
    Can we actually prove
    that the area of the disk
  • 54:37 - 54:41
    is pi r squared and the
    area of the ellipse--
  • 54:41 - 54:43
    inside the ellipse
    will be god knows what.
  • 54:43 - 54:47
    And we will discover
    that by ourselves.
  • 54:47 - 54:49
    I think that's the
    beauty of mathematics.
  • 54:49 - 54:54
    Because every now and then
    even if you discover things
  • 54:54 - 54:56
    that people have known
    for hundreds of years,
  • 54:56 - 54:58
    it still gives you
    the satisfaction
  • 54:58 - 55:02
    that you did something by
    yourself-- all on yourself.
  • 55:02 - 55:06
    Like, when you feel
    build a helicopter or you
  • 55:06 - 55:08
    build a table.
  • 55:08 - 55:10
    There are many more
    beautiful tables
  • 55:10 - 55:12
    that were built before
    you, but still it's
  • 55:12 - 55:15
    a lot of satisfaction that
    you do all by yourself.
  • 55:15 - 55:17
    It's the same with mathematics.
  • 55:17 - 55:23
    So let's see what we can
    do now for the first time.
  • 55:23 - 55:25
    Not for the first time.
  • 55:25 - 55:28
    We do it in other ways.
  • 55:28 - 55:38
    Can you prove using the lemma
    or Green's theorem-- which
  • 55:38 - 55:43
    is the same thing-- either
    one-- that the area of the disk
  • 55:43 - 55:48
    of radius r-- this is the r.
  • 55:48 - 55:52
    so this the radius
    r is pi r squared.
  • 55:52 - 55:56
  • 55:56 - 55:58
    I hope so.
  • 55:58 - 56:00
    And the answer is, I hope so.
  • 56:00 - 56:01
    And that's all.
  • 56:01 - 56:04
  • 56:04 - 56:09
    Area of the disk of radius r.
  • 56:09 - 56:10
    Oh my god.
  • 56:10 - 56:13
    So you go, well.
  • 56:13 - 56:19
    If I knew the parameterization
    of that boundary C,
  • 56:19 - 56:21
    it would be a piece of cake.
  • 56:21 - 56:26
    Because I would just-- I know
    how to do a path integral now.
  • 56:26 - 56:28
    I've learned in the
    previous sections,
  • 56:28 - 56:30
    so this should be easy.
  • 56:30 - 56:33
    Can we do that?
  • 56:33 - 56:33
    So let's see.
  • 56:33 - 56:36
  • 56:36 - 56:38
    Without computing
    the double integral,
  • 56:38 - 56:41
    because I can always do
    that with polar coordinates.
  • 56:41 - 56:43
    And we are going to do that.
  • 56:43 - 56:48
  • 56:48 - 56:50
    Let's do that as
    well, as practice.
  • 56:50 - 56:54
    Because so you
    review for the exam.
  • 56:54 - 56:57
  • 56:57 - 57:01
    But another way to
    do it would be what?
  • 57:01 - 57:07
    1/2 integral over the circle.
  • 57:07 - 57:14
    And how do I parametrize a
    circle of fixed radius r?
  • 57:14 - 57:15
    Who tells me?
  • 57:15 - 57:18
    x of t will be--
    that was Chapter 10.
  • 57:18 - 57:21
    Everything is a
    circle in mathematics.
  • 57:21 - 57:22
    STUDENT: r cosine t.
  • 57:22 - 57:23
    MAGDALENA TODA: r cosine t.
  • 57:23 - 57:24
    Excellent.
  • 57:24 - 57:26
    y of t is?
  • 57:26 - 57:27
    STUDENT: r sine t.
  • 57:27 - 57:29
    MAGDALENA TODA: r sine t.
  • 57:29 - 57:32
    So, finally I'm going to
    go ahead and use this one.
  • 57:32 - 57:37
    And I'm going to say, well,
    minus y to be plugged in.
  • 57:37 - 57:40
  • 57:40 - 57:43
    This is minus y.
  • 57:43 - 57:45
    Multiply by dx.
  • 57:45 - 57:48
    Well, you say, wait a
    minute. dx with respect.
  • 57:48 - 57:49
    What is dx?
  • 57:49 - 57:52
    dx is just x prime dt.
  • 57:52 - 57:55
    Dy is just y prime dt.
  • 57:55 - 57:56
    And t goes out.
  • 57:56 - 57:58
    It's banished.
  • 57:58 - 58:00
    No, he's the most important guy.
  • 58:00 - 58:03
    So t goes from something
    to something else.
  • 58:03 - 58:05
    We will see that later.
  • 58:05 - 58:07
    What is x prime dt?
  • 58:07 - 58:13
    X prime is minus r sine
    theta-- sine t, Magdalena.
  • 58:13 - 58:16
    Minus r sine t.
  • 58:16 - 58:18
    That was x prime.
  • 58:18 - 58:19
    Change the color.
  • 58:19 - 58:23
    Give people some
    variation in their life.
  • 58:23 - 58:32
    Plus r cosine t,
    because this x--
  • 58:32 - 58:33
    STUDENT: [INAUDIBLE].
  • 58:33 - 58:39
  • 58:39 - 58:46
    MAGDALENA TODA: --times
    the y, which is r cosine t.
  • 58:46 - 58:49
    So it suddenly became beautiful.
  • 58:49 - 58:52
    It looks-- first it looks ugly,
    but now it became beautiful.
  • 58:52 - 58:53
    Why?
  • 58:53 - 58:54
    How come it became beautiful?
  • 58:54 - 58:57
    STUDENT: Because you got sine
    squared plus cosine square.
  • 58:57 - 58:58
    MAGDALENA TODA:
    Because I got a plus.
  • 58:58 - 59:02
    If you pay attention, plus sine
    squared plus cosine squared.
  • 59:02 - 59:05
    So I have, what is sine
    squared plus cosine squared?
  • 59:05 - 59:08
    I heard that our
    students in trig--
  • 59:08 - 59:12
    Poly told me-- who still don't
    know that this is the most
  • 59:12 - 59:14
    important thing you
    learn in trigonometry--
  • 59:14 - 59:15
    is Pythagorean theorem.
  • 59:15 - 59:16
    Right?
  • 59:16 - 59:24
    So you have 1/2 integral
  • 59:24 - 59:27
    STUDENT: r squared--
  • 59:27 - 59:28
    MAGDALENA TODA:
    r-- no, I'm lazy.
  • 59:28 - 59:31
    I'm going slow-- r.
  • 59:31 - 59:33
    dt.
  • 59:33 - 59:35
    T from what to what?
  • 59:35 - 59:37
    From 0 times 0.
  • 59:37 - 59:40
    I'm starting whatever
    I want, actually.
  • 59:40 - 59:44
    I go counterclockwise
    I'm into pi.
  • 59:44 - 59:46
    STUDENT: Why is
    that not r squared?
  • 59:46 - 59:48
    It should be r squared.
  • 59:48 - 59:49
    MAGDALENA TODA: I'm sorry, guys.
  • 59:49 - 59:50
    I'm sorry.
  • 59:50 - 59:54
    I don't know what
    I am-- r squared.
  • 59:54 - 59:57
    1/2 r squared times 2 pi.
  • 59:57 - 60:01
  • 60:01 - 60:03
    So we have pi r squared.
  • 60:03 - 60:07
    And if you did not
    tell me it's r squared,
  • 60:07 - 60:10
    we wouldn't have
    gotten the answer.
  • 60:10 - 60:10
    That's good.
  • 60:10 - 60:14
  • 60:14 - 60:16
    What's the other way to do it?
  • 60:16 - 60:19
    If a problem on
    the final would ask
  • 60:19 - 60:22
    you prove in two different
    ways that the rubber
  • 60:22 - 60:25
    disk is pi r squared using
    Calc 3, or whatever--
  • 60:25 - 60:26
    STUDENT: Would require--
  • 60:26 - 60:28
    MAGDALENA TODA: The
    double integral, right?
  • 60:28 - 60:29
    Right?
  • 60:29 - 60:31
    STUDENT: Could have done
    Cartesian coordinates as well.
  • 60:31 - 60:33
    If that counts as a second way.
  • 60:33 - 60:34
    MAGDALENA TODA: Yeah.
  • 60:34 - 60:35
    You can-- OK.
  • 60:35 - 60:36
    What could this be?
  • 60:36 - 60:37
    Oh my god.
  • 60:37 - 60:42
    This would be minus 1
    to 1 minus square root
  • 60:42 - 60:46
    1 minus x squared to square
    root 1 minus x squared.
  • 60:46 - 60:47
    Am i right guys?
  • 60:47 - 60:47
    STUDENT: Yep.
  • 60:47 - 60:49
    MAGDALENA TODA: 1 dy dx.
  • 60:49 - 60:51
    Of course it's a pain.
  • 60:51 - 60:54
    STUDENT: You could double that
    and set the bottoms both equal
  • 60:54 - 60:55
    to 0.
  • 60:55 - 60:56
    MAGDALENA TODA: Right.
  • 60:56 - 61:01
    So we can do by symmetry--
  • 61:01 - 61:03
    STUDENT: Yeah.
  • 61:03 - 61:05
    MAGDALENA TODA: I'm--
    shall I erase or leave it.
  • 61:05 - 61:08
    Are you understand
    what Alex is saying?
  • 61:08 - 61:12
    This is 2i is the integral
    that you will get.
  • 61:12 - 61:14
    STUDENT: Just write
    it next to it--
  • 61:14 - 61:15
    MAGDALENA TODA: I tell
    you four times, you
  • 61:15 - 61:16
    see, Alex, because you have--
  • 61:16 - 61:17
    STUDENT: Oh, yeah.
  • 61:17 - 61:19
    MAGDALENA TODA: --symmetry
    with respect to the x-axis,
  • 61:19 - 61:21
    and symmetry with
    respect to y-axis.
  • 61:21 - 61:27
    And you can take 0
    to 1 and 0 to that.
  • 61:27 - 61:29
    And you have x from 0 to 1.
  • 61:29 - 61:34
    You have y from 0 to stop.
  • 61:34 - 61:35
    Square root of 1 minus x square.
  • 61:35 - 61:37
    Like the strips.
  • 61:37 - 61:42
    And you have 4
    times that A1, which
  • 61:42 - 61:45
    would be the area of
    the first quadratic.
  • 61:45 - 61:46
    You can do that, too.
  • 61:46 - 61:47
    It's easier.
  • 61:47 - 61:50
    But the best way to do that is
    not in Cartesian coordinates.
  • 61:50 - 61:53
    The best way is to do
    it in polar coordinates.
  • 61:53 - 61:57
    Always remember
    your Jacobian is r.
  • 61:57 - 62:01
    So if you have
    Jacobian r-- erase.
  • 62:01 - 62:03
    Let's put r here again.
  • 62:03 - 62:08
    And then dr d theta.
  • 62:08 - 62:10
    But now you say, wait
    a minute, Magdalena.
  • 62:10 - 62:12
    You said r is fixed.
  • 62:12 - 62:12
    Yes.
  • 62:12 - 62:14
    And that's why I
    need to learn Greek,
  • 62:14 - 62:16
    because it's all Greek to me.
  • 62:16 - 62:19
    Instead of r I put
    rho as a variable.
  • 62:19 - 62:24
    And I say, rho is
    between 0 and r.
  • 62:24 - 62:25
    r is fixed.
  • 62:25 - 62:27
    That's my [INAUDIBLE].
  • 62:27 - 62:32
    Big r is not usually written
    as a variable from 0 to some.
  • 62:32 - 62:33
    I cannot use that.
  • 62:33 - 62:37
    So I have to us a Greek letter,
    whether I like it or not.
  • 62:37 - 62:40
    And theta is from 0 to 2 pi.
  • 62:40 - 62:42
    And I still get the same thing.
  • 62:42 - 62:47
    I get r-- rho squared
    over 2 between 0 and r.
  • 62:47 - 62:49
    And I have 2 pi.
  • 62:49 - 62:53
    And in the end that means
    pi r squared, and I'm back.
  • 62:53 - 62:56
    And you say, wait,
    this is Example 4.
  • 62:56 - 62:57
    Whatever example.
  • 62:57 - 62:59
    Is it Example 4, 5?
  • 62:59 - 63:01
    You say, this is
    a piece of cake.
  • 63:01 - 63:06
    I have two methods showing
    me that area of the disk
  • 63:06 - 63:07
    is so pi r squared.
  • 63:07 - 63:08
    It's so trivial.
  • 63:08 - 63:12
    Yeah, then let's move
    on and do the ellipse.
  • 63:12 - 63:15
    Or we could have been
    smart and done the ellipse
  • 63:15 - 63:17
    from the beginning.
