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TTU Math2450 Calculus3 Secs 12.6 - 12.7

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    MAGDALENA TODA: Midterm
    covers the following sections.
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    Chapter 9, no-- that
    was practically--
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    that is review, mostly review.
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    10.1, 10.2, 10.4, and
    what I'm writing down
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    will be the same section
    covered in the final.
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    11.1 through 11.8, all of them.
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    11.8 is LaGrange multipliers.
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    That may or may not be
    on the actual midterm,
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    but it's included in
    the [? midterm. ?]
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    12.1 through 12.5, all of them.
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    Skip 12.6 as you know.
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    And 12.7 will be covered
    today-- will be covered today--
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    in the classroom
    after the review
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    because today is the
    long day with all three
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    hours [INAUDIBLE].
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    We have almost
    three hours today.
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    [? Just do that on ?] the
    midterm, and then I'll
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    move onto 12.7.
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    12.7 is the last required
    section in chapter 12.
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    And then there is nothing else
    for Chapter 13 and that's it.
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    12.7, you will see it's called
    cylindrical and spherical
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    coordinates.
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    And you use these
    type of coordinates
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    for triple integrals--
    for triple integrals.
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    Everything is in 3D, three
    dimensional Euclidean stuff.
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    All right.
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    Is it clear?
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    So I'm going to start
    with the specification.
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    [INAUDIBLE] and portable
    electronic devices of all sorts
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    are not allowed during
    the examination.
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    No calculator, no pagers,
    no cellphones open.
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    Taking this exam is subjected to
    the existing rules [INAUDIBLE]
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    regarding academic honesty.
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    So don't attempt cheating,
    looking at the notes,
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    talking to other
    people during the exam.
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    That's not going to be allowed.
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    Write in the spaces provided
    under every problem.
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    No additional papers
    have to be turned in.
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    When you'll actually
    get the exam,
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    it's going to be typed a little
    bit larger so you will have
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    spaces between the problems.
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    In those spaces, you
    will be able to write.
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    The answers are really short.
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    You'll be surprised
    how short they will be.
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    On top of those two
    pages, there will
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    be a third page which is blank.
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    In that third blank page, you
    can scribble your computations.
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    You will not have many
    computations to scribble,
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    but the space provided
    should be practically enough
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    for you to write your answers.
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    Two or three of
    those 10 problems
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    will have multiple
    choice answers.
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    So you're going to
    ask me, what do I
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    expect about that
    multiple choice answer?
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    I will tell you in
    a second and I'm
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    going to also give
    you an example.
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    So I'm just expecting some
    circling some numerical answer
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    that you have [INAUDIBLE].
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    And I'll tell you in the context
    of this sample what those are.
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    Who's missing the midterm?
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    Come and pick it up, please.
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    And would you distribute
    this to the others?
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    [INAUDIBLE]
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    All right.
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    Number 1, write the
    total differential
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    of the following function.
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    You will have something like
    that for a different function.
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    But you will have to do
    the total differential.
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    And remember the
    total differential
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    is not a sum or
    partial derivative.
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    So if you want to
    kill me, say that.
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    You're going to get a
    big 0 on that, right,
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    but you're also going to
    kill me in the process.
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    So what was the
    total differential
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    in the function
    of two variables?
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    Now you know it.
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    You can help me write it down.
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    STUDENT: Partial derivative
    in the x direction
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    dx [? plus 1. ?]
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    MAGDALENA TODA: And that's
    an infinitesimal element.
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    If you skip that, everything
    you write is nonsense.
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    So pay attention that this
    part, the whole combination
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    of scalar real value functions
    and infinitesimal elements
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    would be good.
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    So what is the answer
    for my problem here
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    if f is-- what's your problem?
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    Let's see, what's your problem?
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    Cosine of xy.
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    And I'm going to
    do this in lime.
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    I hope it's visible
    enough for the video.
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    What's the derivative with
    respect to x of cosine of xy?
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    STUDENT: Negative y sine xy.
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    MAGDALENA TODA:
    Negative y sine xy.
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    So pay attention
    to the chain rule.
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    You'll have to remember
    that the derivative
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    of this function with respect to
    x assumes that y is a constant.
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    So when you differentiate
    xy with respect to xy,
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    it remains [INAUDIBLE]
    of the product.
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    All right.
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    dx, [INAUDIBLE] and say dx
    plus the infinitesimal element
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    [? dx ?] plus-- what next?
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    The same thing.
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    It's a symmetric polynomial.
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    But exactly like
    Aaron said, now I'm
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    going to have minus x sine xy.
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    So the same kind of policy.
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    You've seen this
    before on homework.
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    Guys, I don't like
    surprises on the exam,
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    so what I picked for the
    midterm-- and you will see also
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    the final will be
    in the same screen--
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    it is out of those 200
    problems, whatever you
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    have covered in the homework.
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    We don't give you new
    stuff, stuff that you
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    haven't seen in the homework.
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    All right.
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    So with this, your
    answer is ready.
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    You have one or two rows are
    enough for you to write down
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    the answer for that.
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    Actually, one line
    would be enough.
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    Do I expect more than this line?
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    Take one from the
    desk, [INAUDIBLE].
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    So do I expect more than
    this answer under problem 1?
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    No.
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    You either know it
    or you don't know it.
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    If you know the definition,
    you don't have to repeat it.
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    If you know how to
    differentiate, you're fine.
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    You're in business.
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    You've got a perfect score on
    this first problem out of 10.
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    They are not time consuming.
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    I don't like exams that
    are time consuming.
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    They are not testing anything.
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    So I want to walk you
    through the material
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    through many questions so
    that I see what you understood
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    and what concepts
    are well understood
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    and which ones are not.
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    OK.
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    All right.
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    Let's move on to number two.
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    That was number 1.
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    Number 2.
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    Number 2 says find the
    directional derivative
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    of a function f of xy, which
    is equal to cosine of xy.
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    What do you see?
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    I have already prepared
    you for this problem
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    because it's the same
    function as before.
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    You have computed f sub
    x and f sub y already.
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    That should be
    helpful when you write
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    the directional derivative.
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    In the direction--
    and by direction,
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    we mean unit vector-- direction
    of something means unit vector.
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    What direction do they say
    the highest [? ascent? ?]
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    So this problem is walking you
    through the whole chapter 11
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    by testing what you understood.
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    So what is the direction
    of the highest [? ascent ?]
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    for a function like that?
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    STUDENT: The gradient
    of the [INAUDIBLE].
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    MAGDALENA TODA: The gradient.
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    So if you know what the
    direction of the gradient
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    is [INAUDIBLE], at the
    point p of coordinate 0, 0--
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    so p is the point at 0, 0--
    if such a direction exists,
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    can you say-- well
    of course it exists.
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    It's a gradient.
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    Justify your answer.
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    All right.
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    So when would it not exists?
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    STUDENT: If there's no
    direction of highest decent.
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    MAGDALENA TODA: Right.
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    STUDENT: All of
    them are the same.
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    MAGDALENA TODA: Right.
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    All right.
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    So what would you
    have to write in terms
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    of directional derivative
    for an arbitrary function?
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    What do you know about the
    [? directional ?] derivative
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    of a function at the point in
    the direction of a vector u?
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    You can write the
    definition with limit.
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    That's going to be an
    expression like that eating up
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    all your space, but
    that's not what I mean.
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    I mean that you'll have
    to know the theorem that
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    says this is partial
    derivative with respect
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    to x measure that
    the point p times u1
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    plus partial derivative
    with respect to y
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    measured at the point
    p times u2 where
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    u1 and u2 are the components
    of your unit vector
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    that we talked about before.
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    Now, when I compute
    f sub x and p,
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    I have to say oh, I
    know where sub x is.
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    But if I compute it at
    p and p is 0, 0, my god,
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    this is going to be 0, right?
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    And if I do f sub
    y at p and p is 0,
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    well, you also know that the
    second partial derivative is 0.
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    So at 0, this is
    going to be 0 as well.
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    So the directional
    derivative is 0.
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    Did I have to find the
    direction of the gradient?
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    No, because in the
    end, you got 0.
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    So it's always
    important to write down
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    the final thing you
    want, the definition
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    of the directional derivative.
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    In the actual exam, you may
    have a different situation.
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    So let's work on alternative
    one, alternative problem
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    like that.
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    I'll pick an easy f of x and y.
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    All of the examples would
    be [INAUDIBLE] numerically,
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    computationally.
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    The [? point ?] components
    [? 1,1 ?] in the [INAUDIBLE].
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    Do the same problem for
    this different data.
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    Who will be u?
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    u will be the direction
    of the gradient.
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    If I'm talking about the
    direction of the highest
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    asset for-- or highest
    asset direction,
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    Sometimes I may give
    you that direction,
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    and it doesn't have to be
    the highest asset direction.
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    But in this case, it has to
    be because the problems are
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    solved.
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    So you have to say, what
    is the gradient in my case?
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    Well, piece of cake.
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    That's going to be 1 times
    i plus 1 times j divided
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    by square root of 2.
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    So u1 is 1 over root
    2, u2 is 1 over root 2.
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    And can I write [? this view ?]
    in such an alternative problem,
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    ah, it should be easy.
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    Well, it is easy.
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    The first number will
    be 1 because that's
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    the derivative with respect
    to x times u1, 1 over root 2
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    plus the derivative with
    respect to y, 1, times u2 1
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    over root 2.
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    Only now do you
    leave it like this.
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    Or you leave it like
    that and you get 100%.
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    I really don't care.
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    But what if the
    problem is formulated
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    as a multiple choice?
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    It will be formulated as
    multiple choice with A, B,
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    C choices like that, we'll
    never write it-- well,
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    if we are normal people, we'll
    never write it like that.
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    So what do you think the
    answer, the correct answer,
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    out of those possible
    answers will be in this case?
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    One answer will be 0, one
    answer will be 2, one answer--
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    STUDENT: Root 2.2
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    MAGDALENA TODA: Root 2.
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    So what are you supposed to do?
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    Just go to the answer
    [INAUDIBLE] circle it.
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    Do you have to show anyone?
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    No.
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    But you only have, like, two
    such multiple choice problems.
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    Everything else is show work.
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    All right.
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    Yes, sir.
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    STUDENT: How can a
    problem change because
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    of the steepest descent?
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    MAGDALENA TODA: The
    steepest descent
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    will happen in the opposite
    direction of the gradient.
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    So it's going to happen exactly
    in the direction minus i,
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    minus j over root 2.
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    And if you compute the
    directional derivative
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    in that direction, you're going
    to have exactly the opposite
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    of that minus root 2.
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    All right.
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    STUDENT: It says
    justify your answer.
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    How would you write that?
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    MAGDALENA TODA: Oh.
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    Justify your answer.
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    Let me justify the
    answer [INAUDIBLE] here.
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    The steepest ascent takes
    place in the direction u
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    corresponding to the gradient.
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    Delta f formula [? au ?]
    bar f of p formula
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    above means the theorem
    that was from chapter 11.
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    You don't have to
    know which theorem,
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    but you just write down
    this [? was a ?] theorem.
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    You plugged in, you
    got 0 for your example.
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    For the actual midterm,
    it may be different.
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    The same kind of
    problem, absolutely.
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    So you have to say--
    justify your answer.
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    I may or may not say justify
    your answer in the end,
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    but you have to
    know this anyway.
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    You have to know
    this part anyway.
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    You have to know
    this formula anyway.
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    So justification means
    showing the formula in itself
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    and explaining that the
    steepest ascent take place
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    in the direction
    of the gradient.