  • 63:17 - 63:19
    And then the circular
    disk would have
  • 63:19 - 63:23
    been just a trivial, particular
    example of the ellipse.
  • 63:23 - 63:25
    But let's do the ellipse
    with this magic formula
  • 63:25 - 63:27
    that I just taught you.
  • 63:27 - 63:30
  • 63:30 - 63:34
    In the finals-- I'm going to
    send you a bunch of finals.
  • 63:34 - 63:37
    You're going to be
    amused, because you're
  • 63:37 - 63:38
    going to look at
    them and you say,
  • 63:38 - 63:42
    regardless of the year and
    semester when the final was
  • 63:42 - 63:44
    given for Calc 3,
    there was always
  • 63:44 - 63:49
    one of the problems at the
    end using direct application
  • 63:49 - 63:51
    of Green's theorem.
  • 63:51 - 63:53
    So Green's theorem
    is an obsession,
  • 63:53 - 63:55
    and not only at Tech.
  • 63:55 - 63:59
    I was looking UT Austin,
    A&M, other schools--
  • 63:59 - 64:06
    California Berkley-- all the
    Calc 3 courses on the final
  • 64:06 - 64:11
    have at least one application--
    direct application
  • 64:11 - 64:12
    applying principal.
  • 64:12 - 64:13
    OK.
  • 64:13 - 64:17
  • 64:17 - 64:19
    So what did I say?
  • 64:19 - 64:22
    I said that we have
    to draw an ellipse.
  • 64:22 - 64:25
    How do we draw an ellipse
    without making it up?
  • 64:25 - 64:27
    That's the question.
  • 64:27 - 64:29
    STUDENT: Draw a circle.
  • 64:29 - 64:30
    MAGDALENA TODA: Draw a circle.
  • 64:30 - 64:32
    Good answer.
  • 64:32 - 64:34
    OK.
  • 64:34 - 64:35
    All right.
  • 64:35 - 64:40
    And guys this
    started really bad.
  • 64:40 - 64:43
    So I'm doing what I can.
  • 64:43 - 64:46
  • 64:46 - 64:49
    I should have tried
    more coffee today,
  • 64:49 - 64:52
    because I'm getting
    insecure and very shaky.
  • 64:52 - 64:53
    OK.
  • 64:53 - 64:58
    So I have the ellipse
    in standard form
  • 64:58 - 65:02
    of center O, x squared over
    x squared plus y squared
  • 65:02 - 65:05
    over B squared equals 1.
  • 65:05 - 65:08
    And now you are going to
    me who is A and who is B?
  • 65:08 - 65:09
    What are they called?
  • 65:09 - 65:10
    Semi--
  • 65:10 - 65:11
    STUDENT: Semiotics.
  • 65:11 - 65:12
    MAGDALENA TODA: Semiotics.
  • 65:12 - 65:15
    A and B. Good.
  • 65:15 - 65:19
    Find the area.
  • 65:19 - 65:22
    I don't like-- OK.
  • 65:22 - 65:27
    Let's put B inside, and let's
    put C outside the boundary.
  • 65:27 - 65:43
    So area of the ellipse domain
    D will be-- by the lemma-- 1/2
  • 65:43 - 65:46
    integral over C.
  • 65:46 - 65:47
    This is C. Is not f.
  • 65:47 - 65:48
    Don't confuse it.
  • 65:48 - 65:51
    It is my beautiful
    script C. I've
  • 65:51 - 65:52
    tried to use it many times.
  • 65:52 - 65:55
    Going to be minus y dx plus xdy.
  • 65:55 - 65:58
  • 65:58 - 65:59
    Again, why was that?
  • 65:59 - 66:05
    Because we said this
    is M and this is N,
  • 66:05 - 66:09
    and Green's theorem will give
    you double integral of N sub x
  • 66:09 - 66:11
    minus M sub y.
  • 66:11 - 66:14
    So you have 1 minus
    minus 1, which is 2.
  • 66:14 - 66:16
    And 2 knocked that out.
  • 66:16 - 66:16
    OK.
  • 66:16 - 66:19
    That's how we prove it.
  • 66:19 - 66:20
    OK.
  • 66:20 - 66:24
    Problem is that I do not the
    parametrization of the ellipse.
  • 66:24 - 66:28
    And if somebody doesn't help me,
    I'm going to be in big trouble.
  • 66:28 - 66:33
  • 66:33 - 66:34
    And I'll start
    cursing and I'm not
  • 66:34 - 66:37
    allowed to curse in
    front of the classroom.
  • 66:37 - 66:41
    But you can help me on
    that, because this reminds
  • 66:41 - 66:46
    you of a famous Greek identity.
  • 66:46 - 66:49
    The fundamental trig identity.
  • 66:49 - 66:52
    If this would be cosine
    squared of theta,
  • 66:52 - 66:55
    and this would be sine squared
    of theta, as two animals,
  • 66:55 - 66:57
    their sum would be 1.
  • 66:57 - 67:01
    And whenever you have sums
    of sum squared thingies,
  • 67:01 - 67:04
    then you have to think trig.
  • 67:04 - 67:07
    So, what would be
    good as a parameter?
  • 67:07 - 67:07
    OK.
  • 67:07 - 67:10
    What would be good
    as a parametrization
  • 67:10 - 67:12
    to make this come true?
  • 67:12 - 67:15
    STUDENT: You have the cosine
    of theta would equal x over x.
  • 67:15 - 67:16
    MAGDALENA TODA: Uh-huh.
  • 67:16 - 67:18
    So then x would be A times--
  • 67:18 - 67:19
    STUDENT: The cosine of theta.
  • 67:19 - 67:22
    MAGDALENA TODA:
    Do you like theta?
  • 67:22 - 67:24
    You don't, because
    you're not Greek.
  • 67:24 - 67:25
    That's the problem.
  • 67:25 - 67:27
    If you were Greek,
    you would like it.
  • 67:27 - 67:29
    We had a colleague who
    is not here anymore.
  • 67:29 - 67:31
    Greek from Cypress.
  • 67:31 - 67:38
    And he could claim that the
    most important-- most important
  • 67:38 - 67:40
    alphabet is the
    Greek one, and that's
  • 67:40 - 67:44
    why the mathematicians
    adopted it.
  • 67:44 - 67:45
    OK?
  • 67:45 - 67:47
    B sine t.
  • 67:47 - 67:48
    How do you check?
  • 67:48 - 67:49
    You always think, OK.
  • 67:49 - 67:51
    This over that is cosine.
  • 67:51 - 67:53
    This over this is sine.
  • 67:53 - 67:54
    I square them.
  • 67:54 - 67:56
    I get exactly that
    and I get a 1.
  • 67:56 - 67:57
    Good.
  • 67:57 - 67:58
    I'm in good shape.
  • 67:58 - 68:01
    I know that this
    implicit equation--
  • 68:01 - 68:05
    this is an implicit
    equation-- happens if and only
  • 68:05 - 68:11
    if I have this system of
    the parametrization with t
  • 68:11 - 68:17
    between-- anything I want,
    including the basic 0 to 2
  • 68:17 - 68:18
    pi interval.
  • 68:18 - 68:22
    And then if I were to move
    all around for time real t
  • 68:22 - 68:26
    I would wind around that the
    circle infinitely many times.
  • 68:26 - 68:29
    Between time equals
    minus infinity--
  • 68:29 - 68:33
    that nobody remembers-- and
    time equals plus infinity--
  • 68:33 - 68:36
    that nobody will
    ever get to know.
  • 68:36 - 68:39
    So those are the values of it.
  • 68:39 - 68:41
    All the real values, actually.
  • 68:41 - 68:45
    I only needed from 0 to 2
    pi to wind one time around.
  • 68:45 - 68:47
    And this is the idea.
  • 68:47 - 68:49
    I wind one time around.
  • 68:49 - 68:51
    Now people-- you're going
    to see mathematicians
  • 68:51 - 68:53
    are not the greatest people.
  • 68:53 - 69:01
    I've seen engineers and
    physicists use a lot this sign.
  • 69:01 - 69:02
    Do you know what this means?
  • 69:02 - 69:04
    STUDENT: It means
    one full revolution.
  • 69:04 - 69:07
    MAGDALENA TODA: It
    means a full revolution.
  • 69:07 - 69:10
    You're going to have
    a loop-- loops, that's
  • 69:10 - 69:11
    whatever you want.
  • 69:11 - 69:13
    Here and goes counterclockwise.
  • 69:13 - 69:16
    And they put this
    little sign showing
  • 69:16 - 69:22
    I'm going counterclockwise on
    a closed curved, or a loop.
  • 69:22 - 69:23
    All right.
  • 69:23 - 69:24
    Don't think they are crazy.
  • 69:24 - 69:27
    This was used in lots
    of scientific papers
  • 69:27 - 69:31
    in math, physics, and
    engineering, and so on.
  • 69:31 - 69:31
    OK.
  • 69:31 - 69:35
  • 69:35 - 69:37
    Let's do it then.
  • 69:37 - 69:38
    Can we do it by ourselves?
  • 69:38 - 69:39
    I think so.
  • 69:39 - 69:40
    That's see.
  • 69:40 - 69:42
    1/2 is 1.
  • 69:42 - 69:45
    And I don't like
    the pink marker.
  • 69:45 - 69:47
    Integral log.
  • 69:47 - 69:52
    Time from 0 to 2 pi
    should be measured.
  • 69:52 - 69:56
    y minus B sine t.
  • 69:56 - 70:02
  • 70:02 - 70:04
    dx-- what tells me that?
  • 70:04 - 70:07
    STUDENT: B minus--
  • 70:07 - 70:07
  • 70:07 - 70:08
    MAGDALENA TODA: Very good.
  • 70:08 - 70:10
    Minus A sine t.
  • 70:10 - 70:11
    How hard is that?
  • 70:11 - 70:16
    It's a piece of cake Plus x--
  • 70:16 - 70:18
    STUDENT: A cosine.
  • 70:18 - 70:19
    MAGDALENA TODA: Very good.
  • 70:19 - 70:22
    A cosine t.
  • 70:22 - 70:23
    TImes--
  • 70:23 - 70:26
    STUDENT: B cosine t.
  • 70:26 - 70:29
    MAGDALENA TODA: --B cosine t.
  • 70:29 - 70:30
    And dt.
  • 70:30 - 70:33
    And this thing-- look at it.
  • 70:33 - 70:33
    It's huge.
  • 70:33 - 70:36
    It looks huge, but it's
    so beautiful, because--
  • 70:36 - 70:37
    STUDENT: AB.
  • 70:37 - 70:37
    MAGDALENA TODA: AB.
  • 70:37 - 70:39
    Why is it AB?
  • 70:39 - 70:44
    It's AB because sine squared
    plus cosine squared inside
  • 70:44 - 70:46
    becomes 1.
  • 70:46 - 70:50
    And I have plus AB,
    plus AB, AB out.
  • 70:50 - 70:52
    Kick out the AB.
  • 70:52 - 70:57
    Kick out the A and
    the B and you get
  • 70:57 - 71:02
    something beautiful-- sine
    squared t plus cosine squared
  • 71:02 - 71:03
    t is your old friend.
  • 71:03 - 71:05
    And he says, I'm 1.
  • 71:05 - 71:08
    Look how beautiful
    life is for you.
  • 71:08 - 71:09
    Finally, we proved it.
  • 71:09 - 71:11
    What did we prove?
  • 71:11 - 71:12
    We are almost there.
  • 71:12 - 71:13
    We got a 1/2.
  • 71:13 - 71:16
  • 71:16 - 71:19
    A constant value kick out, AB.
  • 71:19 - 71:22
  • 71:22 - 71:22
    STUDENT: Times 2 pi.
  • 71:22 - 71:24
    MAGDALENA TODA: Times 2 pi.
  • 71:24 - 71:27
  • 71:27 - 71:28
    Good.
  • 71:28 - 71:30
    2 goes away.
  • 71:30 - 71:33
    And we got a magic thing that
    nobody taught us in school,
  • 71:33 - 71:35
    because they were mean.
  • 71:35 - 71:37
    They really didn't want
    us to learn too much.
  • 71:37 - 71:39
    That's the thingy.
  • 71:39 - 71:41
    AB pi.
  • 71:41 - 71:45
    AB pi is what we were
    hoping for, because, look.
  • 71:45 - 71:48
    I mean it's almost
    too good to be true.
  • 71:48 - 71:54
    Well, it's a disk of radius
    r, A and B are equal.
  • 71:54 - 71:56
    And they are the
    radius of the disk.
  • 71:56 - 71:59
    And that's why we
    have pi r squared
  • 71:59 - 72:01
    as a particular
    example of the disk
  • 72:01 - 72:05
    of the area of this ellipse.
  • 72:05 - 72:08
    When I saw it the first
    time, I was like, well,
  • 72:08 - 72:12
    I'm glad that I lived to be
    30 or something to learn this.
  • 72:12 - 72:18
    Because nobody had shown it
    to me in K-12 or in college.
  • 72:18 - 72:23
    And I was a completing-- I was
    a PhD and I didn't know it.
  • 72:23 - 72:25
    And then I said, oh,
    that's why-- pi AB.
  • 72:25 - 72:27
    Yes, OK.
  • 72:27 - 72:28
    All right.
  • 72:28 - 72:32
    So it's so easy to
    understand once you-- well.
  • 72:32 - 72:33
    Once you learn the section.
  • 72:33 - 72:35
    If you don't learn
    the section you
  • 72:35 - 72:39
    will not be able to understand.
  • 72:39 - 72:39
    OK.
  • 72:39 - 72:40
    All right.
  • 72:40 - 72:42
    I'm going to go
    ahead and erase this.
  • 72:42 - 72:45
    And I'll show you
    an example that
  • 72:45 - 72:50
    was popping up like an obsession
    with the numbers changed
  • 72:50 - 72:53
    in most of the final exams
    that happen in the last three
  • 72:53 - 72:59
    years, regardless of
    who wrote the exam.
  • 72:59 - 73:05
    Because this problem really
    matches the learning outcomes,
  • 73:05 - 73:09
    oh, just about any university--
    any good university
  • 73:09 - 73:11
    around the world.
  • 73:11 - 73:12
    So you'll say, wow.
  • 73:12 - 73:13
    It's so easy.
  • 73:13 - 73:17
    I could not believe it
    that-- how easy it is.
  • 73:17 - 73:26
    But once you see it, you
    will-- you'll say, wow.
  • 73:26 - 73:27
    It's easy.
  • 73:27 - 73:35
  • 73:35 - 73:35
    OK.
  • 73:35 - 73:41
  • 73:41 - 73:44
    [CHATTER]
  • 73:44 - 73:46
    Let's try this one.
  • 73:46 - 73:49
    You have a circle.
  • 73:49 - 73:58
    and the circle will be
    a circle radius r given
  • 73:58 - 74:04
    and origin 0 of 4, 9, 0, and 0.
  • 74:04 - 74:09
  • 74:09 - 74:17
    And I'm going to
    write-- I'm going
  • 74:17 - 74:20
    to give you-- first I'm going
    to give you a very simple one.
  • 74:20 - 74:31
  • 74:31 - 74:38
    Compute in the
    simplest possible way.
  • 74:38 - 74:42
    If you don't want to
    parametrize the circle--
  • 74:42 - 74:43
    you can always
    parametrize the circle.
  • 74:43 - 74:44
    Right?
  • 74:44 - 74:45
    But you don't want to.
  • 74:45 - 74:49
    You want to do it the
    fastest possible way
  • 74:49 - 74:51
    without parameterizing
    the circle.
  • 74:51 - 74:54
    Without writing down
    what I'm writing down.
  • 74:54 - 74:55
    You are in a hurry.
  • 74:55 - 74:59
    You have 20-- 15 minutes
    left of your final.
  • 74:59 - 75:01
    And you're looking
    at me and say, I
  • 75:01 - 75:02
    hope I get an A in this final.
  • 75:02 - 75:06
    So what do you have to
    remember when you look at that?
  • 75:06 - 75:10
  • 75:10 - 75:15
    M and M. M and M.
    No, M and N. OK.
  • 75:15 - 75:19
    And you have to remember
    that you are over a circle
  • 75:19 - 75:20
    so you have a closed loop.
  • 75:20 - 75:22
    And that's a Jordan curve.
  • 75:22 - 75:24
    That's enclosing a disk.
  • 75:24 - 75:28
    So you have a relationship
    between the path
  • 75:28 - 75:35
    integral along the C and the
    area along the D-- over D.
  • 75:35 - 75:36
    Which is of what?
  • 75:36 - 75:39
    Is N sub x minus M sub y.
  • 75:39 - 75:41
    So let me write it
    in this form, which
  • 75:41 - 75:46
    is the same thing my students
    mostly prefer to write it as.
  • 75:46 - 75:49
    N sub x minus M sub y.
  • 75:49 - 75:52
    The t-shirt I have
    has it written
  • 75:52 - 75:57
    like that, because it was
    bought from nerdytshirt.com
  • 75:57 - 76:01
    And it was especially
    created to impress nerds.
  • 76:01 - 76:04
    And of course if you
    look at the del notation
  • 76:04 - 76:07
    that gives you that kind
    of snobbish attitude
  • 76:07 - 76:12
    that you aren't a scientist.
  • 76:12 - 76:12
    OK.
  • 76:12 - 76:16
    So what is this
    going to be then?
  • 76:16 - 76:19
    Double integral over d.
  • 76:19 - 76:22
    And sub x is up
    here so it gave 5.
  • 76:22 - 76:25
    And sub y is a piece of cake.
  • 76:25 - 76:37
    3 dx dy equals 2 out times
    the area of the disk, which
  • 76:37 - 76:38
    is something you know.
  • 76:38 - 76:41
    And I'm not going to ask you
    to prove that all over again.
  • 76:41 - 76:43
    So you have to say 2.
  • 76:43 - 76:47
    I know the area of the
    disk-- pi r squared.
  • 76:47 - 76:48
    And that's the answer.
  • 76:48 - 76:49
    And you leave the room.
  • 76:49 - 76:50
    And that's it.
  • 76:50 - 76:52
    It's almost too
    easy to believe it,
  • 76:52 - 76:58
    but it was always there in
    the simplest possible way.
  • 76:58 - 77:03
    And now I'm wondering, if I
    were to give you something hard,
  • 77:03 - 77:08
    because-- you know my theory
    that when you practice
  • 77:08 - 77:12
    at something in
    the classroom you
  • 77:12 - 77:17
    have to be working on harder
    things in the classroom
  • 77:17 - 77:19
    to do better in the exam.
  • 77:19 - 77:23
    So let me cook up
    something ugly for you.
  • 77:23 - 77:26
    The same kind of disk.
  • 77:26 - 77:28
    And I'm changing the functions.
  • 77:28 - 77:33
    And I'll make it
    more complicated.
  • 77:33 - 77:36
  • 77:36 - 77:40
    Let's see how you
    perform on this one.
  • 77:40 - 77:47
  • 77:47 - 77:50
    We avoided that one,
    probably, on finals
  • 77:50 - 77:52
    because I think the
    majority of students
  • 77:52 - 77:58
    wouldn't have understood what
    theorem they needed to apply.
  • 77:58 - 78:00
    It looks a little bit scary.
  • 78:00 - 78:02
    But let's say that I've
    given you the hint,
  • 78:02 - 78:05
    apply Greens theorem
    on the same path
  • 78:05 - 78:10
    integral, which is a circle
    of origin 0 and radius r.
  • 78:10 - 78:14
    I now draw counterclockwise.
  • 78:14 - 78:18
    You apply Green's theorem and
    you say, I know how to do this,
  • 78:18 - 78:21
    because now I know the theorem.
  • 78:21 - 78:27
    This is M. This is N. And I--
    my t-shirt did not say M and N.
  • 78:27 - 78:31
    It said P and Q. Do you
    want to put P and Q?
  • 78:31 - 78:32
    I put P and Q.
  • 78:32 - 78:35
    So I can-- I can have this
    like it is on my t-shirt.
  • 78:35 - 78:39
    So this is going
    to be P sub x-- no.
  • 78:39 - 78:40
    Q sub x.
  • 78:40 - 78:41
    Sorry.
  • 78:41 - 78:45
    M and N. So the second
    one with respect to x.
  • 78:45 - 78:49
    The one that sticks to the y
    is prime root respect to x.
  • 78:49 - 78:54
    The one that sticks to dx is
    prime root with respect to y.
  • 78:54 - 78:57
    And I think one
    time-- the one time
  • 78:57 - 79:01
    when that my friend and
    colleague wrote that,
  • 79:01 - 79:03
    he did it differently.
  • 79:03 - 79:06
    He wrote something
    like, just-- I'll
  • 79:06 - 79:10
    put-- I don't remember what.
  • 79:10 - 79:11
    He put this one.
  • 79:11 - 79:14
  • 79:14 - 79:17
    Then the student
    was used to dx/dy
  • 79:17 - 79:19
    and got completely confused.
  • 79:19 - 79:26
    So pay attention to
    what you are saying.
  • 79:26 - 79:29
    Most of us write it
    in x and y first.
  • 79:29 - 79:33
    And we can see that the
    derivative with respect
  • 79:33 - 79:39
    to x of q, because that is
    the one next to be the y.
  • 79:39 - 79:42
    When he gave it to me
    like that, he messed up
  • 79:42 - 79:45
    everybody's notations.
  • 79:45 - 79:46
    No.
  • 79:46 - 79:47
    Good students steal data.
  • 79:47 - 79:50
    So you guys have to
    put it in standard form
  • 79:50 - 79:53
    and pay attention to
    what you are doing.
  • 79:53 - 79:54
    All right.
  • 79:54 - 79:57
    So that one form can
    be swapped by people
  • 79:57 - 79:59
    who try to play games.
  • 79:59 - 80:03
  • 80:03 - 80:08
    Now in this one-- So you
    have q sub x minus b sub y.
  • 80:08 - 80:16
    You have 3x squared minus
    minus, or just plus, 3y squared.
  • 80:16 - 80:16
    Good.
  • 80:16 - 80:17
    Wonderful.
  • 80:17 - 80:20
    Am I happy, do you
    think I'm happy?
  • 80:20 - 80:23
    Why would I be so happy?
  • 80:23 - 80:26
    Why is this a happy thing?
  • 80:26 - 80:28
    I could have had
    something more wild.
  • 80:28 - 80:28
    I don't.
  • 80:28 - 80:30
    I'm happy I don't.
  • 80:30 - 80:32
    Why am I so happy?
  • 80:32 - 80:34
    Let's see.
  • 80:34 - 80:40
    3 out over the disk.
  • 80:40 - 80:42
    Is this ringing a bell?
  • 80:42 - 80:49
  • 80:49 - 80:50
    Yeah.
  • 80:50 - 80:53
    It's r squared if I
    do this in former.
  • 80:53 - 80:59
    So if I do this in former,
    its going to be rdr, d theta.
  • 80:59 - 81:01
    So life is not as
    hard as you believe.
  • 81:01 - 81:04
    It can look like
    a harder problem,
  • 81:04 - 81:06
    but in reality, it's not really.
  • 81:06 - 81:12
    So I have 3 times-- now, I
    have r squared, I have r cubed.
  • 81:12 - 81:17
    r cubed dr d theta, r between.
  • 81:17 - 81:21
  • 81:21 - 81:31
    r was between 0 and big
    R. Theta will always
  • 81:31 - 81:34
    be between 0 and 2 pi.
  • 81:34 - 81:42
    So, I want you, without
    me to compute the answer
  • 81:42 - 81:44
    and tell me what you got.
  • 81:44 - 81:47
    STUDENT: Just say it?
  • 81:47 - 81:48
    MAGDALENA TODA: Yep.
  • 81:48 - 81:53
    STUDENT: 3/2, pi
    r to the fourth.
  • 81:53 - 81:54
    MAGDALENA TODA: So
    how did you do that?
  • 81:54 - 81:57
    You said, r to the
    4 over 4, coming
  • 81:57 - 82:00
    from integration times the 2 pi,
    coming from integration times
  • 82:00 - 82:02
    3.
  • 82:02 - 82:05
    Are you guys with me?
  • 82:05 - 82:09
    Is everybody with me on this?
  • 82:09 - 82:12
    OK so, we will simplify
    the answer, we'll do that.
  • 82:12 - 82:17
    What regard is the
    radius of the disk?
  • 82:17 - 82:18
    STUDENT: How did he
    solve that integral
  • 82:18 - 82:20
    without switching the poles?
  • 82:20 - 82:26
  • 82:26 - 82:29
    MAGDALENA TODA: It would
    have been a killer.
  • 82:29 - 82:31
    Let me write it out.
  • 82:31 - 82:32
    [LAUGHTER]
  • 82:32 - 82:35
    Because you want to
    write it out, of course.
  • 82:35 - 82:41
    OK, 3 integral, integral
    x squared plus y
  • 82:41 - 82:45
    squared, dy/dx, just to make
    my life a little bit funnier,
  • 82:45 - 82:50
    and then y between minus
    square root-- you're
  • 82:50 - 82:52
    looking for trouble, huh?