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    All right.
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    OK.
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    Number 2.
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    Number 3.
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    They're all related.
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    They're all the
    same [? constant ?].
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    So I'm going to go ahead
    and erase this part.
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    And it says find number three.
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    For the function f of
    x equals cosine of xy,
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    as if we never saw that
    before, find the gradient.
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    What are you supposed to
    write on such a problem
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    to justify your answer?
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    And also, it says
    write parenthesis
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    specify the equation of the
    tangent plane to the graph z
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    equals f of xy at
    the point-- I forgot
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    the word at-- at the point
    a of coordinate 0, 0, 1.
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    All right.
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    So let's say-- this
    problem has two parts,
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    but they shouldn't be long.
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    Number 3 says what?
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    Find me the gradient
    of this function.
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    What are you supposed to write?
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    You have two alternatives here.
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    Either you write f sub xi plus
    f sub yj equals minus y sine xy
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    i minus x sine xy j.
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    Or this is up to you.
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    This is how I would
    write the gradient.
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    Some people prefer to
    forget the x and y.
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    They don't write the
    gradient in standard basis.
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    They're assuming it
    is the standard basis
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    and they only write
    the coordinates.
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    In angular brackets,
    assume with respect
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    to the standard basis,
    canonical basis.
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    Whichever you want is fine.
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    Are you guys with me?
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    Any questions?
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    All right.
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    Is this hard?
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    No.
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    Let's see how hard
    is the next one.
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    What do you think I have to do?
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    I'm waiting for your input.
  • 18:09 - 18:12
    [? Write, ?]
    parenthesis, specify
  • 18:12 - 18:16
    the equation of the tangent
    plane to the graph z
  • 18:16 - 18:17
    equals f of xy.
  • 18:17 - 18:20
    That graph is going to be the
    graph of a surface, right?
  • 18:20 - 18:23
    z equals f of x sub y.
  • 18:23 - 18:27
    We want the equation
    of the tangent plane
  • 18:27 - 18:30
    to the graph at
    the point 0, 0, 1,
  • 18:30 - 18:35
    which means I have to take
    x, 0 to be 0, y, 0 to be 0.
  • 18:35 - 18:41
    And consequently, z, 0 will
    be cosine of 0, which is 1.
  • 18:41 - 18:47
    So it makes sense that
    point p is on the graph.
  • 18:47 - 18:50
    Or a is on the graph, a.
  • 18:50 - 18:52
    [INAUDIBLE]
  • 18:52 - 18:54
    Good.
  • 18:54 - 18:57
    At least I know I didn't
    make a mistake about that.
  • 18:57 - 19:04
    How do we write
    the tangent plane
  • 19:04 - 19:12
    when someone gives us the
    explicit equation of the graph?
  • 19:12 - 19:15
    z equals f of xy.
  • 19:15 - 19:18
    Knowing that f is a function,
    how is this function?
  • 19:18 - 19:19
    Well look at it.
  • 19:19 - 19:20
    It's z infinity.
  • 19:20 - 19:24
    It has differentiable
    infinitely many times,
  • 19:24 - 19:26
    and all the derivatives
    are continuous.
  • 19:26 - 19:28
    So we are really
    lucky we don't have
  • 19:28 - 19:30
    any headaches in this case.
  • 19:30 - 19:32
    [INAUDIBLE] both
    partial derivatives
  • 19:32 - 19:34
    existed that are
    continuous, I'm going
  • 19:34 - 19:37
    to write down the equation
    of the tangent [INAUDIBLE].
  • 19:37 - 19:39
    But not by myself.
  • 19:39 - 19:42
    With your help because
    it's been a long time.
  • 19:42 - 19:47
    But you are not allowed
    to forget the formula.
  • 19:47 - 19:52
    What was the general formula for
    the tangent plane in this case?
  • 19:52 - 19:52
    [INAUDIBLE]
  • 19:52 - 19:55
  • 19:55 - 19:58
    And I'll try to
    keep my mouth shut.
  • 19:58 - 19:59
    z--
  • 19:59 - 20:00
    STUDENT: Minus z0.
  • 20:00 - 20:03
    MAGDALENA TODA: Minus z0.
  • 20:03 - 20:05
    Remember the linear
    approximation
  • 20:05 - 20:09
    via the surface, the current
    surface, with the plane.
  • 20:09 - 20:11
    That's the linear approximation.
  • 20:11 - 20:12
    STUDENT: x with
    respect [INAUDIBLE].
  • 20:12 - 20:14
    MAGDALENA TODA: That's right.
  • 20:14 - 20:19
    I want to say with respect to
    [INAUDIBLE] x and y at 0, 0--
  • 20:19 - 20:23
    good, we'll do that
    later-- times--
  • 20:23 - 20:24
    STUDENT: x minus x0.
  • 20:24 - 20:27
    MAGDALENA TODA:
    --x minus x0 plus--
  • 20:27 - 20:27
    STUDENT: f sub y.
  • 20:27 - 20:32
    MAGDALENA TODA: f
    sub y at 0, 0 times--
  • 20:32 - 20:33
    STUDENT: y minus y0.
  • 20:33 - 20:35
    MAGDALENA TODA: y minus y0.
  • 20:35 - 20:41
    But again, x0 is 0.
    y0 is 0. z0 is 1.
  • 20:41 - 20:44
    Now, we know more than
    that because I gave you
  • 20:44 - 20:45
    a problem that's too easy.
  • 20:45 - 20:49
    [INAUDIBLE] trying to
    do something impossible.
  • 20:49 - 20:53
    f sub x at 0, 0, we
    already computed that.
  • 20:53 - 20:56
    And we noticed
    that was 0 and this
  • 20:56 - 21:02
    was-- so we are exceedingly
    lucky in this case.
  • 21:02 - 21:05
    Not all the problems
    are so beautiful.
  • 21:05 - 21:07
    The problems that
    we give in the exam
  • 21:07 - 21:10
    generally are more beautiful
    than all the problems
  • 21:10 - 21:12
    that happen in
    reality, real life.
  • 21:12 - 21:16
    z equals 1 will be your
    answer in this case.
  • 21:16 - 21:18
    What is z equals 1?
  • 21:18 - 21:24
    It's the horizontal plane
    that z equals [? 1. ?] So
  • 21:24 - 21:27
    that will be the [INAUDIBLE].
  • 21:27 - 21:28
    And you're done.
  • 21:28 - 21:33
    You have problem--
    what problem was that?
  • 21:33 - 21:35
    Problem 3 finished.
  • 21:35 - 21:38
    They are short and they
    are, again, [INAUDIBLE]
  • 21:38 - 21:41
    the ones on Thursday.
  • 21:41 - 21:42
    Next Thursday,
    not this Thursday.
  • 21:42 - 21:46
    It will be very easy to solve.
  • 21:46 - 21:49
    I'm just testing
    you on the concepts,
  • 21:49 - 21:54
    see what do you remember
    from the concepts.
  • 21:54 - 21:59
    So now you know that
    write a note to yourself.
  • 21:59 - 22:03
    So she expects me to know the
    equation of the tangent plane
  • 22:03 - 22:07
    for both the midterm and
    for the final by heart.
  • 22:07 - 22:08
    Yes, I do.
  • 22:08 - 22:10
    And I think compared to
    other things that you
  • 22:10 - 22:14
    have to learn, memorize for
    your engineering courses,
  • 22:14 - 22:16
    this is a piece of cake.
  • 22:16 - 22:19
    You only have a few things
    that you have to memorize.
  • 22:19 - 22:21
    Very few things you
    have to memorize.
  • 22:21 - 22:22
    All right.
  • 22:22 - 22:27
    Number 4, find the direction
    in which the function--
  • 22:27 - 22:30
    I'm changing the
    function, finally.
  • 22:30 - 22:35
    I say function x
    plus y increases
  • 22:35 - 22:39
    most rapidly at the
    point p of 1, 1.
  • 22:39 - 22:44
    Or in which direction is
    this function increasing
  • 22:44 - 22:47
    most rapidly at 1, 1?
  • 22:47 - 22:57
    In which direction
    is this function
  • 22:57 - 23:11
    increasing most rapidly at 1, 1.
  • 23:11 - 23:14
    That means that the 0
    equals 1, 1, [? 0 ?].
  • 23:14 - 23:17
    We've done these kind
    of things before.
  • 23:17 - 23:19
    We know the direction
    will be the direction
  • 23:19 - 23:22
    corresponding to that gradient.
  • 23:22 - 23:27
    But the tension, when I say
    direction, what do I mean?
  • 23:27 - 23:28
    Normalize it.
  • 23:28 - 23:29
    OK.
  • 23:29 - 23:29
    All right.
  • 23:29 - 23:40
    So gradient of f at 1, 1 will
    be 1 times i plus 1 times j.
  • 23:40 - 23:43
    I'm not allowed to
    leave it like this.
  • 23:43 - 23:48
    I would say the answer
    is u equals gradient
  • 23:48 - 23:51
    of f over normal
    gradient of f, which
  • 23:51 - 23:57
    is i plus j over square root of
    2, which is the same as writing
  • 23:57 - 24:01
    1 over 2, 1 over root 2.
  • 24:01 - 24:02
    And that's it.
  • 24:02 - 24:08
  • 24:08 - 24:13
    So if x is this axis
    and y is this other one,
  • 24:13 - 24:17
    I'm modeling it with my hands.
  • 24:17 - 24:22
    The direction I'm talking
    about is the first [INAUDIBLE]
  • 24:22 - 24:25
    of this quadrant.
  • 24:25 - 24:34
    [INAUDIBLE] If I'd done
    steepest as a steepest descent,
  • 24:34 - 24:36
    it's going to be in
    the opposite direction.
  • 24:36 - 24:41
  • 24:41 - 24:46
    I'm going to go
    ahead and erase-- I
  • 24:46 - 24:48
    don't have [INAUDIBLE] number.
  • 24:48 - 24:51
  • 24:51 - 24:51
    All right.
  • 24:51 - 24:54
    Is it the same problem?
  • 24:54 - 24:55
    Yes.
  • 24:55 - 25:00
    So let's keep this on the
    board and [? find ?] what is
  • 25:00 - 25:04
    the maximal rate of change of
    the function f of xy equals x
  • 25:04 - 25:09
    plus y at the point
    [? p, 1,1. ?] That is another
  • 25:09 - 25:10
    theorem.
  • 25:10 - 25:14
    So how do I justify my
    answer in this case?
  • 25:14 - 25:20
    There is another theorem that
    says the maximum rate of change
  • 25:20 - 25:23
    will be the
    directional derivative.
  • 25:23 - 25:33
    So the maximum
    rate of change will
  • 25:33 - 25:47
    be the directional
    derivative of f
  • 25:47 - 26:01
    in the direction u of
    the gradient lambda
  • 26:01 - 26:03
    f at the point p.
  • 26:03 - 26:07
  • 26:07 - 26:12
    This is what I would
    have done as a student
  • 26:12 - 26:16
    because I think I would
    have remembered only
  • 26:16 - 26:24
    the theorem without
    remembering that this
  • 26:24 - 26:30
    is the same time, the
    same thing, as what?
  • 26:30 - 26:35
    The length of the
    radian at that point.
  • 26:35 - 26:38
    I think I would've
    forgotten that because I'm
  • 26:38 - 26:42
    trying to remember who I
    was more than 20 years ago
  • 26:42 - 26:46
    and see how I would have
    answered this question.
  • 26:46 - 26:51
    Now, I think I would've
    gotten to the same answer.
  • 26:51 - 26:55
    Nevertheless, I would have
    struggled a little bit
  • 26:55 - 26:59
    and I would've thought just
    in the middle of the exam,
  • 26:59 - 27:01
    why in the world is that?
  • 27:01 - 27:05
    Because I always find myself
    not remembering things
  • 27:05 - 27:09
    in the exams, and I would
    try to remember why is that?
  • 27:09 - 27:12
    So by the way, why is that?
  • 27:12 - 27:15
    The directional derivative
    in the direction
  • 27:15 - 27:21
    of u of f at the point
    p also was returned.
  • 27:21 - 27:25
    I wrote it it down
    before f sub x u1 plus f
  • 27:25 - 27:29
    sub y u2 where you guys
    told me what that was.
  • 27:29 - 27:35
    That was a certain scalar
    product, or dot product,
  • 27:35 - 27:40
    between the direction of the
    gradient and the vector u.
  • 27:40 - 27:43
    And I was grateful you told me
    that that was a long time ago,
  • 27:43 - 27:47
    or it was two weeks, three
    weeks ago, something like that.
  • 27:47 - 27:50
    So we noted together
    that it's the same thing
  • 27:50 - 27:53
    if you write [INAUDIBLE] f
    gradient [INAUDIBLE] product
  • 27:53 - 27:56
    with u.
  • 27:56 - 28:01
    But if u itself is gradient
    of f, well, over the length,
  • 28:01 - 28:03
    let's write it down.
  • 28:03 - 28:05
    If I'm talking
    highest ascent, then
  • 28:05 - 28:11
    u itself is the gradient
    of f over the form,
  • 28:11 - 28:14
    the lengths of the gradient.
  • 28:14 - 28:17
    So what is the answer?
  • 28:17 - 28:21
    That is-- [INAUDIBLE].
  • 28:21 - 28:25
    It would be exactly
    the square of the norm,
  • 28:25 - 28:29
    the square of the length,
    divided by the length.
  • 28:29 - 28:34
    So I proved again, because
    I'm forgetful and I'm silly,
  • 28:34 - 28:39
    I put again that this
    maximum rate of change
  • 28:39 - 28:45
    is exactly the length
    of the gradient.
  • 28:45 - 28:47
    For somebody who
    is better than me
  • 28:47 - 28:50
    when it comes to
    memorizing things,
  • 28:50 - 28:52
    they wouldn't have
    had to do that.
  • 28:52 - 28:54
    I'm just doing review.
  • 28:54 - 28:57
    So what was expected from
    you if you studied and you're
  • 28:57 - 29:00
    a good student.
  • 29:00 - 29:02
    We expected only
    that you would write.
  • 29:02 - 29:05
  • 29:05 - 29:13
    The answer would
    be-- which is what?
  • 29:13 - 29:15
    Who's telling me what this is?
  • 29:15 - 29:16
    STUDENT: The square root of 2.
  • 29:16 - 29:17
    MAGDALENA TODA: The
    square root of 2.
  • 29:17 - 29:17
    Piece of cake.
  • 29:17 - 29:20
    So it depends on how
    much you remember,
  • 29:20 - 29:23
    how much you understood
    from the material,
  • 29:23 - 29:28
    and also a little bit of
    memorization, yes, helps.
  • 29:28 - 29:30
    If you're not able
    to memorize, you
  • 29:30 - 29:32
    can always come up to
    the right conclusion,
  • 29:32 - 29:35
    but it takes forever
    and you don't
  • 29:35 - 29:39
    have time, 1 hour and 20 minutes
    or whatever that is, 1 hour 20
  • 29:39 - 29:44
    minutes to [? see ?] too much.
  • 29:44 - 29:44
    OK.
  • 29:44 - 29:47
    I'm going to erase--
    what should I erase?
  • 29:47 - 29:50
    Number 4, maybe I should erase.
  • 29:50 - 29:51
    And--
  • 29:51 - 29:53
  • 29:53 - 29:54
    STUDENT: [INAUDIBLE],
    I was going
  • 29:54 - 29:56
    to ask you about number 4.
  • 29:56 - 29:56
    MAGDALENA TODA: Huh?
  • 29:56 - 29:58
    STUDENT: On problem 6, it
    asks you about that one
  • 29:58 - 30:00
    specifically?
  • 30:00 - 30:02
    MAGDALENA TODA: And
    number 5 is asking you--
  • 30:02 - 30:04
    STUDENT: We just did number 5.
  • 30:04 - 30:05
    MAGDALENA TODA: Yeah.
  • 30:05 - 30:06
    And the answer is root 2.
  • 30:06 - 30:07
    And number 4--
  • 30:07 - 30:10
    STUDENT: It pretty much just
    asks you about that direction.
  • 30:10 - 30:12
    MAGDALENA TODA: It asks
    you about that direction.
  • 30:12 - 30:14
    That's what you have to print
    on the exam [INAUDIBLE].
  • 30:14 - 30:17
  • 30:17 - 30:21
    So again, the actual
    exam may ask you
  • 30:21 - 30:25
    to do this by printing it out.
  • 30:25 - 30:28
    Which of those following
    numbers will represent
  • 30:28 - 30:30
    the maximum rate of change?
  • 30:30 - 30:36
    0, 1, the square root of
    2, 792, stuff like that.
  • 30:36 - 30:41
    So you would have to
    circle root 2 in this case.
  • 30:41 - 30:42
    STUDENT: [INAUDIBLE].
  • 30:42 - 30:43
    MAGDALENA TODA: What?
  • 30:43 - 30:43
    STUDENT: I'm saying
    you might not
  • 30:43 - 30:46
    want to erase number 4
    because I was about to ask you
  • 30:46 - 30:46
    about number 4.
  • 30:46 - 30:48
    MAGDALENA TODA: Oh my God.
  • 30:48 - 30:51
    You are deeper than me.
  • 30:51 - 30:54
    OK.
  • 30:54 - 30:57
    Is the direction that you
    found that point for unique
  • 30:57 - 30:59
    for the given point?
  • 30:59 - 31:00
    Yes or no?
  • 31:00 - 31:03
  • 31:03 - 31:07
    What do you think?
  • 31:07 - 31:08
    Well, OK.
  • 31:08 - 31:10
    By direction, we mean what?
  • 31:10 - 31:13
    Not all the colinear vectors
    that go in that direction,
  • 31:13 - 31:23
    but the actual uniquely
    defined number as that, right?
  • 31:23 - 31:28
    So you can write an essay
    based on the uniqueness
  • 31:28 - 31:29
    of that [INAUDIBLE].
  • 31:29 - 31:32
    Let's just say the
    direction is this.
  • 31:32 - 31:37
    Some people use direction
    in other courses,
  • 31:37 - 31:38
    like linear algebra.
  • 31:38 - 31:42
    In linear algebra, you will
    see they say 1, 1, 1 direction.
  • 31:42 - 31:44
    2, 2, 2 is the same direction.
  • 31:44 - 31:46
    3, 3, 3 is the same direction.
  • 31:46 - 31:49
    But I thought you mean
    that restrictive case
  • 31:49 - 31:52
    of this course, my
    direction will mean that.
  • 31:52 - 31:54
    So it's 0.
  • 31:54 - 31:54
    All right.
  • 31:54 - 31:56
    What else do we have here?
  • 31:56 - 31:59
  • 31:59 - 32:00
    STUDENT: I have a
    question about that.
  • 32:00 - 32:01
    MAGDALENA TODA: Huh?
  • 32:01 - 32:02
    STUDENT: Why would
    that be unique
  • 32:02 - 32:05
    if it really doesn't
    matter what the point is
  • 32:05 - 32:07
    if you're going to get that?
  • 32:07 - 32:08
    MAGDALENA TODA:
    For a given point.
  • 32:08 - 32:12
    So once somebody gave
    you a given point in 0,
  • 32:12 - 32:17
    y0, you have only
    one answer, which
  • 32:17 - 32:24
    is f sub x and x0,
    y0, f sub y at x0,
  • 32:24 - 32:29
    y0 in angular brackets
    divided by-- I'm
  • 32:29 - 32:32
    too lazy to write
    it down, but I will.
  • 32:32 - 32:36
    This is the answer.
  • 32:36 - 32:40
    So somebody [? got ?],
    gave you a point x0, y0.
  • 32:40 - 32:41
    And it asks you--
    and a function.
  • 32:41 - 32:42
    A point and a function.
  • 32:42 - 32:46
    And the point is on the
    graph of the function.
  • 32:46 - 32:48
    It asks you what is that
    direction? [INAUDIBLE].
  • 32:48 - 32:51
  • 32:51 - 32:54
    So again, in other
    classes, you will
  • 32:54 - 32:57
    see people who say, well,
    after changing orientation,
  • 32:57 - 33:01
    I can go back to Amarillo
    if I was driving this way.
  • 33:01 - 33:02
    It's the same direction.
  • 33:02 - 33:03
    For us, no.
  • 33:03 - 33:07
    So for us, that is exactly
    the opposite direction.
  • 33:07 - 33:12
  • 33:12 - 33:12
    Compute the volume.
  • 33:12 - 33:18
    Now, you like this one and I
    know you remember it very well.
  • 33:18 - 33:21
  • 33:21 - 33:24
    If you don't like
    this kind of question,
  • 33:24 - 33:27
    I can switch to another one.
  • 33:27 - 33:29
    But all the questions
    should be easy.
  • 33:29 - 33:30
    STUDENT: [INAUDIBLE].
  • 33:30 - 33:31
    MAGDALENA TODA: Yes, ma'am.
  • 33:31 - 33:35
    STUDENT: I don't
    understand why number 6 is
  • 33:35 - 33:36
    unique at that point.
  • 33:36 - 33:38
    Isn't the gradient the
    same at every other point
  • 33:38 - 33:43
    since the derivatives of f of
    x-- or since f of x and f of y
  • 33:43 - 33:46
    don't have x's and y's in them.
  • 33:46 - 33:48
    They're both 1.
  • 33:48 - 33:50
    So is it not the same
    for the entire graph,
  • 33:50 - 33:54
    but at a different point?
  • 33:54 - 33:56
    MAGDALENA TODA: No.
  • 33:56 - 33:59
    If you take another point--
    OK, let's take this one, right.
  • 33:59 - 34:01
  • 34:01 - 34:02
    STUDENT: Isn't it
    asking specifically
  • 34:02 - 34:04
    for the graph of x plus y?
  • 34:04 - 34:08
    MAGDALENA TODA: Specifically
    for the graph of x plus y.
  • 34:08 - 34:09
    [INAUDIBLE]
  • 34:09 - 34:11
    What is that direction for here?
  • 34:11 - 34:14
    i plus j over square root of 2.
  • 34:14 - 34:16
  • 34:16 - 34:18
    That's unique.
  • 34:18 - 34:18
    STUDENT: OK.
  • 34:18 - 34:20
    So it's not asking
    for the point.
  • 34:20 - 34:22
    It's asking for the function.
  • 34:22 - 34:24
    MAGDALENA TODA: At
    the given point.
  • 34:24 - 34:29
    So let me eliminate--
    this is too philosophical.
  • 34:29 - 34:32
    But it says, unique
    for the given point
  • 34:32 - 34:36
    because the point is
    still given as 1, 1.
  • 34:36 - 34:39
    For that given point 1, 1
    the direction is unique.