  • 82:52 - 83:00
    Y squared minus x squared to
    r squared minus s squared.
  • 83:00 - 83:01
    And again, you could
    do what you just
  • 83:01 - 83:05
    said, split into four integrals
    over four different domains,
  • 83:05 - 83:07
    or two up and down.
  • 83:07 - 83:12
    And minus r and are
    you guys with me?
  • 83:12 - 83:15
    And then, when you go
    and integrate that,
  • 83:15 - 83:23
    you integrate with respect
    to y-- [INAUDIBLE].
  • 83:23 - 83:25
    Well he's right,
    so you can get x
  • 83:25 - 83:28
    squared y plus y cubed over 3.
  • 83:28 - 83:31
  • 83:31 - 83:34
    Between those points, minus 12.
  • 83:34 - 83:36
    And from that moment,
    that would just
  • 83:36 - 83:40
    leave it and go for a walk.
  • 83:40 - 83:43
    I will not have the
    patience to do this.
  • 83:43 - 83:45
    Just a second, Matthew.
  • 83:45 - 83:47
    For this kind of
    stuff, of course
  • 83:47 - 83:50
    I could put this in Maple.
  • 83:50 - 83:54
    You know Maple has these
    little interactive fields,
  • 83:54 - 83:56
    like little squares?
  • 83:56 - 83:59
    And you go inside there
    and add your endpoints.
  • 83:59 - 84:03
    And even if it looks very ugly,
    Maple will spit you the answer.
  • 84:03 - 84:06
    If you know your
    syntax and do it right,
  • 84:06 - 84:08
    even if you don't
    switch to polar
  • 84:08 - 84:10
    coordinates or put
    it in Cartesian.
  • 84:10 - 84:13
    Give it the right data, and
    it's going to spit the answer.
  • 84:13 - 84:14
    Yes, Matthew?
  • 84:14 - 84:16
    STUDENT: I was
    out of the room, I
  • 84:16 - 84:19
    was wondering why
    it's now y cubed.
  • 84:19 - 84:21
    MAGDALENA TODA: Because if
    you integrate with respect
  • 84:21 - 84:24
    to y first--
  • 84:24 - 84:27
    STUDENT: Because when I
    walked out, it was negative y.
  • 84:27 - 84:29
    MAGDALENA TODA: If
    I didn't put minus.
  • 84:29 - 84:30
    STUDENT: It's a new problem.
  • 84:30 - 84:32
    That's what he's confused about.
  • 84:32 - 84:35
    He walked out of the room
    during the previous problem
  • 84:35 - 84:36
    and came back after this one.
  • 84:36 - 84:38
    And now he's confused.
  • 84:38 - 84:40
    MAGDALENA TODA: You don't
    care about what I just asked?
  • 84:40 - 84:40
    STUDENT: Oh.
  • 84:40 - 84:41
    No.
  • 84:41 - 84:44
  • 84:44 - 84:46
    I like the polar coordinates.
  • 84:46 - 84:48
    MAGDALENA TODA: Let
    me ask you a question
  • 84:48 - 84:50
    before I talk any further.
  • 84:50 - 84:53
    I was about to put a plus here.
  • 84:53 - 84:56
    What would have been the problem
    if I had put a plus here?
  • 84:56 - 85:00
  • 85:00 - 85:03
    If I worked this out,
    I would have gotten
  • 85:03 - 85:06
    x squared minus y squared.
  • 85:06 - 85:08
    Would that have been
    the end of the world?
  • 85:08 - 85:10
    No.
  • 85:10 - 85:16
    But it would have complicated
    my life a little bit more.
  • 85:16 - 85:21
    Let's do that one as well.
  • 85:21 - 85:22
    STUDENT: I was
    just curious of how
  • 85:22 - 85:25
    you do any of these problems
    when you can't switch to polar.
  • 85:25 - 85:28
    MAGDALENA TODA: Right, let's see
    what-- because Actually, even
  • 85:28 - 85:32
    in this case, life is not so
    hard, not as hard as you think.
  • 85:32 - 85:35
    The persistence in that matters.
  • 85:35 - 85:38
    You never give up on a
    problem that freaks you out.
  • 85:38 - 85:41
    That's the definition
    of a mathematician.
  • 85:41 - 85:48
    3x squared minus 3y
    squared over dx/dy.
  • 85:48 - 85:50
    Do it slowly because
    I'm not in a hurry.
  • 85:50 - 85:56
    We are almost done with 13.4.
  • 85:56 - 85:57
    This is OK, right?
  • 85:57 - 85:59
    Just the minus sign again?
  • 85:59 - 86:01
    STUDENT: Well not
    the minus sign.
  • 86:01 - 86:04
    I was just wondering because
    in the previous problem
  • 86:04 - 86:07
    you were doing the ellipse, you
    started out with the equation
  • 86:07 - 86:09
    with the negative y--
  • 86:09 - 86:11
    MAGDALENA TODA:
    For this one that's
  • 86:11 - 86:15
    just the limit that says that
    this is the go double integral
  • 86:15 - 86:19
    of the area of the domain.
  • 86:19 - 86:23
    It's just a consequence--
    or correlate if you want.
  • 86:23 - 86:28
    It's a consequence
    of Green's theorem.
  • 86:28 - 86:31
    When you forget that consequence
    of Green's theorem and we say
  • 86:31 - 86:32
    goodbye to that.
  • 86:32 - 86:36
    But while you were out,
    this is Green's theorem.
  • 86:36 - 86:39
    The real Green's theorem,
    the one that was a teacher.
  • 86:39 - 86:41
    There are several
    Greens I can give you.
  • 86:41 - 86:43
    The famous Green
    theorem is the one
  • 86:43 - 86:47
    I said when you have--
    this is what we apply here.
  • 86:47 - 86:51
    The integral of M dx plus M dy.
  • 86:51 - 87:01
    You have a double integral of
    M sub x minus M sub y over c.
  • 87:01 - 87:03
  • 87:03 - 87:08
    So I'm assuming we would have
    had this case of maybe me not
  • 87:08 - 87:11
    paying attention, or
    being mean and not wanting
  • 87:11 - 87:14
    to give you a simple problem.
  • 87:14 - 87:18
    And what do you
    do in such a case?
  • 87:18 - 87:20
    It's not obvious to
    everybody, but you will see.
  • 87:20 - 87:22
    It's so pretty at some
    point, if you know
  • 87:22 - 87:24
    how to get out of the mess.
  • 87:24 - 87:27
  • 87:27 - 87:31
    I was already thinking, but
    I'm using polar coordinates.
  • 87:31 - 87:36
    So that's arc of sine, so I
    have to go back to the basics.
  • 87:36 - 87:40
    If I go back to the
    basics, ideas come to me.
  • 87:40 - 87:42
    Right?
  • 87:42 - 87:46
    So, OK.
  • 87:46 - 87:52
    r-- let's put dr d theta,
    just to get rid of it,
  • 87:52 - 87:54
    because it's on my nerves.
  • 87:54 - 88:00
    This is 0 to 2 pi,
    this is 0 to r.
  • 88:00 - 88:03
    And now, you say,
    OK, in our mind,
  • 88:03 - 88:07
    because we are lazy
    people, plug in those
  • 88:07 - 88:11
    and pull out what you can.
  • 88:11 - 88:15
    One 3 out equals for what?
  • 88:15 - 88:18
    Inside, you have r squared.
  • 88:18 - 88:21
    Do you agree?
  • 88:21 - 88:30
    And times your favorite
    expression, which is cosine
  • 88:30 - 88:33
    squared theta, minus
    i squared theta.
  • 88:33 - 88:35
    And you're going to ask me why.
  • 88:35 - 88:36
    You shouldn't ask me why.
  • 88:36 - 88:40
    You just square these
    and subtract them,
  • 88:40 - 88:44
    and see what in the world
    you're going to get.
  • 88:44 - 88:48
    Because you get r squared
    times cosine squared,
  • 88:48 - 88:50
    minus i squared.
  • 88:50 - 88:51
    I'm too lazy to write
    down the argument.
  • 88:51 - 88:53
    But you know we
    have trigonometry.
  • 88:53 - 88:56
  • 88:56 - 88:58
    Yes, you see why it's
    important for you
  • 88:58 - 89:02
    to learn trigonometry
    when you are little.
  • 89:02 - 89:06
    You may be 50 or
    60, in high school,
  • 89:06 - 89:09
    or you may be freshman year.
  • 89:09 - 89:12
    I don't care when, but you
    have to learn that this is
  • 89:12 - 89:14
    the cosine of the double angle.
  • 89:14 - 89:16
    How many of you remember that?
  • 89:16 - 89:19
    Maybe you learned that?
  • 89:19 - 89:19
    Remember that?
  • 89:19 - 89:21
    OK.
  • 89:21 - 89:26
    I don't blame you at all
    when you don't remember,
  • 89:26 - 89:31
    because since I've been
    the main checker of finals
  • 89:31 - 89:39
    for the past five years--
    it's a lot of finals.
  • 89:39 - 89:41
    Yeah, the i is there.
  • 89:41 - 89:43
    That's exactly what
    I wanted to tell you,
  • 89:43 - 89:46
    that's why I left some room.
  • 89:46 - 89:53
    This data would be t.
  • 89:53 - 89:56
    The double angle formula did
    not appear on many finals.
  • 89:56 - 89:58
    And I was thinking
    it's a period.
  • 89:58 - 90:00
    When I ask the
    instructors, generally they
  • 90:00 - 90:07
    say students have trouble
    remembering or understanding
  • 90:07 - 90:10
    this later on, by
    avoiding the issue,
  • 90:10 - 90:14
    you sort of bound to it for
    the first time in Cal 2,
  • 90:14 - 90:17
    because there are any
    geometric formulas.
  • 90:17 - 90:22
    And then, you bump again
    inside it in Cal 3.
  • 90:22 - 90:23
    And it never leaves you.
  • 90:23 - 90:28
    So this, just knowing this
    will help you so much.
  • 90:28 - 90:31
    Let me put the r nicely here.
  • 90:31 - 90:34
    And now finally, we know
    how to solve it, because I'm
  • 90:34 - 90:35
    going to go ahead and erase.
  • 90:35 - 90:45
  • 90:45 - 90:49
    So why it is good for us is
    that-- as Matthew observed
  • 90:49 - 90:53
    a few moments ago,
    whenever you have
  • 90:53 - 90:57
    a product of a function, you
    not only in a function in theta
  • 90:57 - 91:01
    only, your life becomes easier
    because you can separate them
  • 91:01 - 91:03
    between the rhos.
  • 91:03 - 91:04
    In two different products.
  • 91:04 - 91:06
    So that's would be this theorem.
  • 91:06 - 91:11
    And you have 3 times-- the
    part that depends only on r,
  • 91:11 - 91:14
    and the part that depends
    only on theta, let's
  • 91:14 - 91:15
    put them separate.
  • 91:15 - 91:22
    We need theta, and
    dr. And what do you
  • 91:22 - 91:25
    integrate when you integrate?
  • 91:25 - 91:25
    r cubed.
  • 91:25 - 91:29
    Attention, do not do rr.
  • 91:29 - 91:31
    From 0 to r.
  • 91:31 - 91:32
    OK?
  • 91:32 - 91:34
    STUDENT: And cosine theta?
  • 91:34 - 91:40
    MAGDALENA TODA: And then you
    have a 0 to 2 pi, cosine 2.
  • 91:40 - 91:42
    now, let me give
    you-- Let me tell you
  • 91:42 - 91:45
    what it is, because when
    I was young, I was naive
  • 91:45 - 91:48
    and I always started with that.
  • 91:48 - 91:52
    You should always start with the
    part, the trig part in theta.
  • 91:52 - 91:54
    Because that becomes 0.
  • 91:54 - 91:57
    So no matter how
    ugly this is, I've
  • 91:57 - 92:00
    had professors who are
    playing games with us,
  • 92:00 - 92:04
    and they were giving us
    some extremely ugly thing
  • 92:04 - 92:06
    that would take you forever
    for you to integrate.
  • 92:06 - 92:09
    Or sometimes, it would have
    been impossible to integrate.
  • 92:09 - 92:12
    But then, the whole
    thing would have been 0
  • 92:12 - 92:14
    because when you
    integrate cosine 2 theta,
  • 92:14 - 92:17
    it goes to sine theta.
  • 92:17 - 92:21
    Sine 2 theta at 2 pi and 0
    are the same things, 0 minus 0
  • 92:21 - 92:21
    equals z.
  • 92:21 - 92:24
    So the answer is z.
  • 92:24 - 92:27
    I cannot tell you how many
    professors I've had who will
  • 92:27 - 92:29
    play this game with us.
  • 92:29 - 92:30
    They give us something
    that discouraged us.
  • 92:30 - 92:34
    No, it's not a piece of cake,
    compared to what I have.
  • 92:34 - 92:37
    Some integral value
    will go over two lines,
  • 92:37 - 92:40
    with a huge polynomial
    or something.
  • 92:40 - 92:44
    But in the end, the integral
    was 0 for such a result. Yes?
  • 92:44 - 92:45
    STUDENT: So I have a question.
  • 92:45 - 92:50
    Could we take that force and
    prove that it was conservative?
  • 92:50 - 92:55
    MAGDALENA TODA: So now
    that I'm questioning this,
  • 92:55 - 93:00
    I'm not questioning
    you, but I-- is
  • 93:00 - 93:06
    the force, that is with you--
    what is the original force
  • 93:06 - 93:08
    that Alex is talking about?
  • 93:08 - 93:17
    If I take y cubed i plus x cubed
    j-- and you have to be careful.
  • 93:17 - 93:19
    Is this conservative?
  • 93:19 - 93:23
  • 93:23 - 93:25
    STUDENT: Yeah.
  • 93:25 - 93:28
    MAGDALENA TODA: Really?
  • 93:28 - 93:31
    Why would we pick
    a conservative?
  • 93:31 - 93:34
    STUDENT: Y squared plus
    x squared over 2 is--
  • 93:34 - 93:36
    MAGDALENA TODA: Why is
    it not conservative?
  • 93:36 - 93:39
  • 93:39 - 93:41
    IT doesn't pass the hole test.
  • 93:41 - 93:44
  • 93:44 - 93:48
    So p sub y is not
    equal to q sub x.
  • 93:48 - 93:52
    If you primed this with respect
    to y, you get that dy squared.
  • 93:52 - 93:55
    Prime this with this respect
    to x, you get 3x squared.
  • 93:55 - 93:57
    So it's not concerned with him.
  • 93:57 - 94:01
    And still, I'm
    getting-- it's a loop,
  • 94:01 - 94:05
    and I'm getting a 0, sort
    of like I would expect it
  • 94:05 - 94:08
    I had any dependence of that.
  • 94:08 - 94:09
    What is the secret here?
  • 94:09 - 94:14
    STUDENT: That is conservative,
    given a condition.
  • 94:14 - 94:17
    MAGDALENA TODA: Yes,
    given a condition
  • 94:17 - 94:21
    that your x and y are moving
    on the serpent's circle.
  • 94:21 - 94:26
    And that happens, because this
    is a symmetric expression,
  • 94:26 - 94:28
    and x and y are
    moving on a circle,
  • 94:28 - 94:31
    and one is the cosine theta
    and one is sine theta.
  • 94:31 - 94:35
    So in the end, it
    simplifies out.
  • 94:35 - 94:40
    But in general, if I would
    have this kind of problem--
  • 94:40 - 94:44
    if somebody asked me is this
    conservative, the answer is no.
  • 94:44 - 94:46
    Let me give you a
    few more examples.
  • 94:46 - 94:58
  • 94:58 - 95:15
    One example that maybe will look
    hard to most people is here.
  • 95:15 - 95:37
  • 95:37 - 95:50
    The vector value function
    given by f of x, y incline,
  • 95:50 - 95:52
    are two values.
  • 95:52 - 95:55
    No, I mean define two
    values of [INAUDIBLE].
  • 95:55 - 96:17
  • 96:17 - 96:19
    A typical exam problem.
  • 96:19 - 96:23
    And I saw it at
    Texas A&M, as well.
  • 96:23 - 96:28
    So maybe some people like this
    kind of a, b, c, d problem.
  • 96:28 - 96:29
    Is f conservative?
  • 96:29 - 96:37
  • 96:37 - 96:38
    STUDENT: Yep
  • 96:38 - 96:40
    MAGDALENA TODA:
    You already did it?
  • 96:40 - 96:41
    Good for you guys.
  • 96:41 - 96:45
    So if I gave you one that
    has three components what
  • 96:45 - 96:47
    did you have to do?
  • 96:47 - 96:50
    Compute the curl.
  • 96:50 - 96:52
    You can, of course, compute
    the curl also on this one
  • 96:52 - 96:55
    and have 0 for the
    third component.
  • 96:55 - 97:02
    But the simplest thing
    is to do f1 and f2.
  • 97:02 - 97:07
    f1 prime with respect to y
    equals f2 prime with respect
  • 97:07 - 97:08
    to x.
  • 97:08 - 97:13
    So I'm going to
    make a smile here.
  • 97:13 - 97:16
    And you realize that the authors
    of such a problem, whether they
  • 97:16 - 97:21
    are at Tech or at Texas
    A&M. They do that on purpose
  • 97:21 - 97:28
    so that you can use this
    result to the next level.
  • 97:28 - 98:04
    And they're saying compute
    the happy u over the curve
  • 98:04 - 98:23
    x cubed and y cubed equals 8 on
    the path that connects points
  • 98:23 - 98:29
    2, 1 and 1, 2 in [INAUDIBLE].
  • 98:29 - 98:39
  • 98:39 - 98:46
    Does this integral depend on f?
  • 98:46 - 98:51
  • 98:51 - 98:52
    State why.
  • 98:52 - 98:58
  • 98:58 - 99:05
    And you see, they don't tell
    you find the scalar potential.
  • 99:05 - 99:07
    Which is bad, and
    many of you will
  • 99:07 - 99:09
    be able to see it
    because you have
  • 99:09 - 99:14
    good mathematical intuition,
    and a computer process
  • 99:14 - 99:17
    planning in the background
    over all the other processes.
  • 99:17 - 99:19
    We are very visual people.
  • 99:19 - 99:22
    If you realize that every time
    just there with each other
  • 99:22 - 99:26
    through the classroom, there
    are hundreds of distractions.
  • 99:26 - 99:28
    There's the screen,
    there is somebody
  • 99:28 - 99:31
    who's next to you
    who's sneezing,
  • 99:31 - 99:35
    all sorts of distractions.
  • 99:35 - 99:38
    Still, your computer
    unit can still
  • 99:38 - 99:41
    function, trying to
    integrate and find the scalar
  • 99:41 - 99:42
    potential, which is a miracle.
  • 99:42 - 99:46
    I don't know how we managed
    to do that after all.
  • 99:46 - 99:50
    If you don't manage to do that,
    what do you have to set up?
  • 99:50 - 99:55
    You have to say, find is
    there-- well, you know there is.
  • 99:55 - 100:00
    So you're not going to question
    the existence of the scalar
  • 100:00 - 100:04
    potential You know it exists,
    but you don't know what it is.
  • 100:04 - 100:10
    What is f such that f sub
    x would be 6xy plus 1,
  • 100:10 - 100:14
    and m sub y will be 3x squared?
  • 100:14 - 100:18
    And normally, you would
    have to integrate backwards.
  • 100:18 - 100:21
    Now, I'll give you 10 seconds.
  • 100:21 - 100:25
    If in 10 seconds, you don't
    find me a scalar potential,
  • 100:25 - 100:27
    I'm going to make you
    integrate backwards.
  • 100:27 - 100:31
    So this is finding the scalar
    potential by integration.
  • 100:31 - 100:34
    The way you should, if
    you weren't very smart.
  • 100:34 - 100:38
    But I think you're
    smart enough to smell
  • 100:38 - 100:42
    the potential-- Very good.
  • 100:42 - 100:44
    But what if you don't?
  • 100:44 - 100:46
    OK I'm asking.
  • 100:46 - 100:50
    So we had one or two
    student who figured it out.
  • 100:50 - 100:51
    What if you don't?
  • 100:51 - 100:55
    If you don't, you can still do
    perfectly fine on this problem.
  • 100:55 - 101:01
    Let's see how we do it
    without seeing or guessing.
  • 101:01 - 101:03
    His brain was running
    in the background.
  • 101:03 - 101:05
    He came up with the answer.
  • 101:05 - 101:06
    He's happy.
  • 101:06 - 101:10
    He can move on to
    the next level.
  • 101:10 - 101:12
    STUDENT: Integrate both
    sides with respect to r.
  • 101:12 - 101:16
    MAGDALENA TODA: Right, and
    then mix and match them.
  • 101:16 - 101:18
    Make them in work.
  • 101:18 - 101:21
    So try to integrate
    with respect to x.
  • 101:21 - 101:26
    6y-- or plus 1, I'm sorry guys.
  • 101:26 - 101:29
    And once you get it,
    you're going to get--
  • 101:29 - 101:32
    STUDENT: 3x squared y plus x.
  • 101:32 - 101:35
    MAGDALENA TODA: And
    plus a c of what?
  • 101:35 - 101:38
    And then take this fellow and
    prime it with respect to y.
  • 101:38 - 101:41
    And you're going to
    get-- it's not hard.
  • 101:41 - 101:44
    You're going to get dx
    squared plus nothing,
  • 101:44 - 101:50
    plus c from the y, and it's
    good because I gave you
  • 101:50 - 101:51
    a simple one.
  • 101:51 - 101:54
    So sometimes you can
    have something here,
  • 101:54 - 101:57
    but in this case, it was just 0.
  • 101:57 - 102:00
    So c is kappa as a constant.
  • 102:00 - 102:05
    So instead of why we teach
    found with a plus kappa here,
  • 102:05 - 102:08
    and it still does it.
  • 102:08 - 102:13
    So on such a problem,
    I don't know,
  • 102:13 - 102:18
    but I think I would give equal
    weights to it, B and C. Compute
  • 102:18 - 102:21
    the path integral
    over the curve.
  • 102:21 - 102:24
    This is horrible, as
    an increasing curve.
  • 102:24 - 102:27
    But I know that
    there is a path that
  • 102:27 - 102:29
    connects the points 2, 1 and 1.
  • 102:29 - 102:30
    What I have to pay
    attention to in my mind
  • 102:30 - 102:33
    is that these points
    actually are on the curve.
  • 102:33 - 102:36
    And they are, because I
    have 8 times 1 equals 8,
  • 102:36 - 102:38
    1 times 8 equals 8.
  • 102:38 - 102:41
    So while I was writing it,
    I had to think a little bit
  • 102:41 - 102:43
    on the problem.
  • 102:43 - 102:45
    If you were to
    draw-- well that's
  • 102:45 - 102:48
    for you have to find
    out when you go home.
  • 102:48 - 102:52
    What do you think
    this is going to be?
  • 102:52 - 102:55
  • 102:55 - 102:58
    Actually, we have to
    do it now, because it's
  • 102:58 - 103:02
    a lot simpler than
    you think it is.
  • 103:02 - 103:07
    x and y will be positive,
    I can also restrict that.
  • 103:07 - 103:09
    It looks horrible, but
    it's actually much easier
  • 103:09 - 103:10
    than you think.
  • 103:10 - 103:16
    So how do I compute that path
    integral that makes the points?
  • 103:16 - 103:19
    I'm going to have
    fundamental there.
  • 103:19 - 103:23
  • 103:23 - 103:27
    Which has f of x at q
    minus f, with p, which
  • 103:27 - 103:31
    says that little f is here.
  • 103:31 - 103:41
    3x squared y plus
    x at 2, 1 minus 3x
  • 103:41 - 103:47
    squared y plus x at 1, 2.
  • 103:47 - 103:53
    So all I have to do is
    go ahead and-- do you
  • 103:53 - 103:57
    see what I'm actually doing?
  • 103:57 - 103:58
    It's funny.
  • 103:58 - 104:02
    Which one is the origin, and
    which one is the endpoint?
  • 104:02 - 104:04
    The problem doesn't tell you.
  • 104:04 - 104:07
    It tells you only you are
    connecting the two points.
  • 104:07 - 104:10
    But which one is the alpha,
    and which one is the omega?
  • 104:10 - 104:11
    Where do you start?
  • 104:11 - 104:13
    You start here or
    you start here?
  • 104:13 - 104:16
  • 104:16 - 104:17
    OK.
  • 104:17 - 104:19
    Sort of arbitrary.
  • 104:19 - 104:22
    How do you handle this problem?
  • 104:22 - 104:26
    Depending on the direction--
    pick one direction you move on
  • 104:26 - 104:29
    along the r, it's up to you.
  • 104:29 - 104:32
    And then you get an answer, and
    if you change the direction,
  • 104:32 - 104:34
    what's going to happen
    to the integral?
  • 104:34 - 104:38
    It's just change the
    sign and that's all.