  • 34:39 - 34:41
    In the sense, this
    is exactly what
  • 34:41 - 34:44
    I wanted to emphasize
    that in other classes,
  • 34:44 - 34:47
    they will say the direction 1, 1
    is the same as the direction 2,
  • 34:47 - 34:49
    2 is the same as
    the direction 3,
  • 34:49 - 34:53
    3 is the same as the
    direction 1, 1, 2, 1, 1, 1, 2.
  • 34:53 - 34:56
    All the colinear vectors
    are the same direction.
  • 34:56 - 34:58
    They point in the
    same direction.
  • 34:58 - 35:01
    But in our course,
    this direction
  • 35:01 - 35:06
    is uniquely defined as the
    gradient over its norm,
  • 35:06 - 35:08
    especially to make it unique.
  • 35:08 - 35:11
    We build that especially
    to make it unique.
  • 35:11 - 35:15
    I'm pointing in your
    direction, but every arrow
  • 35:15 - 35:17
    that I'm pointing
    in your direction
  • 35:17 - 35:21
    could have any magnitude, and
    [INAUDIBLE] in everyday life
  • 35:21 - 35:26
    speaking, in physics-- ask
    anybody in physics, mechanics--
  • 35:26 - 35:29
    they will say it's the
    same direction pointing
  • 35:29 - 35:31
    towards her whether you
    call it this or that
  • 35:31 - 35:33
    or that, it's the
    same direction.
  • 35:33 - 35:35
    You are pointing in
    the same direction
  • 35:35 - 35:39
    because they consider direction
    being all the colinear vectors.
  • 35:39 - 35:44
    I consider direction only this.
  • 35:44 - 35:46
    Then [INAUDIBLE].
  • 35:46 - 35:50
    It's just-- it's not even
    a mathematical problem.
  • 35:50 - 35:52
    It's a philosophical concept
    I'm trying to make [? out ?].
  • 35:52 - 35:55
  • 35:55 - 35:59
    But now that is more
    like the homework problem
  • 35:59 - 36:02
    you had before.
  • 36:02 - 36:02
    OK.
  • 36:02 - 36:04
    This one you had
    in your homework.
  • 36:04 - 36:29
    [INAUDIBLE] the volume of the
    tetrahedron, x plus y plus z
  • 36:29 - 36:35
    equals one, situating
    the [INAUDIBLE].
  • 36:35 - 36:36
    Maybe in the actual
    exam, I'm going
  • 36:36 - 36:43
    to say let's run up the integral
    of the volume without solving
  • 36:43 - 36:45
    it, or something like that.
  • 36:45 - 36:48
    Let's do both because
    I am afraid that you're
  • 36:48 - 36:49
    going to cheat.
  • 36:49 - 36:52
    And you're welcome to
    cheat on this problem
  • 36:52 - 36:53
    as much as you want.
  • 36:53 - 36:59
    But I would like you to also
    show me the actual integral.
  • 36:59 - 37:03
    So the volume will be how much?
  • 37:03 - 37:09
    This is 1, 0, 0;
    0, 1, 0; 0, 0, 1.
  • 37:09 - 37:12
    The plane is x plus
    y plus z equals 1.
  • 37:12 - 37:13
    Am I right?
  • 37:13 - 37:15
    Did I put 1 or I
    put another number?
  • 37:15 - 37:17
    I put 1.
  • 37:17 - 37:18
    OK.
  • 37:18 - 37:20
    So you know how to
    cheat on this problem.
  • 37:20 - 37:25
    So volume means area of the base
    times the height divided by 3,
  • 37:25 - 37:30
    which is 1/2 times 1/3 is 1/6.
  • 37:30 - 37:32
    But what I'm going
    to get, I think
  • 37:32 - 37:34
    I'm going to
    rephrase the problem,
  • 37:34 - 37:39
    say set up the integral
    as in triple integral
  • 37:39 - 37:42
    with or without solving it.
  • 37:42 - 37:46
    If you show me the answer,
    you get extra credit.
  • 37:46 - 37:50
    You don't have to solve
    it by hand in this case.
  • 37:50 - 37:53
    So you guys showed
    me last time what
  • 37:53 - 38:00
    the answer was for dz, dy,
    dx order of integration.
  • 38:00 - 38:03
    And how was it, guys?
  • 38:03 - 38:05
    Mr. x is moving freely.
  • 38:05 - 38:08
    He's the only free
    man in the picture
  • 38:08 - 38:11
    because even he
    has bound limits.
  • 38:11 - 38:15
    But he's free to move
    between 0 and 1 [INAUDIBLE].
  • 38:15 - 38:22
    And then y will go
    to x plus y plus 1.
  • 38:22 - 38:29
    So y will go all the way to
    between 0 and 1 minus x, right?
  • 38:29 - 38:30
    So let me write it down.
  • 38:30 - 38:33
    0 to 1.
  • 38:33 - 38:37
    Next, 0 to--
  • 38:37 - 38:37
    STUDENT: [INAUDIBLE].
  • 38:37 - 38:39
    MAGDALENA TODA: 1 minus--
  • 38:39 - 38:41
    STUDENT: Oh, I'm sorry.
  • 38:41 - 38:42
    [INAUDIBLE]
  • 38:42 - 38:43
    MAGDALENA TODA: --x.
  • 38:43 - 38:45
    STUDENT: I thought you were
    asking about [INAUDIBLE].
  • 38:45 - 38:46
    MAGDALENA TODA: You're fine.
  • 38:46 - 38:49
    I mean, this is--
    you can change.
  • 38:49 - 38:53
    Actually one time, I think,
    last year-- maybe two years ago,
  • 38:53 - 38:55
    last year-- we said
    to the students,
  • 38:55 - 39:00
    without solving this,
    show the volume integral
  • 39:00 - 39:04
    in three different
    ways by changing
  • 39:04 - 39:06
    your order of integration.
  • 39:06 - 39:10
    So you can have dz, dy, dx.
  • 39:10 - 39:12
    Or you can have dy, dz, dx.
  • 39:12 - 39:15
    Or you can have dx, dy, dz.
  • 39:15 - 39:17
    So they have to turn
    their heads in many ways,
  • 39:17 - 39:20
    and rotate, and see how it is.
  • 39:20 - 39:23
    But it's a nice problem because
    it's very easy to figure out
  • 39:23 - 39:25
    what the endpoints are.
  • 39:25 - 39:28
    The last endpoint-- actually,
    the first endpoint if you think
  • 39:28 - 39:31
    of integration-- 0 to--
  • 39:31 - 39:32
    STUDENT: 1 minus y.
  • 39:32 - 39:36
    MAGDALENA TODA: --1 minus x
    minus y because you see Mr. z,
  • 39:36 - 39:40
    Mr. z goes up like a helium
    balloon from the floor
  • 39:40 - 39:42
    and he hits his head here.
  • 39:42 - 39:47
    And he says, I hit my head there
    because I'm between 0 and 1
  • 39:47 - 39:48
    minus x minus y.
  • 39:48 - 39:52
    And that's the
    upper bound for z.
  • 39:52 - 39:53
    And you're done.
  • 39:53 - 39:56
    And that's what I
    would-- the problem
  • 39:56 - 39:57
    would be the same problem.
  • 39:57 - 39:59
    Well, maybe a problem like that.
  • 39:59 - 40:00
    But not hard.
  • 40:00 - 40:05
  • 40:05 - 40:07
    Number-- what was that?
  • 40:07 - 40:09
    STUDENT: 7.
  • 40:09 - 40:10
    MAGDALENA TODA: Thank you.
  • 40:10 - 40:18
  • 40:18 - 40:19
    Yes.
  • 40:19 - 40:23
    STUDENT: Can you change the
    order of dx, dy, and dz?
  • 40:23 - 40:26
    MAGDALENA TODA: Yes
    OK, let's do one.
  • 40:26 - 40:28
  • 40:28 - 40:30
    Of course I can, but
    do you want to see?
  • 40:30 - 40:31
    STUDENT: Yeah.
  • 40:31 - 40:32
    I want to see, please.
  • 40:32 - 40:36
    MAGDALENA TODA: 1,
    dx-- whatever I want.
  • 40:36 - 40:39
    I can do whatever.
    dz, dy or dy, dz?
  • 40:39 - 40:39
    STUDENT: dy, dz.
  • 40:39 - 40:42
    MAGDALENA TODA: dy, dz.
  • 40:42 - 40:43
    So z is still between 0 and 1.
  • 40:43 - 40:49
    He is the guy to start with.
  • 40:49 - 40:50
    So what do you think?
  • 40:50 - 40:53
    If you want to do it like this--
  • 40:53 - 40:54
    STUDENT: Next one is a dy.
  • 40:54 - 40:57
    Then we'll do the 1 minus x.
  • 40:57 - 40:59
    MAGDALENA TODA: The
    relationship that
  • 40:59 - 41:02
    counts in the first picture,
    the first frame that you see
  • 41:02 - 41:08
    [INAUDIBLE], is the
    relationship between y and z.
  • 41:08 - 41:15
    So Mr. z is free to move from
    0 to 1, and Mr. y is here,
  • 41:15 - 41:21
    and he's conditioned by z.
  • 41:21 - 41:24
    And you have to write down the
    equation of this line, which
  • 41:24 - 41:27
    is y plus z equals 1.
  • 41:27 - 41:29
    [INAUDIBLE]
  • 41:29 - 41:34
    So y goes all the way
    from 0 to y minus z.
  • 41:34 - 41:38
    And x goes all the
    way from 0 to what?
  • 41:38 - 41:41
    STUDENT: [INAUDIBLE].
  • 41:41 - 41:42
    MAGDALENA TODA: y minus z.
  • 41:42 - 41:44
    The same thing.
  • 41:44 - 41:47
    So how can you even [INAUDIBLE]?
  • 41:47 - 41:50
    Do you guys play cards?
  • 41:50 - 41:53
    You know what a-- OK.
  • 41:53 - 41:56
    It's like in cards at the end.
  • 41:56 - 41:58
    After king, the ace is coming.
  • 41:58 - 42:01
    And after the ace, a [? 2y ?].
  • 42:01 - 42:05
    So it's a circular
    permutation in the sense
  • 42:05 - 42:08
    that x can be replaced by
    y, can be replaced by z,
  • 42:08 - 42:10
    can be replaced by x, and so on.
  • 42:10 - 42:13
    So what do you
    replace in this case
  • 42:13 - 42:17
    to make a circular permutation?
  • 42:17 - 42:20
    z becomes x.
  • 42:20 - 42:23
    y becomes y.
  • 42:23 - 42:25
    This is held in place.
  • 42:25 - 42:32
    And z becomes and
    x becomes the z.
  • 42:32 - 42:41
    So what I can do is just replace
    the x's by z's and I'm done.
  • 42:41 - 42:46
    And the x, the x by
    z and the z by x.
  • 42:46 - 42:48
    This is circular permutation.
  • 42:48 - 42:51
    Have you heard the
    presentation before?
  • 42:51 - 42:54
    You can write them
    even in matrix form.
  • 42:54 - 42:56
    I don't know if
    in linear algebra
  • 42:56 - 42:59
    they will do permutations,
    but they should.
  • 42:59 - 43:05
    They cover permutations usually
    in higher math, in 3310.
  • 43:05 - 43:09
    Or in graduate school, they
    start with that in algebra.
  • 43:09 - 43:10
    All right.
  • 43:10 - 43:12
    I'm going to move on.
  • 43:12 - 43:15
  • 43:15 - 43:20
    I'm thinking I'm not sure
    what I want to do really.
  • 43:20 - 43:23
    But I'm also thinking of
    proposing an extra credit
  • 43:23 - 43:24
    problem.