  • 104:38 - 104:43
    3 times 4, times 1, plus 2--
    guys, keep an eye on my algebra
  • 104:43 - 104:48
    please, because I
    don't want to mess up.
  • 104:48 - 104:50
    Am I right, here?
  • 104:50 - 104:50
    STUDENT: Yes.
  • 104:50 - 104:52
    MAGDALENA TODA: So how much?
  • 104:52 - 104:54
    14, is it?
  • 104:54 - 104:56
    STUDENT: It's 7.
  • 104:56 - 104:57
    MAGDALENA TODA: Minus 7.
  • 104:57 - 105:06
  • 105:06 - 105:07
    Good.
  • 105:07 - 105:08
    Wonderful.
  • 105:08 - 105:12
    So we know what to get,
    and we know this does not
  • 105:12 - 105:13
    depend on the fact.
  • 105:13 - 105:17
    How much blah, blah,
    blah does the instructor
  • 105:17 - 105:21
    expect for you to get full
    credit on the problem?
  • 105:21 - 105:22
    STUDENT: Just enough to explain.
  • 105:22 - 105:24
    MAGDALENA TODA: Just
    enough to explain.
  • 105:24 - 105:30
    About 2 lines or 1 line saying
    you can say anything really.
  • 105:30 - 105:34
    You can say this is the theorem
    that either shows independence
  • 105:34 - 105:36
    of that integral.
  • 105:36 - 105:43
    If the force F vector value
    function is conservative,
  • 105:43 - 105:47
    then this is what
    you have to write.
  • 105:47 - 105:49
    This doesn't depend
    on the path c.
  • 105:49 - 105:51
    And you apply the
    fundamental theorem
  • 105:51 - 105:54
    of path integrals for
    the scalar potential.
  • 105:54 - 105:58
    And that scalar potential
    depends on the endpoints
  • 105:58 - 106:00
    that you're taking.
  • 106:00 - 106:02
    And the value of
    the work depends--
  • 106:02 - 106:06
    the work depends only on the
    scalar potential and the two
  • 106:06 - 106:08
    points.
  • 106:08 - 106:08
    That's enough.
  • 106:08 - 106:10
    That's more than enough.
  • 106:10 - 106:14
    What if somebody's
    not good with wording?
  • 106:14 - 106:17
    I'm not going to write
    her all that explanation.
  • 106:17 - 106:22
    I'm just going to say whatever.
  • 106:22 - 106:25
    I'm going to give
    her the theorem
  • 106:25 - 106:27
    in mathematical compressed way.
  • 106:27 - 106:31
    And I don't care if she
    understands it or not.
  • 106:31 - 106:35
    Even if you write this
    formula with not much wording,
  • 106:35 - 106:37
    I still give you credit.
  • 106:37 - 106:39
    But I would prefer
    that you give me
  • 106:39 - 106:42
    some sort of-- some
    sort of explanation.
  • 106:42 - 106:43
    Yes, sir.
  • 106:43 - 106:44
    STUDENT: You said answer was 0.
  • 106:44 - 106:46
    Then it would have
    been path independent?
  • 106:46 - 106:51
  • 106:51 - 106:54
    MAGDALENA TODA: No, the
    answer would not be for sure 0
  • 106:54 - 106:57
    if it was a longer loop.
  • 106:57 - 106:59
    If it were a longer
    closed curve,
  • 106:59 - 107:04
    that way where it
    starts, it ends.
  • 107:04 - 107:07
    Even if I take a weekly
    road between the two points,
  • 107:07 - 107:09
    I still get 7, right?
  • 107:09 - 107:11
    That's the whole idea.
  • 107:11 - 107:13
    Am I clear about that?
  • 107:13 - 107:15
    Are we clear about that?
  • 107:15 - 107:21
    Let me ask you though,
    how do you find out?
  • 107:21 - 107:26
    Because I don't know how
    many of you figured out
  • 107:26 - 107:29
    what kind of curve that is.
  • 107:29 - 107:33
    And it looks like an enemy
    to you, but there is a catch.
  • 107:33 - 107:39
    It's an old friend of
    yours and you don't see it.
  • 107:39 - 107:40
    So what is the curve?
  • 107:40 - 107:41
    What is the curve?
  • 107:41 - 107:47
    And what is this arc of a
    curve between 2, 1 and 1, 2?
  • 107:47 - 107:48
    Can we find out what that is?
  • 107:48 - 107:49
    Of course, or cubic.
  • 107:49 - 107:50
    It's a fake cubic.
  • 107:50 - 107:54
    It's a fake cubic--
  • 107:54 - 107:56
    STUDENT: To function together?
  • 107:56 - 107:58
    MAGDALENA TODA: Let's
    see what this is.
  • 107:58 - 108:03
    xy cubed minus 2 cubed equals 0.
  • 108:03 - 108:06
    We were in fourth grade--
    well, our teachers--
  • 108:06 - 108:14
    I think our teachers teach us
    when we were little that this,
  • 108:14 - 108:17
    if you divided by a
    minus- I wasn't little.
  • 108:17 - 108:19
    I was in high school.
  • 108:19 - 108:21
    Well, 14-year-old.
  • 108:21 - 108:22
    STUDENT: A cubed.
  • 108:22 - 108:23
    STUDENT: A squared.
  • 108:23 - 108:24
    MAGDALENA TODA: A squared.
  • 108:24 - 108:26
    STUDENT: Minus 2AB.
  • 108:26 - 108:27
    Plus 2AB.
  • 108:27 - 108:29
    MAGDALENA TODA: Very good.
  • 108:29 - 108:31
    Plus AB, not 2AB.
  • 108:31 - 108:32
    STUDENT: Oh, darn.
  • 108:32 - 108:34
    MAGDALENA TODA: Plus B squared.
  • 108:34 - 108:35
    Suppose you don't believe.
  • 108:35 - 108:37
    That proves this.
  • 108:37 - 108:38
    Let's multiply.
  • 108:38 - 108:42
    A cubed plus A squared
    B plus AB squared.
  • 108:42 - 108:44
    I'm done with the
    first multiplication.
  • 108:44 - 108:50
    Minus BA squared minus
    AB squared minus B cubed.
  • 108:50 - 108:52
    Do they cancel out?
  • 108:52 - 108:54
    Yes.
  • 108:54 - 108:55
    Good.
  • 108:55 - 108:58
    Cancel out.
  • 108:58 - 109:00
    And cancel out.
  • 109:00 - 109:02
    Out, poof.
  • 109:02 - 109:03
    We've proved it, why?
  • 109:03 - 109:09
    Because maybe some of you--
    nobody gave it to proof before.
  • 109:09 - 109:12
  • 109:12 - 109:18
    So as an application,
    what is this?
  • 109:18 - 109:18
    There.
  • 109:18 - 109:19
    Who is A and who is B?
  • 109:19 - 109:24
    A is xy, B is 2.
  • 109:24 - 109:34
    So you have xy minus 2 times
    all this fluffy guy, xy
  • 109:34 - 109:42
    squared plus 2xy plus--
  • 109:42 - 109:45
    STUDENT: 4.
  • 109:45 - 109:45
    MAGDALENA TODA: 4.
  • 109:45 - 109:49
    And I also said, because
    I was sneaky, that's why.
  • 109:49 - 109:55
    To make your life easier
    or harder. xy is positive.
  • 109:55 - 109:58
    When I said xy was positive,
    what was I intending?
  • 109:58 - 110:03
    I was intending for you to see
    that this cannot be 0 ever.
  • 110:03 - 110:08
    So the only possible
    for you to have 0 here
  • 110:08 - 110:10
    is when xy equals 2.
  • 110:10 - 110:14
    And xy equals 2 is a
    much simpler curve.
  • 110:14 - 110:18
    And I want to know
    if you realize
  • 110:18 - 110:22
    that this will have the points
    2,1 and 1, 2 staring at you.
  • 110:22 - 110:23
    Have a nice day today.
  • 110:23 - 110:25
    Take care.
  • 110:25 - 110:27
    And good luck.
  • 110:27 - 110:32
  • 110:32 - 110:34
    What is it?
  • 110:34 - 110:35
    STUDENT: [INAUDIBLE].
  • 110:35 - 110:37
    MAGDALENA TODA:
    Some sort of animal.
  • 110:37 - 110:38
    It's a curve, a linear curve.
  • 110:38 - 110:42
    It's not a line.
  • 110:42 - 110:43
    What is it?
  • 110:43 - 110:48
    Talking about conics because
    I was talking a little bit
  • 110:48 - 110:50
    with Casey about conics.
  • 110:50 - 110:53
    Is this a conic?
  • 110:53 - 110:53
    Yeah.
  • 110:53 - 110:55
    What is a conic?
  • 110:55 - 111:00
    A conic is any kind of
    curve that looks like this.
  • 111:00 - 111:05
    In general form--
    oh my god, ABCD.
  • 111:05 - 111:08
    Now I got my ABC
    plus f equals 0.
  • 111:08 - 111:10
    This is a conic in plane.
  • 111:10 - 111:14
    My conic is missing
    everything else.
  • 111:14 - 111:16
    And B is 0.
  • 111:16 - 111:19
    And there is a way where
    you-- I showed you how you
  • 111:19 - 111:22
    know what kind of conic it is.
  • 111:22 - 111:28
    A, A, B, B, C. A is
    positive is-- no, A is 0,
  • 111:28 - 111:32
    B is-- it should be 2 here.
  • 111:32 - 111:34
    So you split this in half.
  • 111:34 - 111:37
    1/2, 1/2, and 0.
  • 111:37 - 111:41
    The determinant of this is
    negative, the discriminant.
  • 111:41 - 111:44
    That's why we call it
    discriminant about the conic.
  • 111:44 - 111:45
    So it cannot be an ellipse.
  • 111:45 - 111:46
    So what the heck is it?
  • 111:46 - 111:47
    STUDENT: [INAUDIBLE].
  • 111:47 - 111:49
    MAGDALENA TODA: Well, I'm silly.
  • 111:49 - 111:50
    I should have pulled out for y.
  • 111:50 - 111:53
  • 111:53 - 111:57
    And I knew that it
    goes down like 1/x.
  • 111:57 - 112:01
    But I'm asking you, why in
    the world is that a conic?
  • 112:01 - 112:02
    Because you say, wait.
  • 112:02 - 112:03
    Wait a minute.
  • 112:03 - 112:10
    I know this curve since I was
    five year old in kindergarten.
  • 112:10 - 112:13
    And this is the point 2, 1.
  • 112:13 - 112:17
  • 112:17 - 112:17
    It's on it.
  • 112:17 - 112:23
    And there is a symmetric
    point for your pleasure here.
  • 112:23 - 112:25
    1, 2.
  • 112:25 - 112:27
    And between the
    two points, there
  • 112:27 - 112:32
    is just one arc of a curve.
  • 112:32 - 112:34
    And this is the path that
    you are dragging some object
  • 112:34 - 112:35
    with force f.
  • 112:35 - 112:38
    You are computing
    the work of a-- maybe
  • 112:38 - 112:41
    you're computing the work of
    a neutron between those two
  • 112:41 - 112:43
    locations.
  • 112:43 - 112:44
    It's a--
  • 112:44 - 112:45
    STUDENT: Hyperbola?
  • 112:45 - 112:46
    MAGDALENA TODA: Hyperbola.
  • 112:46 - 112:47
    Why Nitish?
  • 112:47 - 112:48
    Yes, sir.
  • 112:48 - 112:50
    STUDENT: I was just
    wondering, couldn't we
  • 112:50 - 112:52
    have gone to xy equals 2 plane?
  • 112:52 - 112:53
    STUDENT: Yeah, way quicker.
  • 112:53 - 112:55
    STUDENT: x cubed, y
    cubed equals 2 cubed.
  • 112:55 - 112:57
    Then you'd just do both sides--
  • 112:57 - 112:57
    MAGDALENA TODA:
    That's what I did.
  • 112:57 - 112:58
    STUDENT: The cubed root.
  • 112:58 - 112:59
    MAGDALENA TODA:
    Didn't I do that?
  • 112:59 - 113:03
    No, because in
    general, it's not--
  • 113:03 - 113:07
    you cannot say if and only
    if xy equals 2 in general.
  • 113:07 - 113:11
    You have to write to
    decompose the polynomial.
  • 113:11 - 113:12
    You were lucky
    this was positive.
  • 113:12 - 113:15
    STUDENT: Well, because
    we divided by x cubed.
  • 113:15 - 113:17
    We could have just
    divided everything
  • 113:17 - 113:19
    by x cubed, and then taken
    the cube root of both sides.
  • 113:19 - 113:20
    MAGDALENA TODA: He's
    saying the same thing.