  • 43:24 - 43:28
    I will say maybe
    something like that.
  • 43:28 - 43:33
  • 43:33 - 43:36
    y equals x, or maybe
    any one of the problems
  • 43:36 - 43:38
    could be considered
    extra credit problem.
  • 43:38 - 43:41
    I don't know.
  • 43:41 - 43:45
    The same idea of reversing
    the order of the integral,
  • 43:45 - 43:49
    I would like you guys
    to-- Where do they meet?
  • 43:49 - 43:49
    At 1?
  • 43:49 - 43:52
  • 43:52 - 43:53
    Right.
  • 43:53 - 43:57
    So keep in mind that I may
    not give you the points
  • 43:57 - 44:01
    and may only give
    you the functions.
  • 44:01 - 44:03
    And you have to find
    the points where
  • 44:03 - 44:06
    the two functions intersect,
    the two lines intersect.
  • 44:06 - 44:10
    And it's a piece of cake
    because you set x as x squared.
  • 44:10 - 44:12
    x squared minus x is 0.
  • 44:12 - 44:14
    x times x minus 1 is 0.
  • 44:14 - 44:16
    So you have solution
    x1 equals 0.
  • 44:16 - 44:19
    That gives you the origin.
  • 44:19 - 44:22
    And x2 equals 1.
  • 44:22 - 44:25
    That gives you 1 and 1 and
    then becomes a piece of cake.
  • 44:25 - 44:29
    I may ask you to
    say the following.
  • 44:29 - 44:36
    Find me the area of this
    beautiful leaf by both methods,
  • 44:36 - 44:38
    or reverse the order
    of integration.
  • 44:38 - 44:43
    Set up the integrals in both
    ways and get me the answer.
  • 44:43 - 44:45
    I have no idea
    what the answer is.
  • 44:45 - 44:48
    I used to know these things
    by heart, [INAUDIBLE].
  • 44:48 - 44:52
    So you have integral
    from 0 to 1, integral
  • 44:52 - 44:55
    from x squared to x.
  • 44:55 - 44:57
    Am I right?
  • 44:57 - 44:58
    1 dy dx.
  • 44:58 - 45:00
  • 45:00 - 45:03
    Or-- and now I'll shut up
    Magdalena, and let people
  • 45:03 - 45:06
    talk-- reverse the
    order of integration.
  • 45:06 - 45:07
    What do you have?
  • 45:07 - 45:09
    STUDENT: Still at 0, 1.
  • 45:09 - 45:13
    MAGDALENA TODA: Still 0 to 1,
    but Mr. y is happy about that.
  • 45:13 - 45:15
    [INAUDIBLE].
  • 45:15 - 45:18
    We have to [INAUDIBLE] in
    our head and [INAUDIBLE].
  • 45:18 - 45:21
    STUDENT: Square root of y.
  • 45:21 - 45:23
    MAGDALENA TODA: y
    squared is smaller.
  • 45:23 - 45:23
    Yes.
  • 45:23 - 45:27
    He wants to be on the
    bottom and this is why.
  • 45:27 - 45:30
    So I'm too lazy
    to write it down.
  • 45:30 - 45:32
    If I have three people
    who will tell me
  • 45:32 - 45:36
    what the answer is [? so I'll ?]
    write the answer down.
  • 45:36 - 45:37
    The area.
  • 45:37 - 45:39
    The area of this
    beautiful shape.
  • 45:39 - 45:40
    STUDENT: [INAUDIBLE].
  • 45:40 - 45:42
    MAGDALENA TODA: Is it?
  • 45:42 - 45:42
    Yeah.
  • 45:42 - 45:47
    I need three people to tell
    me what it is because it's not
  • 45:47 - 45:48
    that I don't believe you.
  • 45:48 - 45:50
    I know you're a good
    student, but I just--
  • 45:50 - 45:53
    I need witnesses so I
    can sign the document.
  • 45:53 - 45:56
  • 45:56 - 45:57
    Integrate.
  • 45:57 - 46:04
    STUDENT: [INAUDIBLE] integration
    [INAUDIBLE] y squared.
  • 46:04 - 46:07
    MAGDALENA TODA: x is
    between y squared and y.
  • 46:07 - 46:08
    y [? is usually ?] [INAUDIBLE].
  • 46:08 - 46:09
    STUDENT: It would
    be square root of y.
  • 46:09 - 46:10
    Square root of y, yeah.
  • 46:10 - 46:12
    Square root of y.
  • 46:12 - 46:14
    MAGDALENA TODA: Oh.
  • 46:14 - 46:15
    Thank you.
  • 46:15 - 46:21
    So x is square root of y,
    and x-- thank you very much.
  • 46:21 - 46:22
    I'm very happy.
  • 46:22 - 46:24
    You told me and I believed you.
  • 46:24 - 46:26
    See why you should
    never believe me.
  • 46:26 - 46:29
    Square root of y.
  • 46:29 - 46:34
    And this is x
    equals y, of course.
  • 46:34 - 46:34
    Good.
  • 46:34 - 46:35
    So very good.
  • 46:35 - 46:37
    So which one are
    you going to do?
  • 46:37 - 46:39
    This one or this one?
  • 46:39 - 46:39
    Hmm.
  • 46:39 - 46:42
    It's easier to do this
    one numerically quickly
  • 46:42 - 46:43
    in your mind.
  • 46:43 - 47:00
  • 47:00 - 47:01
    Come on. [INAUDIBLE].
  • 47:01 - 47:02
    STUDENT: We have 1/6.
  • 47:02 - 47:03
    MAGDALENA TODA: OK.
  • 47:03 - 47:08
    So square root over
    2, x cubed, 1/6.
  • 47:08 - 47:11
    So I'm sorry for not believing,
    but I should [INAUDIBLE].
  • 47:11 - 47:12
    STUDENT: That's still
    only two people.
  • 47:12 - 47:13
    MAGDALENA TODA: Huh?
  • 47:13 - 47:15
    STUDENT: That's still
    only two people.
  • 47:15 - 47:17
    MAGDALENA TODA: Yes.
  • 47:17 - 47:18
    All right.
  • 47:18 - 47:20
  • 47:20 - 47:28
    Don't expect something hard,
    but of course, always check it.
  • 47:28 - 47:30
    Check your work even
    if you trust yourself
  • 47:30 - 47:33
    because any of us
    can make a mistake.
  • 47:33 - 47:34
    This was [INAUDIBLE].
  • 47:34 - 47:40
    So you see just
    think of everything
  • 47:40 - 47:45
    you write down and think,
    is this what [INAUDIBLE]?
  • 47:45 - 47:47
    Even if you know the
    material very well,
  • 47:47 - 47:50
    you can make an algebra
    mistake any time.
  • 47:50 - 47:50
    All right.
  • 47:50 - 47:59
  • 47:59 - 48:08
    [INAUDIBLE] number 8.
  • 48:08 - 48:22
  • 48:22 - 48:26
    Compute the area of the
    part of the plane which
  • 48:26 - 48:32
    lies about the xy lane
    in the first [INAUDIBLE].
  • 48:32 - 48:36
    So practically they say
    line about the xy plane,
  • 48:36 - 48:41
    there is this part of
    the x plus y plus z.
  • 48:41 - 48:44
    You want the area of that guy.
  • 48:44 - 48:47
    Now, two ways to do it.
  • 48:47 - 48:52
    I would not feel like repeating
    it because it's in your notes.
  • 48:52 - 48:56
    How did you do this-- OK.
  • 48:56 - 48:59
    How can you do this by
    elementary mathematics?
  • 48:59 - 49:01
    STUDENT: It's an
    equilateral triangle.
  • 49:01 - 49:04
    MAGDALENA TODA: It's an
    equilateral triangle of side l,
  • 49:04 - 49:08
    and then you said
    area is l squared.
  • 49:08 - 49:10
    Square root of 3 over 4.
  • 49:10 - 49:17
    How di we do that with a
    height-- this is l over 2.
  • 49:17 - 49:17
    This is l.
  • 49:17 - 49:22
    This is square
    root of 3l over 2.
  • 49:22 - 49:23
    We did the area.
  • 49:23 - 49:25
    We came up with that.
  • 49:25 - 49:31
    So the answer would
    be l is root 2, right.
  • 49:31 - 49:32
    This is 1 and this is 1.
  • 49:32 - 49:38
    So root 2, root 3 over
    4 is root 3 over 2.
  • 49:38 - 49:42
    But that's not how I
    wanted to solve it.
  • 49:42 - 49:51
    So I may say using the
    formula of the surface area,
  • 49:51 - 49:54
    find me the area
    of the triangular
  • 49:54 - 49:57
    surface in the picture.
  • 49:57 - 50:00
    And in that case,
    what do I need to do?
  • 50:00 - 50:03
    We need to know a
    formula, which is what?
  • 50:03 - 50:09
    Which says double integral over
    the domain d square root of 1
  • 50:09 - 50:14
    plus f sub x squared plus
    x sub y squared dx dy
  • 50:14 - 50:19
    where f is easy to pull out
    from here-- 1 minus x minus y.
  • 50:19 - 50:22
  • 50:22 - 50:24
    Who is d?
  • 50:24 - 50:26
    Who remembers who d is?
  • 50:26 - 50:31
    He must be the
    [? projection ?] on the floor.
  • 50:31 - 50:36
    So for d, I say x
    is between 0 and 1.
  • 50:36 - 50:38
    Am I right or am I wrong?
  • 50:38 - 50:43
    y is between 0 and 1 minus x.
  • 50:43 - 50:48
    This is x, y, and z.
  • 50:48 - 50:50
    What is this number?
  • 50:50 - 50:53
  • 50:53 - 50:56
    Formulas we give on the exams,
    usually a piece of cake.
  • 50:56 - 50:59
    This problem was
    picked so that z
  • 50:59 - 51:03
    would be so beautiful in order
    for you to integrate quickly
  • 51:03 - 51:06
    to the square root of--
    what is this number?
  • 51:06 - 51:08
    Minus 1 squared is 1.
  • 51:08 - 51:09
    1 plus 1 plus 1.
  • 51:09 - 51:13
    Root 3, square root of 3.
  • 51:13 - 51:16
    And square root of
    3 will multiply.
  • 51:16 - 51:21
    OK, what is the meaning
    of double integral 1, 1,
  • 51:21 - 51:23
    dx dy over the domain?
  • 51:23 - 51:26
    It's actually the
    area of that domain.
  • 51:26 - 51:27
    Say what, Magdalena?
  • 51:27 - 51:28
    Remember that.
  • 51:28 - 51:30
    When you had double
    integral, you
  • 51:30 - 51:33
    don't have to do the
    work here because double
  • 51:33 - 51:38
    integral over domain will be
    easy to compute [INAUDIBLE].
  • 51:38 - 51:39
    This is [INAUDIBLE].
  • 51:39 - 51:41
    So you cheat only in part.
  • 51:41 - 51:47
    You pretend that you've
    already done the triangle area.
  • 51:47 - 51:49
    Otherwise, you must
    say area of the d
  • 51:49 - 51:59
    will be my hard worker, 0 to
    1, 0 to 1 minus x 1 dy dx.
  • 51:59 - 52:03
    And [INAUDIBLE].
  • 52:03 - 52:06
  • 52:06 - 52:08
    STUDENT: Squared.
  • 52:08 - 52:09
    MAGDALENA TODA: Yeah.
  • 52:09 - 52:16
    So it's x over x between 0 and 1
    minus x squared [? over 2, ?] 0
  • 52:16 - 52:19
    and 1, 1 minus 1/2, 1/2.
  • 52:19 - 52:22
    I actually proved
    what in this part,
  • 52:22 - 52:24
    that the area of this
    triangle on the floor
  • 52:24 - 52:28
    is 1/2 as if we didn't
    know that from school.
  • 52:28 - 52:30
    But I have to
    pretend that I don't
  • 52:30 - 52:34
    know the area, the
    pink area, is 1/2.
  • 52:34 - 52:34
    All right.
  • 52:34 - 52:38
  • 52:38 - 52:39
    OK.
  • 52:39 - 52:41
    In this [INAUDIBLE], where
    else do I want to go?
  • 52:41 - 52:46
  • 52:46 - 52:50
    I want to do this
    with your help.
  • 52:50 - 52:55
    It's sort of like this problem
    before but a little bit
  • 52:55 - 52:58
    different.
  • 52:58 - 53:00
    Can I go ahead and erase or--
  • 53:00 - 53:01
    STUDENT: [INAUDIBLE].
  • 53:01 - 53:02
    MAGDALENA TODA: OK.
  • 53:02 - 53:04
    So I'll write it down.
  • 53:04 - 53:04
    Yes.
  • 53:04 - 53:08
    STUDENT: In this
    case, [INAUDIBLE]
  • 53:08 - 53:11
    x plus y [INAUDIBLE].
  • 53:11 - 53:12
    MAGDALENA TODA: Mm-hmm.
  • 53:12 - 53:14
    STUDENT: How would
    we go from there?
  • 53:14 - 53:18
    MAGDALENA TODA: So you
    know that that's above
  • 53:18 - 53:24
    because the plane
    intersects the axes
  • 53:24 - 53:30
    and coordinates by this line,
    by this line, and by this line.
  • 53:30 - 53:36
    If you think that line's
    above in this first octent
  • 53:36 - 53:40
    because it is said-- although
    maybe lies above the plane
  • 53:40 - 53:41
    but everywhere.
  • 53:41 - 53:43
    Then you will be in
    trouble because you'll
  • 53:43 - 53:45
    get an infinite area.
  • 53:45 - 53:49
    But in the first octent,
    you have a finite volume
  • 53:49 - 53:55
    because your triangle coming
    from here all the way down,
  • 53:55 - 53:58
    it cuts the planes and you
    get that the only thing
  • 53:58 - 54:04
    you have above the floor is this
    triangle, the triangle that you
  • 54:04 - 54:06
    draw in your imagination because
    if I start drawing they will
  • 54:06 - 54:08
    fire me, even if I have tenure.
  • 54:08 - 54:12
    If I start drawing with
    the marker on the board,
  • 54:12 - 54:14
    I'll get in trouble.
  • 54:14 - 54:18
    Or maybe they make me
    pay like $10,000 fine.
  • 54:18 - 54:20
    But you have to
    imagine this corner
  • 54:20 - 54:27
    as being exactly that one and
    those three being your 1, 2,
  • 54:27 - 54:30
    and 3 lines.
  • 54:30 - 54:34
    That's the only thing that's
    above in the first octet.
  • 54:34 - 54:36
    All right.
  • 54:36 - 54:39
    [INAUDIBLE] you
    have no alternative,
  • 54:39 - 54:41
    you don't have something like
    that. [INAUDIBLE] yes, sir.
  • 54:41 - 54:44
    STUDENT: I was wondering,
    where'd the square root of 1
  • 54:44 - 54:47
    and then the partial derivative
    of x, partial derivative of 1
  • 54:47 - 54:49
    come from just that--
  • 54:49 - 54:50
    MAGDALENA TODA: This?
  • 54:50 - 54:53
    STUDENT: Yes, that part.
  • 54:53 - 54:55
    Like, I understand the
    area and everything,
  • 54:55 - 54:56
    but I don't understand--
  • 54:56 - 54:57
    MAGDALENA TODA: We've
    done that before.
  • 54:57 - 54:59
    I'll tell you in a second.
  • 54:59 - 55:07
    So when we computed this kind
    of problem, there was a surface
  • 55:07 - 55:09
    and this was parameterized.
  • 55:09 - 55:13
    And we proved that there
    is a position vector,
  • 55:13 - 55:18
    and for that, you have--
    imagine like a car
  • 55:18 - 55:19
    with coordinate lines.
  • 55:19 - 55:24
    And we've said we want to
    approximate the curvilinear
  • 55:24 - 55:30
    domain between some mesh,
    or a rectangular mesh.
  • 55:30 - 55:32
    And then you have a
    curvilinear square.
  • 55:32 - 55:37
    And the best approximation for
    the area of that curvilinear
  • 55:37 - 55:40
    square was the parallelogram,
    the parallelogram
  • 55:40 - 55:46
    that had the velocities-- so
    you have this kind of stuff.
  • 55:46 - 55:52
    You have [INAUDIBLE], and
    you have a delta y here,
  • 55:52 - 55:58
    and here you have r sub x,
    and here you have r sub y.
  • 55:58 - 56:02
    And you say I don't want
    the big parallelogram.
  • 56:02 - 56:05
    I want the one that is
    approximately infinitesimally
  • 56:05 - 56:07
    small.
  • 56:07 - 56:07
    So you make
  • 56:07 - 56:09
    make pixels, and
    pixels, and pixels
  • 56:09 - 56:11
    that are smaller and smaller.
  • 56:11 - 56:13
    And you can say, if
    this curvilinear pixel
  • 56:13 - 56:22
    is small enough, then
    its area will be what?
  • 56:22 - 56:26
    r sub x, r sub y,
    and cross product
  • 56:26 - 56:31
    in length, which is the area of
    the parallelogram times dx dy.
  • 56:31 - 56:35
  • 56:35 - 56:36
    Right?
  • 56:36 - 56:39
    It's like delta x and
    delta y displacement.
  • 56:39 - 56:44
    When we did the kind of--
    this is infinitesimal area.
  • 56:44 - 56:49
    When we did the integral,
    what we said, write rx,
  • 56:49 - 56:53
    ry cross product dx dy.
  • 56:53 - 56:56
    And I'm going to say, oh
    my God, this is such a pan
  • 56:56 - 56:57
    to write the surface area.
  • 56:57 - 57:02
    That's going to be the
    surface area of the graph.
  • 57:02 - 57:06
    This is the graph
    s, from surface.
  • 57:06 - 57:09
    Area of s.
  • 57:09 - 57:10
    We came up with this.
  • 57:10 - 57:12
    If you remember, it
    was a long time ago.
  • 57:12 - 57:15
    It was before the spring break.
  • 57:15 - 57:16
    OK.
  • 57:16 - 57:19
    We took r as the
    parametrization,
  • 57:19 - 57:23
    and we said, wait a minute,
    if r is my parametrization,
  • 57:23 - 57:26
    it better be easy,
    otherwise my life
  • 57:26 - 57:28
    is going to be too complicated.
  • 57:28 - 57:34
    So I g x is x, y is y, and
    z will be instead of z,
  • 57:34 - 57:37
    we put the graph f of x, y.
  • 57:37 - 57:40
    And then we did what?
  • 57:40 - 57:45
    Then we said, r sub x was 1, and
    this is where the 1 comes from.
  • 57:45 - 57:53
    1, 0, f sub x, r sub y
    equals 0, 1, f sub y.
  • 57:53 - 57:56
    And when we computed
    the cross product,
  • 57:56 - 58:01
    we got-- what is the cross
    product, guys, I forget.
  • 58:01 - 58:07
    ijk, the determinant that
    has ijk and the coordinates
  • 58:07 - 58:10
    on the first row and
    on the second row.
  • 58:10 - 58:12
    So I'm practically
    proving the theorem.
  • 58:12 - 58:15
    This is the theorem.
  • 58:15 - 58:17
    Most people don't prove
    anything in the classroom.
  • 58:17 - 58:20
    They just say, swallow
    these formulas.
  • 58:20 - 58:21
    They come from God.
  • 58:21 - 58:22
    You have to believe them.
  • 58:22 - 58:23
    Right?
  • 58:23 - 58:27
    But the whole
    artificial argument
  • 58:27 - 58:32
    was brought up by people later.
  • 58:32 - 58:37
    The way Gauss and Euler,
    independently anyway,
  • 58:37 - 58:40
    came up with formulas
    like that was
  • 58:40 - 58:45
    by finding this
    curvilinear little red area
  • 58:45 - 58:48
    of this curvilinear square
    written as an integral.
  • 58:48 - 58:51
    And this becomes
    much more beautiful
  • 58:51 - 58:58
    when you have z equals f
    of x, y as parametrization.
  • 58:58 - 59:00
    What do you do in that case?
  • 59:00 - 59:04
    Well, you take the
    lengths of this vector.
  • 59:04 - 59:05
    What is the length
    of this vector?
  • 59:05 - 59:08
    What is this vector, actually?
  • 59:08 - 59:12
    This vector should
    be-- somebody help me,
  • 59:12 - 59:23
    please-- minus f sub x, i,
    minus f sub y, j plus k.
  • 59:23 - 59:26
    OK, so what is the
    length of this vector?
  • 59:26 - 59:29
    The length of this vector
    will be exactly that.
  • 59:29 - 59:32
  • 59:32 - 59:35
    So this is exactly the
    length of the-- the area
  • 59:35 - 59:38
    of the little parallelogram,
    curvilinear parallelogram.
  • 59:38 - 59:44
    That area element will be this.
  • 59:44 - 59:47
    And that's why you
    have this area element.
  • 59:47 - 59:50
    Let's call this area element.
  • 59:50 - 59:53
    In general, it doesn't
    have to be so beautiful.
  • 59:53 - 59:54
    In general, it's really ugly.
  • 59:54 - 60:00
    It's an integral that you have
    to involve Matlab in, or Maple,
  • 60:00 - 60:02
    or something really hard.
  • 60:02 - 60:05
    You cannot solve this by hand.
  • 60:05 - 60:11
    Imagine even if you have a
    simple example like-- guys,
  • 60:11 - 60:17
    think of the paraboloid, or
    the paraboloid that you liked,
  • 60:17 - 60:19
    that looks like a vase.
  • 60:19 - 60:24
    What would be the
    parametrization?
  • 60:24 - 60:30
    You have to do square root,
    double integral 1 plus
  • 60:30 - 60:31
    STUDENT: 4x squared.
  • 60:31 - 60:33
    MAGDALENA TODA: 4x
    squared plus 4y squared.
  • 60:33 - 60:39
    If you were to do that in a
    domain that's rectangular,
  • 60:39 - 60:41
    you'd just kill yourself.
  • 60:41 - 60:43
    STUDENT: Could you
    say change to polar?
  • 60:43 - 60:45
    MAGDALENA TODA: With polar, it's
    easy, but writing the domain
  • 60:45 - 60:47
    is ugly.
  • 60:47 - 60:52
    If it's a round domain, like
    a disc on top of a disc,
  • 60:52 - 60:53
    you switch to polar,
    and you say, thank
  • 60:53 - 60:56
    God I'm above a disc,
    but otherwise, it
  • 60:56 - 60:58
    would be really hard.
  • 60:58 - 61:00
    So what do you do when
    you cannot integrate
  • 61:00 - 61:03
    because the integration
    is too hard to do?
  • 61:03 - 61:07
    You go to Matlab, which
    is written for engineers,
  • 61:07 - 61:09
    but mathematicians
    use Matlab a lot.