  • 113:20 - 113:24
    But in mathematics, we don't--
    let me show you something.
  • 113:24 - 113:25
    STUDENT: It would
    work for this case,
  • 113:25 - 113:27
    but not necessarily
    for all cases?
  • 113:27 - 113:28
    MAGDALENA TODA: Yeah.
  • 113:28 - 113:39
    Let me show you some other
    example where you just-- how
  • 113:39 - 113:41
    do you solve this equation?
  • 113:41 - 113:46
    By the way, a math
    field test is coming.
  • 113:46 - 113:48
    No, only if you're a math major.
  • 113:48 - 113:51
    Sorry, junior or senior.
  • 113:51 - 113:53
    In one math field test,
    you don't have to take it.
  • 113:53 - 113:57
    But some people who
    go to graduate school,
  • 113:57 - 114:01
    if they take the math field
    test, that replaces the GRE,
  • 114:01 - 114:03
    if the school agrees.
  • 114:03 - 114:06
    So there was this questions,
    how many roots does it have
  • 114:06 - 114:08
    and what kind?
  • 114:08 - 114:11
    Two are imaginary
    and one is real.
  • 114:11 - 114:15
    But everybody said
    it only had one root.
  • 114:15 - 114:17
    How can it have one root
    if it's a cubic equation?
  • 114:17 - 114:19
    So one root.
  • 114:19 - 114:21
    x1 is 1.
  • 114:21 - 114:23
    The other two are imaginary.
  • 114:23 - 114:24
    This is the case in this also.
  • 114:24 - 114:26
    You have some imaginary roots.
  • 114:26 - 114:31
    So those roots
    are funny, but you
  • 114:31 - 114:36
    would have to
    solve this equation
  • 114:36 - 114:42
    because this is x minus 1
    times x squared plus x plus 1.
  • 114:42 - 114:46
    So the roots are minus
    1, plus minus square root
  • 114:46 - 114:52
    of b squared minus 4ac
    over 2, which are minus 1
  • 114:52 - 114:57
    plus minus square
    root of 3i over 2.
  • 114:57 - 115:01
    Do you guys know
    how they are called?
  • 115:01 - 115:06
    You know them because in
    some countries we learn them.
  • 115:06 - 115:08
    But do you know the notations?
  • 115:08 - 115:09
    STUDENT: What they call them?
  • 115:09 - 115:10
    MAGDALENA TODA: Yeah.
  • 115:10 - 115:12
  • 115:12 - 115:14
    There is a Greek letter.
  • 115:14 - 115:16
    STUDENT: Iota.
  • 115:16 - 115:17
    MAGDALENA TODA: In
    India, probably.
  • 115:17 - 115:19
    In my country, it was omega.
  • 115:19 - 115:20
    But I don't think--
  • 115:20 - 115:21
    STUDENT: In India, iota.
  • 115:21 - 115:23
  • 115:23 - 115:26
    MAGDALENA TODA: But we call
    them omega and omega squared.
  • 115:26 - 115:29
    Because one is the
    square of the other.
  • 115:29 - 115:30
    They are, of course,
    both imaginary.
  • 115:30 - 115:36
    And we call this the
    cubic roots of unity.
  • 115:36 - 115:39
  • 115:39 - 115:42
    You say Magdalena, why would
    you talk about imaginary numbers
  • 115:42 - 115:44
    when everything is real?
  • 115:44 - 115:44
    OK.
  • 115:44 - 115:48
    It's real for the time being
    while you are still with me.
  • 115:48 - 115:50
    The moment you're going
    to say goodbye to me
  • 115:50 - 115:55
    and you know in 3350 your
    life is going to change.
  • 115:55 - 115:57
    In that course,
    they will ask you
  • 115:57 - 116:03
    to solve this equation just like
    we asked all our 3350 students.
  • 116:03 - 116:05
    To our surprise,
    the students don't
  • 116:05 - 116:07
    know what imaginary roots are.
  • 116:07 - 116:08
    Many, you know.
  • 116:08 - 116:10
    You will refresh your memory.
  • 116:10 - 116:12
    But the majority of
    the students didn't
  • 116:12 - 116:15
    know how to get to
    those imaginary numbers.
  • 116:15 - 116:20
    You're going to need to not
    only use them, but also express
  • 116:20 - 116:23
    these in terms of trigonometry.
  • 116:23 - 116:26
  • 116:26 - 116:32
    So just out of curiosity, since
    I am already talking to you,
  • 116:32 - 116:35
    and since I've preparing you a
    little bit for the differential
  • 116:35 - 116:39
    equations class where you
    have lots of electric circuits
  • 116:39 - 116:41
    and applications
    of trigonometry,
  • 116:41 - 116:46
    these imaginary numbers
    can also be put-- they
  • 116:46 - 116:51
    are in general of the form
    a plus ib. a plus minus ib.
  • 116:51 - 116:55
    And we agree that in
    3350 you have to do that.
  • 116:55 - 116:57
    Out of curiosity,
    is there anybody
  • 116:57 - 117:03
    who knows the trigonometric
    form of these complex numbers?
  • 117:03 - 117:06
    STUDENT: Isn't it r e to the j--
  • 117:06 - 117:10
  • 117:10 - 117:14
    MAGDALENA TODA: So you would
    have exactly what he says here.
  • 117:14 - 117:18
    This number will
    be-- if it's plus.
  • 117:18 - 117:21
    r e to the i theta.
  • 117:21 - 117:26
    He knows a little bit
    more than most students.
  • 117:26 - 117:34
    And that is cosine
    theta plus i sine theta.
  • 117:34 - 117:37
    Can you find me the
    angle theta if I
  • 117:37 - 117:43
    want to write cosine theta
    plus i sine theta or cosine
  • 117:43 - 117:46
    theta minus i sine theta?
  • 117:46 - 117:50
    Can you find me
    the angle of theta?
  • 117:50 - 117:51
    Is it hard?
  • 117:51 - 117:53
    Is it easy?
  • 117:53 - 117:55
    What in the world is it?
  • 117:55 - 118:00
  • 118:00 - 118:01
    Think like this.
  • 118:01 - 118:04
    We are done with this
    example, but I'm just
  • 118:04 - 118:08
    saying some things that
    will help you in 3350.
  • 118:08 - 118:12
    If you want cosine
    theta to be minus 1/2
  • 118:12 - 118:21
    and you want sine theta to be
    root 3 over 2, which quadrant?
  • 118:21 - 118:23
    Which quadrant are you in?
  • 118:23 - 118:24
    STUDENT: Second.
  • 118:24 - 118:26
    MAGDALENA TODA: The
    second quadrant.
  • 118:26 - 118:27
    Very good.
  • 118:27 - 118:28
    All right.
  • 118:28 - 118:31
    So think cosine.
  • 118:31 - 118:36
    If cosine would be a half and
    sine would be root 3 over 2,
  • 118:36 - 118:38
    it would be in first quadrant.
  • 118:38 - 118:40
    And what angle would that be?
  • 118:40 - 118:41
    STUDENT: 60.
  • 118:41 - 118:42
    STUDENT: That's 60--
  • 118:42 - 118:46
    MAGDALENA TODA: 60 degrees,
    which is pi over 3, right?
  • 118:46 - 118:53
    But pi over 3 is your
    friend, so he's happy.
  • 118:53 - 118:55
    Well, he is there somewhere.
  • 118:55 - 118:59
  • 118:59 - 119:01
    STUDENT: 120.
  • 119:01 - 119:05
    MAGDALENA TODA: Where you
    are here, you are at what?
  • 119:05 - 119:07
    How much is 120-- very good.
  • 119:07 - 119:09
    How much is 120 pi?
  • 119:09 - 119:11
    STUDENT: 4 pi?
  • 119:11 - 119:12
    MAGDALENA TODA: No.
  • 119:12 - 119:12
    STUDENT: 2 pi over 3.
  • 119:12 - 119:13
    MAGDALENA TODA: 2 pi over 3.
  • 119:13 - 119:14
    Excellent.
  • 119:14 - 119:17
    So 2 pi over 3.
  • 119:17 - 119:21
    This would be if you
    were to think about it--
  • 119:21 - 119:22
    this is in radians.
  • 119:22 - 119:24
    Let me write radians.
  • 119:24 - 119:28
    In degrees, that's 120 degrees.
  • 119:28 - 119:39
    So to conclude my detour
    to introduction to 3350.
  • 119:39 - 119:47
    When they will ask you to solve
    this equation, x cubed minus 1,
  • 119:47 - 119:50
    you have to tell them like that.
  • 119:50 - 119:53
    They will ask you to put
    it in trigonometric form.
  • 119:53 - 120:04
    x1 is 1, x2 is cosine of 2 pi
    over 3 plus i sine 2 pi over 3.
  • 120:04 - 120:07
    And the other one
    is x3 equals cosine
  • 120:07 - 120:16
    of 2 pi over 3 minus
    i sine of 2 pi over 3.
  • 120:16 - 120:17
    The last thing.
  • 120:17 - 120:19
    Because I should let you go.
  • 120:19 - 120:20
    There was no break.
  • 120:20 - 120:23
    I squeezed your brains
    really bad today.
  • 120:23 - 120:26
    We still have like 150 minutes.
  • 120:26 - 120:29
    I stole from you--
    no, I stole really big
  • 120:29 - 120:33
    because we would have-- yeah,
    we still have 15 minutes.
  • 120:33 - 120:37
    But the break was 10 minutes,
    so I didn't give you a break.
  • 120:37 - 120:40
    What would this be if
    you wanted to express it
  • 120:40 - 120:43
    in terms of another angle?
  • 120:43 - 120:47
    That's the last thing
    I'm asking of you.
  • 120:47 - 120:49
    STUDENT: [INAUDIBLE].
  • 120:49 - 120:51
    MAGDALENA TODA: Not minus.
  • 120:51 - 120:53
    Like cosine of an angle
    plus i sine of an angle.
  • 120:53 - 120:56
    You would need to go to
    another quadrant, right?
  • 120:56 - 120:58
    And which quadrant?
  • 120:58 - 120:58
    STUDENT: 4.
  • 120:58 - 121:00
    MAGDALENA TODA:
    You've said it before.
  • 121:00 - 121:03
    That would be 4 pi over 3.
  • 121:03 - 121:05
    And 4 pi over 3.
  • 121:05 - 121:10
    Keep in mind these things
    with imaginary numbers because
  • 121:10 - 121:14
    in 3350, they will rely on
    you knowing these things.
  • 121:14 - 121:16
  • 121:16 - 121:18
    STUDENT: Then you apply
    Euler's formula up there.
  • 121:18 - 121:21
  • 121:21 - 121:22
    MAGDALENA TODA: Oh, yeah.
  • 121:22 - 121:24
    By the way, this is
    called Euler's formula.
  • 121:24 - 121:28
  • 121:28 - 121:31
    STUDENT: In middle
    school, they teach you,
  • 121:31 - 121:34
    and they tell you when
    discriminant is small,
  • 121:34 - 121:36
    there's no solutions.
  • 121:36 - 121:37
    MAGDALENA TODA: Yeah.
  • 121:37 - 121:38
    STUDENT: And you
    go to [INAUDIBLE].
  • 121:38 - 121:40
    MAGDALENA TODA: When the
    discriminant is less than 0,
  • 121:40 - 121:42
    there are no real solutions.
  • 121:42 - 121:44
    But you have in pairs
    imaginary solutions.
  • 121:44 - 121:46
    They always come in pairs.
  • 121:46 - 121:50
  • 121:50 - 121:52
    Do you want me to
    show you probably
  • 121:52 - 121:55
    the most important problem
    in 3350 in 2 minutes,
  • 121:55 - 121:59
    and then I'll let you go?
  • 121:59 - 122:01
    STUDENT: Sure.
  • 122:01 - 122:08
    MAGDALENA TODA: So somebody
    gives you the equation
  • 122:08 - 122:10
    of the harmonic oscillator.
  • 122:10 - 122:12
    And you say, what
    the heck is that?
  • 122:12 - 122:17
    You have a little spring
    and you pull that spring.
  • 122:17 - 122:19
    And it's going to come back.
  • 122:19 - 122:22
    You displace it, it comes back.
  • 122:22 - 122:24
    It oscillates back and forth,
    oscillates back and forth.
  • 122:24 - 122:28
    If you were to write the
    solutions of the harmonic
  • 122:28 - 122:30
    oscillator in electric
    circuits, there
  • 122:30 - 122:31
    would be oscillating functions.
  • 122:31 - 122:37
    So it has to do with sine and
    cosine, so they must be trig.
  • 122:37 - 122:39
    If somebody gives
    you this equation,
  • 122:39 - 122:57
    let's say ax squared-- y
    double prime of x minus b.