  • 61:09 - 61:10
    Or Mathematica,
    which was primarily
  • 61:10 - 61:17
    written for mathematicians,
    I think, by Wolfram
  • 61:17 - 61:20
    in Urbana-Champaign, Illinois.
  • 61:20 - 61:25
    And then, what other softwares?
  • 61:25 - 61:27
    Mainly Matlab.
  • 61:27 - 61:30
    Matlab would be the
    one that helps you.
  • 61:30 - 61:30
    And Maple.
  • 61:30 - 61:32
    You can use Maple.
  • 61:32 - 61:33
    It's very user friendly.
  • 61:33 - 61:39
    You just plug in the endpoints
    for the integral domain,
  • 61:39 - 61:43
    and then you have the
    integrand to that.
  • 61:43 - 61:45
    But Matlab has much
    higher capabilities
  • 61:45 - 61:49
    from computational viewpoints.
  • 61:49 - 61:51
    You can also write
    you own programs.
  • 61:51 - 61:53
    If you are a computer
    science major,
  • 61:53 - 61:57
    you would be able to
    program in C or C++,
  • 61:57 - 62:00
    write a program on how
    to compute the area
  • 62:00 - 62:04
    of a curvilinear graph about
    some-- and that's neat.
  • 62:04 - 62:05
    That's just for fun.
  • 62:05 - 62:09
    Of course, you would neglect
    your other responsibilities,
  • 62:09 - 62:11
    and you say, I'm not
    going to a Saturday party,
  • 62:11 - 62:13
    I am writing this program.
  • 62:13 - 62:18
    And that's how we become nerds,
    by saying no to the parties.
  • 62:18 - 62:20
    All right.
  • 62:20 - 62:25
    So let's do this one.
  • 62:25 - 62:26
    I'm not afraid.
  • 62:26 - 62:30
    I know that you guys
    would do the problem
  • 62:30 - 62:34
    with no problem
    over the interval,
  • 62:34 - 62:37
    but I've never done
    exactly this one,
  • 62:37 - 62:42
    so I want to see
    how you respond.
  • 62:42 - 62:45
    Set up a double
    integral, it says,
  • 62:45 - 62:51
    to compute the area of the
    domain between the two lines,
  • 62:51 - 62:55
    so that you integrate first
    with respect to y and then
  • 62:55 - 62:55
    with respect to x.
  • 62:55 - 62:57
    Reverse the order
    of integration.
  • 62:57 - 62:58
    What is the area?
  • 62:58 - 63:01
    Remark that no written
    computation is necessary.
  • 63:01 - 63:03
    Why?
  • 63:03 - 63:07
    I don't know why-- why
    am I asking you that?
  • 63:07 - 63:11
    Oh, because it's an
    elementary problem.
  • 63:11 - 63:13
    I didn't think of a graph.
  • 63:13 - 63:15
    So the answer would
    be, draw the picture.
  • 63:15 - 63:17
    You will see how funny it is.
  • 63:17 - 63:20
  • 63:20 - 63:21
    y equals x.
  • 63:21 - 63:27
  • 63:27 - 63:28
    y equals x plus 2.
  • 63:28 - 63:29
    It looks horrible.
  • 63:29 - 63:31
    Guys, you have to forgive me.
  • 63:31 - 63:36
    These are parallel
    lines, for God's sake.
  • 63:36 - 63:38
    Do they look parallel to you?
  • 63:38 - 63:40
    Let's say we are in
    hyperbolic space,
  • 63:40 - 63:43
    and then they should--
    could be anything.
  • 63:43 - 63:45
  • 63:45 - 63:51
    Now, we [? split them up ?]
    [? separate. ?] So you have x
  • 63:51 - 63:56
    between-- did they say-- x
    has to be between 0 and 2.
  • 63:56 - 63:59
  • 63:59 - 64:01
    So this is the point 0, 0.
  • 64:01 - 64:03
    This is the point 0, 2.
  • 64:03 - 64:12
    This is the point 2 and 2,
    and this is the point 2 and 4.
  • 64:12 - 64:20
  • 64:20 - 64:21
    OK.
  • 64:21 - 64:24
    Set up a double integral
    to compute the area.
  • 64:24 - 64:25
    Then, reverse the
    order of integration,
  • 64:25 - 64:27
    and tell me the
    area, and tell me
  • 64:27 - 64:32
    why I shouldn't worry too
    much about the computation.
  • 64:32 - 64:38
    So integral from what to what?
  • 64:38 - 64:39
    STUDENT: 0 to 2.
  • 64:39 - 64:40
    MAGDALENA TODA: 0.
  • 64:40 - 64:41
    To 2.
  • 64:41 - 64:43
    STUDENT: And x to x plus 2.
  • 64:43 - 64:44
    MAGDALENA TODA:
    And x to x plus 2.
  • 64:44 - 64:46
    Very good.
  • 64:46 - 64:50
    Of 1, because it's
    in the area, right?
  • 64:50 - 64:50
    dy dx.
  • 64:50 - 64:54
  • 64:54 - 64:56
    Or reverse the order
    of integration,
  • 64:56 - 64:59
    but do it carefully, right?
  • 64:59 - 65:03
  • 65:03 - 65:06
    It's that easy.
  • 65:06 - 65:09
    And then, it's not easy at all.
  • 65:09 - 65:12
    Why is this not easy?
  • 65:12 - 65:14
    First of all, it's not easy
    because my picture sucks.
  • 65:14 - 65:16
    Let's see what it is.
  • 65:16 - 65:19
    I'll do it again.
  • 65:19 - 65:20
    Oh.
  • 65:20 - 65:22
    Will you forgive me for
    this horrible picture?
  • 65:22 - 65:23
    I'm going to draw a better one.
  • 65:23 - 65:26
  • 65:26 - 65:32
    First of all, this is a square.
  • 65:32 - 65:36
    2, 2, and this is 2, 4.
  • 65:36 - 65:39
  • 65:39 - 65:41
    And I'll draw the lines.
  • 65:41 - 65:55
  • 65:55 - 65:58
    OK, now it looks better.
  • 65:58 - 66:00
    Because before, your domains
    would intersect like crazy.
  • 66:00 - 66:07
    So right now I can
    see that-- if I
  • 66:07 - 66:11
    want to do the strip test,
    vertical strip test, that's
  • 66:11 - 66:14
    already done, and I'm glad.
  • 66:14 - 66:18
    But if I want to do
    the horizontal test,
  • 66:18 - 66:21
    I'm in trouble, at
    first, a little bit.
  • 66:21 - 66:22
    Why?
  • 66:22 - 66:24
    STUDENT: [INAUDIBLE] two
    separate [INAUDIBLE].
  • 66:24 - 66:25
    MAGDALENA TODA: Right.
  • 66:25 - 66:28
    So I have to divide, split
    this integral into two.
  • 66:28 - 66:33
    So it's saying,
    area 1 plus area 2.
  • 66:33 - 66:38
    And so when you actually
    decide which method to use,
  • 66:38 - 66:40
    you're never going to
    compute it with this one.
  • 66:40 - 66:40
    Yes, ma'am?
  • 66:40 - 66:42
    STUDENT: Aren't they equal?
  • 66:42 - 66:43
    MAGDALENA TODA: They are
    equal, but I'm saying,
  • 66:43 - 66:48
    when you compute, you don't
    take the worst-- well,
  • 66:48 - 66:49
    you mean the two?
  • 66:49 - 66:50
    STUDENT: Yeah.
  • 66:50 - 66:51
    So can't you just multiply--
  • 66:51 - 66:53
    MAGDALENA TODA: So you
    can say bisymmetry.
  • 66:53 - 66:55
    In this case, you're lucky.
  • 66:55 - 66:57
    In this case, you're lucky.
  • 66:57 - 66:59
    But [? life, ?] in general--
    attention in the actual exam.
  • 66:59 - 67:07
  • 67:07 - 67:09
    And you can have
    something like that.
  • 67:09 - 67:11
    So in general, you add them.
  • 67:11 - 67:13
    You add them, and
    you do like this.
  • 67:13 - 67:15
    In this case, they added them.
  • 67:15 - 67:21
    So I'll write twice,
    but you have to say,
  • 67:21 - 67:22
    you observe that
    bisymmetry, we have
  • 67:22 - 67:27
    to-- the diagonal in
    this parallelogram,
  • 67:27 - 67:30
    we'll divide the parallelogram
    into two congruent triangles.
  • 67:30 - 67:32
    Yes, sir?
  • 67:32 - 67:33
    STUDENT: I don't
    want to sound dumb,
  • 67:33 - 67:38
    but if I take integration
    between 0 and 2,
  • 67:38 - 67:45
    and choose as the top function
    my biggest function, then--
  • 67:45 - 67:48
    MAGDALENA TODA: 0 to 2 is,
    this is the top function,
  • 67:48 - 67:49
    this is the bottom function.
  • 67:49 - 67:50
    STUDENT: No, no.
  • 67:50 - 67:50
    X plus--
  • 67:50 - 67:52
    MAGDALENA TODA:
    For the 2, 2, 4--
  • 67:52 - 67:53
    STUDENT: You have x plus 2--
  • 67:53 - 67:54
    MAGDALENA TODA: --this
    is the top function,
  • 67:54 - 67:55
    this is the bottom function.
  • 67:55 - 67:57
    STUDENT: I take the
    integration between 0 and 2,
  • 67:57 - 67:57
    minus integration--
  • 67:57 - 67:58
    MAGDALENA TODA: Plus, plus.
  • 67:58 - 67:59
    No?
  • 67:59 - 68:00
    STUDENT: No, he's doing
    something different--
  • 68:00 - 68:01
    STUDENT: Different.
  • 68:01 - 68:06
    Integration of 0 to
    2 that is only in x.
  • 68:06 - 68:07
    That will be the
    same area that--
  • 68:07 - 68:09
    MAGDALENA TODA: You
    mean with respect
  • 68:09 - 68:10
    to y, or with respect to x?
  • 68:10 - 68:13
    STUDENT: I'm taking it
    with respect to-- I'm just
  • 68:13 - 68:15
    looking at the graph.
  • 68:15 - 68:16
    MAGDALENA TODA: Which graph?
  • 68:16 - 68:18
    Are you looking like this,
    or are you looking like that?
  • 68:18 - 68:19
    STUDENT: No, this way.
  • 68:19 - 68:19
    Whatever the graph is.
  • 68:19 - 68:20
    MAGDALENA TODA: This way?
  • 68:20 - 68:21
    STUDENT: Yes.
  • 68:21 - 68:22
    MAGDALENA TODA: No.
  • 68:22 - 68:27
    The x is between 0 and 2, or
    y is between 0 and 4 for you.
  • 68:27 - 68:29
    Are you doing horizontal
    strips or vertical strips?
  • 68:29 - 68:30
    STUDENT: No.
  • 68:30 - 68:32
    I'm just using the Calc
    I, base, then finding
  • 68:32 - 68:35
    the area of up to two lines.
  • 68:35 - 68:36
    MAGDALENA TODA: Ah.
  • 68:36 - 68:37
    Then you are using
    vertical strips.
  • 68:37 - 68:44
    Because this is the same as
    Calc I. f of x minus g of x
  • 68:44 - 68:45
    equals x plus 2.
  • 68:45 - 68:48
    We haven't solved
    the integral yet, OK?
  • 68:48 - 68:51
    So we didn't get to solving.
  • 68:51 - 68:55
    We are saying, how do I set up
    the reverse integration thingy.
  • 68:55 - 68:59
    Which I can say observe
    congruent triangles,
  • 68:59 - 69:07
    and then I say twice the
    integral from, this is 0 to 2.