  • 122:57 - 122:59
    Plus.
  • 122:59 - 123:04
    Equals to 0.
  • 123:04 - 123:09
    And here is a y equals 0.
  • 123:09 - 123:12
    Why would that
    show up like that?
  • 123:12 - 123:19
    Well, Hooke's law tells
    you that there is a force.
  • 123:19 - 123:22
    And there is a
    force and the force
  • 123:22 - 123:23
    is mass times acceleration.
  • 123:23 - 123:27
    And acceleration is like this
    type of second derivative
  • 123:27 - 123:31
    of the displacement.
  • 123:31 - 123:38
    And F and the displacement
    are proportional,
  • 123:38 - 123:41
    when you write F
    equals displacement,
  • 123:41 - 123:44
    let's call it y of x.
  • 123:44 - 123:48
    When you have y of x, x is time.
  • 123:48 - 123:49
    That's the displacement.
  • 123:49 - 123:50
    That's the force.
  • 123:50 - 123:51
    That's the k.
  • 123:51 - 123:53
    So you have a certain
    Hooke's constant.
  • 123:53 - 123:55
    Hooke's law constant.
  • 123:55 - 123:57
    So when you write
    this, Hooke's law
  • 123:57 - 123:59
    is going to become like that.
  • 123:59 - 124:05
    Mass times y double prime of
    x equals-- this is the force.
  • 124:05 - 124:07
    k times y of x.
  • 124:07 - 124:10
  • 124:10 - 124:17
    But it depends because
    you can have plus minus.
  • 124:17 - 124:19
    So you can have plus or minus.
  • 124:19 - 124:20
    And these are
    positive functions.
  • 124:20 - 124:28
  • 124:28 - 124:32
    You have two equations
    in that case.
  • 124:32 - 124:40
    One equation is the form y
    double prime plus-- give me
  • 124:40 - 124:40
    a number.
  • 124:40 - 124:43
    Cy equals 0.
  • 124:43 - 124:50
    And the other one would be y
    double prime minus cy equals 0.
  • 124:50 - 124:51
    All right.
  • 124:51 - 124:55
    Now, how hard is to
    guess your solutions?
  • 124:55 - 125:00
  • 125:00 - 125:02
    Can you guess the
    solutions with naked eyes?
  • 125:02 - 125:05
  • 125:05 - 125:06
    STUDENT: e to the x--
  • 125:06 - 125:09
  • 125:09 - 125:14
    MAGDALENA TODA: So if you have--
    you have e to the something.
  • 125:14 - 125:18
    If you didn't have a c, it
    would make your life easier.
  • 125:18 - 125:19
    Forget about the c.
  • 125:19 - 125:21
    The c will act the
    same in the end.
  • 125:21 - 125:26
    So here, what are the
    possible solutions?
  • 125:26 - 125:27
    STUDENT: e to the--
  • 125:27 - 125:29
    MAGDALENA TODA: e to the t
    is one of them. e to the x
  • 125:29 - 125:33
    is one of them, right?
  • 125:33 - 125:36
    So in the end, to
    solve such a problem
  • 125:36 - 125:37
    they teach you the method.
  • 125:37 - 125:40
    You take the equation.
  • 125:40 - 125:42
    And for that, you associate
    the so-called characteristic
  • 125:42 - 125:44
    equation.
  • 125:44 - 125:47
    For power 2, you put r squared.
  • 125:47 - 125:51
    Then you minus n for-- this
    is how many times is it prime?
  • 125:51 - 125:52
    No times.
  • 125:52 - 125:53
    0 times.
  • 125:53 - 125:55
    So you put a 1.
  • 125:55 - 125:58
    If it's prime one times,
    y prime is missing.
  • 125:58 - 126:02
    It's prime 1 time,
    you would put minus r.
  • 126:02 - 126:03
    Equals 0.
  • 126:03 - 126:07
    And then you look at
    the two roots of that.
  • 126:07 - 126:08
    And what are they?
  • 126:08 - 126:09
    Plus minus 1.
  • 126:09 - 126:11
    So r1 is 1, r2 is 2.
  • 126:11 - 126:13
    And there is a
    theorem that says--
  • 126:13 - 126:15
    STUDENT: r2 is minus 1.
  • 126:15 - 126:17
    MAGDALENA TODA: r2 is minus 1.
  • 126:17 - 126:20
    Excuse me.
  • 126:20 - 126:24
    OK, there's a theorem that
    says all the solutions
  • 126:24 - 126:28
    of this equation come as
    linear combinations of e
  • 126:28 - 126:31
    to the r1t and e to the r2t.
  • 126:31 - 126:33
    So linear combination
    means you can
  • 126:33 - 126:39
    take any number a and any
    number b, or c1 and c2, anything
  • 126:39 - 126:40
    like that.
  • 126:40 - 126:45
    So all the solutions of
    this will look like e
  • 126:45 - 126:48
    to the t with an a in
    front plus e to the minus
  • 126:48 - 126:50
    t with a b in front.
  • 126:50 - 126:53
    Could you have seen
    that with naked eye?
  • 126:53 - 126:54
    Well, yeah.
  • 126:54 - 126:57
    I mean, you are smart
    and you guessed one.
  • 126:57 - 126:59
    An you said e to
    the t satisfied.
  • 126:59 - 127:02
    Because if you put e to the
    p and prime it as many times
  • 127:02 - 127:05
    as you want, you
    still get e to the t.
  • 127:05 - 127:06
    So you get 0.
  • 127:06 - 127:09
    But nobody thought of-- or maybe
    some people thought about e
  • 127:09 - 127:10
    to the minus t.
  • 127:10 - 127:11
    STUDENT: Yeah.
  • 127:11 - 127:12
    I was about to go
    through that one.
  • 127:12 - 127:13
    MAGDALENA TODA: You were about.
  • 127:13 - 127:14
    STUDENT: That's for a selection.
  • 127:14 - 127:16
    MAGDALENA TODA: So even if
    you take e to the minus t,
  • 127:16 - 127:17
    you get the same answer.
  • 127:17 - 127:20
    And you get this thing.
  • 127:20 - 127:24
    All right, all the combinations
    will satisfy the same equation
  • 127:24 - 127:25
    as well.
  • 127:25 - 127:27
    This is a superposition
    principle.
  • 127:27 - 127:29
    With this, it was easy.
  • 127:29 - 127:32
    But this is the so-called
    harmonic oscillator equation.
  • 127:32 - 127:36
  • 127:36 - 127:40
    So either you have it simplified
    y double prime plus y equals 0,
  • 127:40 - 127:46
    or you have some constant c.
  • 127:46 - 127:49
    Well, what do you
    do in that case?
  • 127:49 - 127:51
    Let's assume you have 1.
  • 127:51 - 127:54
    Who can guess the solutions?
  • 127:54 - 127:56
    STUDENT: 0 and cosine--
  • 127:56 - 127:58
    MAGDALENA TODA: No, 0
    is the trivial solution
  • 127:58 - 127:59
    and it's not going to count.
  • 127:59 - 128:04
    You can get it from the
    combination of the--
  • 128:04 - 128:05
    STUDENT: y equals sine t.
  • 128:05 - 128:07
    MAGDALENA TODA:
    Sine t is a solution
  • 128:07 - 128:12
    because sine t prime is cosine.
  • 128:12 - 128:14
    When you prime it
    again, it's minus sine.
  • 128:14 - 128:17
    When you add sine and
    minus sine, you get 0.
  • 128:17 - 128:19
    So you just guessed
    1 and you're right.
  • 128:19 - 128:21
    Make a face.
  • 128:21 - 128:22
    Do you see another one?
  • 128:22 - 128:23
    STUDENT: Cosine t.
  • 128:23 - 128:24
    MAGDALENA TODA: Cosine.
  • 128:24 - 128:26
  • 128:26 - 128:29
    They are independent,
    linear independent.
  • 128:29 - 128:31
    And so the multitude
    of solutions
  • 128:31 - 128:34
    for that-- I taught you
    a whole chapter in 3350.
  • 128:34 - 128:37
    Now you don't have
    to take it anymore--
  • 128:37 - 128:40
    is going to be a equals sine t--
  • 128:40 - 128:41
    STUDENT: How about e to the i t?
  • 128:41 - 128:42
    MAGDALENA TODA: Plus b sine t.
  • 128:42 - 128:43
    I tell you in a second.
  • 128:43 - 128:47
    All right, we have to
    do an e to the i t.
  • 128:47 - 128:48
    OK.
  • 128:48 - 128:51
    So you guessed that all the
    solutions will be combinations
  • 128:51 - 128:56
    like-- on the monitor when you
    have cosine and sine, if you
  • 128:56 - 128:59
    add them up-- multiply
    and add them up,
  • 128:59 - 129:02
    you get something like the
    monitor thing at the hospital.
  • 129:02 - 129:04
    So any kind of
    oscillation like that
  • 129:04 - 129:08
    is a combination of this kind.
  • 129:08 - 129:13
    Maybe with some different
    phases and amplitudes.
  • 129:13 - 129:17
    You have cosine of 70 or
    cosine of 5t or something.
  • 129:17 - 129:19
    But let me show
    you what they are
  • 129:19 - 129:25
    going to show you [INAUDIBLE]
    for the harmonic oscillator
  • 129:25 - 129:27
    equation how the method goes.
  • 129:27 - 129:29
    You solve for the
    characteristic equation.
  • 129:29 - 129:35
    So you have r squared
    plus 1 equals 0.
  • 129:35 - 129:39
    Now, here's where most of
    the students in 3350 fail.
  • 129:39 - 129:40
    They understand that.
  • 129:40 - 129:44
    And some of them say, OK,
    this has no solutions.
  • 129:44 - 129:47
    Some of them even say this
    has solutions plus minus 1.
  • 129:47 - 129:49
    I mean, crazy stuff.
  • 129:49 - 129:51
    Now, what are the
    solutions of that?
  • 129:51 - 129:53
    Because the theory
    in this case says
  • 129:53 - 129:57
    if your solutions are
    imaginary, then y1
  • 129:57 - 130:01
    would be e to the ax cosine bx.
  • 130:01 - 130:05
    And y2 will be e
    to the ax sine bx
  • 130:05 - 130:09
    where your imaginary
    solutions are a plus minus ib.
  • 130:09 - 130:14
    It has a lot to do with
    Euler's formula in a way.
  • 130:14 - 130:21
    So if you knew the theory in
    3350 and not be just very smart
  • 130:21 - 130:24
    and get these by yourselves
    by guessing them,
  • 130:24 - 130:27
    how are you supposed
    to know that?
  • 130:27 - 130:31
    Well, r squared
    equals minus 1, right?
  • 130:31 - 130:34
    The square root of minus 1 is i.
  • 130:34 - 130:35
    STUDENT: Or negative.
  • 130:35 - 130:36
    MAGDALENA TODA: Or negative i.
  • 130:36 - 130:41
    So r1 is 0 plus minus i.
  • 130:41 - 130:42
    So who is a?
  • 130:42 - 130:44
    a is 0.
  • 130:44 - 130:46
    Who is b?
  • 130:46 - 130:47
    b is 1.
  • 130:47 - 130:53
    So the solutions are e to
    the 0x equal cosine 1x and e
  • 130:53 - 130:59
    to the 0x sine 1x, which
    is cosine x, sine x.
  • 130:59 - 131:03
    Now you know why you can
    do everything formalized
  • 131:03 - 131:06
    and you get all these
    solutions from a method.
  • 131:06 - 131:10
    This method is an
    entire chapter.
  • 131:10 - 131:12
    It's so much easier than in 350.
  • 131:12 - 131:15
    So much easier than Calculus 3.
  • 131:15 - 131:16
    You will say this is easy.
  • 131:16 - 131:18
    It's a pleasure.
  • 131:18 - 131:23
    You spend about one
    fourth of the semester
  • 131:23 - 131:25
    just on this method.
  • 131:25 - 131:26
    So now you don't have
    to take it anymore.
  • 131:26 - 131:29
    You can learn it all by
    yourself and you're going
  • 131:29 - 131:33
    to be ready for the next thing.
  • 131:33 - 131:35
    So I'm just giving you courage.
  • 131:35 - 131:40
    If you do really, really well in
    Calc 3, 3350 will be a breeze.
  • 131:40 - 131:42
    You can breeze through that.
  • 131:42 - 131:46
    You only have the probability
    in stats for most engineers
  • 131:46 - 131:49
    to take.
  • 131:49 - 131:54
    Math is not so complicated.
Title:
TTU Math2450 Calculus3 Sec 13.3
Description:

Conservative vector fields

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