  • 69:07 - 69:15
    And then this guy is
    y equals x on top.
  • 69:15 - 69:19
    This guy is-- well,
    [? who ?] is first?
  • 69:19 - 69:20
    STUDENT: There
    should be x equals y.
  • 69:20 - 69:25
    MAGDALENA TODA: Should
    be, this is dx dy.
  • 69:25 - 69:25
    OK?
  • 69:25 - 69:26
    This is dx dy.
  • 69:26 - 69:27
    STUDENT: x should go--
  • 69:27 - 69:33
    MAGDALENA TODA: So x is between
    0 on the bottom, and y on top.
  • 69:33 - 69:35
    And you have a 1.
  • 69:35 - 69:39
    And after you do this,
    you would double it.
  • 69:39 - 69:40
    Right?
  • 69:40 - 69:48
    What I wrote is just-- What
    I wrote is just this part.
  • 69:48 - 69:52
    So in the end,
    which one do you do?
  • 69:52 - 69:54
    Which one is easier
    for you to do?
  • 69:54 - 69:57
    For me, what you
    said is the easiest.
  • 69:57 - 69:58
    STUDENT: Yeah.
  • 69:58 - 70:06
    MAGDALENA TODA: So
    you get-- Right?
  • 70:06 - 70:08
    So how would my son solve it?
  • 70:08 - 70:11
    Or your nephew, by the way?
  • 70:11 - 70:13
    He is third grade, fifth grade?
  • 70:13 - 70:16
    STUDENT: [INAUDIBLE]
  • 70:16 - 70:22
    MAGDALENA TODA: He would
    say, take this triangle,
  • 70:22 - 70:24
    cut it, and glue it here.
  • 70:24 - 70:26
    He doesn't know
    parallelogram or anything.
  • 70:26 - 70:29
    So he says, cut this
    triangle, and glue it here.
  • 70:29 - 70:32
    And he knows the
    area of 2 times 2,
  • 70:32 - 70:35
    and he would have gotten it in
    like 5 seconds, what we just
  • 70:35 - 70:38
    discussed for 20 seconds.
  • 70:38 - 70:43
    Now, unfortunately,
    life is not linear.
  • 70:43 - 70:45
    Life is very non-linear,
    and as you saw,
  • 70:45 - 70:49
    you get the most surprising
    fight with a parent,
  • 70:49 - 70:50
    or breakup.
  • 70:50 - 70:54
    That's all examples of
    life being non-linear.
  • 70:54 - 70:57
    We have two
    non-linear functions,
  • 70:57 - 71:00
    or we have some
    curvilinear functions
  • 71:00 - 71:02
    that intersect,
    elementary geometry is not
  • 71:02 - 71:04
    going to help you here.
  • 71:04 - 71:08
    Only calculus for everything
    that is non-linear.
  • 71:08 - 71:10
    STUDENT: That's why
    we have calculus.
  • 71:10 - 71:12
    MAGDALENA TODA: That's
    why we have calculus.
  • 71:12 - 71:13
    STUDENT: Now, question is--
  • 71:13 - 71:14
    MAGDALENA TODA: Yes.
  • 71:14 - 71:16
    I have a question,
    as well, so go ahead.
  • 71:16 - 71:18
    STUDENT: Would you accept
    if I use the Calc-based,
  • 71:18 - 71:19
    even though--
  • 71:19 - 71:22
    MAGDALENA TODA: This is
    what my question was.
  • 71:22 - 71:23
    Would I accept?
  • 71:23 - 71:24
    What do you guys think?
  • 71:24 - 71:27
    So I would like you
    to write this down,
  • 71:27 - 71:29
    because I'm saying it.
  • 71:29 - 71:34
    I'm saying actually write
    down, reverse the integration,
  • 71:34 - 71:35
    and stuff.
  • 71:35 - 71:39
    But if you don't,
    you just say, I
  • 71:39 - 71:41
    see from the
    beginning I have a 4,
  • 71:41 - 71:45
    that the area is 4, that's
    fine with me, as well.
  • 71:45 - 71:47
    I don't care how
    you get the answer.
  • 71:47 - 71:49
    The simplest possible
    way to get an answer
  • 71:49 - 71:51
    is the best thin, as long
    as the answer is correct.
  • 71:51 - 71:54
  • 71:54 - 71:56
    STUDENT: So, will there be
    partial credit on the exam?
  • 71:56 - 71:58
    MAGDALENA TODA: And,
    yeah, by the way.
  • 71:58 - 72:02
    So like, when I say set
    up a double integral,
  • 72:02 - 72:05
    I would say at 50% to do that.
  • 72:05 - 72:07
    And for somebody
    who doesn't know
  • 72:07 - 72:10
    how to do that, I would
    say-- and the person says,
  • 72:10 - 72:13
    I know it's 4, I saw it's 4.
  • 72:13 - 72:15
    It's elementary.
  • 72:15 - 72:16
    50%.
  • 72:16 - 72:17
    Partial credit.
  • 72:17 - 72:18
    Is that fair?
  • 72:18 - 72:20
    I think so.
  • 72:20 - 72:23
    So for setting up
    the two things, half,
  • 72:23 - 72:27
    and for doing the numerical
    part by any method, half.
  • 72:27 - 72:32
    And I do partial credit.
  • 72:32 - 72:32
    All right.
  • 72:32 - 72:37
  • 72:37 - 72:39
    The last problem.
  • 72:39 - 72:41
    The Last of the Mohicans.
  • 72:41 - 72:45
    Write and set up only a
    triple integral in spherical
  • 72:45 - 72:46
    coordinates.
  • 72:46 - 72:49
    Now, you cannot do that, because
    I haven't taught spherical
  • 72:49 - 72:52
    coordinates, and that's
    I'm going to do today.
  • 72:52 - 72:56
    In order to compute the volume
    inside the unit sphere, which
  • 72:56 - 73:01
    is a sphere radius 1
    centered at the origin,
  • 73:01 - 73:06
    we have to do that using
    spherical coordinates.
  • 73:06 - 73:08
    And that's what I'm
    going to do today.
  • 73:08 - 73:11
    So good, that was
    the time to stop.
  • 73:11 - 73:17
    I'm moving to 12.7, Cylindrical
    and Spherical Coordinates.
  • 73:17 - 73:25
  • 73:25 - 73:28
    And you take a
    five minute break.
  • 73:28 - 73:29
    STUDENT: Starting now?
  • 73:29 - 73:30
    MAGDALENA TODA: Yeah.
  • 73:30 - 73:32
    Because it's also time to stop.
  • 73:32 - 73:36
    It's between the review
    and the new thing to teach.
  • 73:36 - 74:06
  • 74:06 - 74:08
    How was your break?
  • 74:08 - 74:11
    STUDENT: [INAUDIBLE]
  • 74:11 - 74:17
  • 74:17 - 74:22
    MAGDALENA TODA: Did you go
    to Florida, or any nice place
  • 74:22 - 74:24
    with lots of palm trees?
  • 74:24 - 74:24
    You went home.
  • 74:24 - 74:26
    That is the best.
  • 74:26 - 74:26
    Home.
  • 74:26 - 74:30
    STUDENT: [INAUDIBLE]
  • 74:30 - 74:52
  • 74:52 - 74:56
    [SIDE CONVERSATIONS]
  • 74:56 - 78:10
  • 78:10 - 78:11
    MAGDALENA TODA: All right.
  • 78:11 - 78:16
    [SIDE CONVERSATIONS]
  • 78:16 - 78:21
    MAGDALENA TODA: Now, if you
    remember polar coordinates,
  • 78:21 - 78:24
    polar coordinates are
    cylindrical coordinates,
  • 78:24 - 78:28
    so they are the
    easier guys to learn.
  • 78:28 - 78:35
    Practically, I'm talking about
    switching from x, y, z in R3
  • 78:35 - 78:41
    to-- back and forth--
    to r, theta, and z.
  • 78:41 - 78:44
    In which way?
  • 78:44 - 78:46
    Well, x, y, r, your old friends.
  • 78:46 - 78:53
    r cosine theta, and r
    sine theta, and z is z.
  • 78:53 - 78:56
  • 78:56 - 78:59
    So this is the change
    between Cartesian coordinates
  • 78:59 - 79:01
    and polar coordinates.
  • 79:01 - 79:03
    And it's a
    differentiable function.
  • 79:03 - 79:05
    So you can go back and forth.
  • 79:05 - 79:09
  • 79:09 - 79:13
    So it's going to be r
    is a function of x, y,
  • 79:13 - 79:18
    square root of x
    squared plus y squared,
  • 79:18 - 79:25
    and then if you look at tangent
    of theta, tangent of theta
  • 79:25 - 79:28
    is always y over x.
  • 79:28 - 79:33
    So theta will be
    r tan of y over x.
  • 79:33 - 79:38
    So you have a bunch
    of inverse functions
  • 79:38 - 79:41
    that are differentiable.
  • 79:41 - 79:42
    OK?
  • 79:42 - 79:45
    Both functions are c1.
  • 79:45 - 79:54
    The one that goes from r
    theta x to x, y, z and back.
  • 79:54 - 79:57
    Circles, c1 functions.
  • 79:57 - 80:01
  • 80:01 - 80:05
    Differentiable, and the
    derivatives are continuous.
  • 80:05 - 80:09
    So you have no problem
    setting up a Jacobian.
  • 80:09 - 80:11
    What will the Jacobian be?
  • 80:11 - 80:21
    That's going to be dx
    dr, dx d theta, dx dz.
  • 80:21 - 80:26
    So you take the x, y,
    z prime with respect
  • 80:26 - 80:29
    to r, theta, and z.
  • 80:29 - 80:37
    Then you have dy dr,
    dy d theta, dy dz.
  • 80:37 - 80:41
    So you can take this function
    of these three variables
  • 80:41 - 80:45
    prime with respect to each
    of the three variables,
  • 80:45 - 80:50
    and then you take this
    z with respect to r,
  • 80:50 - 80:54
    with respect to theta, and
    with respect to z itself.
  • 80:54 - 80:57
    And then you say, oh my
    God, that should be easy,
  • 80:57 - 80:59
    because they are independent.
  • 80:59 - 81:01
    Exactly.
  • 81:01 - 81:03
    So you have independence here.
  • 81:03 - 81:06
  • 81:06 - 81:09
    Declaration of independence
    between x and z.
  • 81:09 - 81:10
    So this is 0.
  • 81:10 - 81:12
    This is 0.
  • 81:12 - 81:12
    This is 0.
  • 81:12 - 81:13
    This is 0.
  • 81:13 - 81:14
    This is 1.
  • 81:14 - 81:16
    He's a lucky guy.
  • 81:16 - 81:19
    And these parts, you've
    seen these guys before.
  • 81:19 - 81:21
    Let's see how well
    you remember them.
  • 81:21 - 81:22
    You don't have to remember them.
  • 81:22 - 81:23
    You compute them again.
  • 81:23 - 81:28
    So if you differentiate
    x with respect to r,
  • 81:28 - 81:30
    you get cosine theta.
  • 81:30 - 81:35
    Taking x prime with
    respect to theta,
  • 81:35 - 81:37
    you get minus r sine theta.
  • 81:37 - 81:40
  • 81:40 - 81:50
    Here, you get y with respect
    to r will be sine theta,
  • 81:50 - 81:56
    and y with respect to theta
    will be r equals sine theta.
  • 81:56 - 81:59
    And again, 0, 0, 0, and 1.
  • 81:59 - 82:02
    So who can compute
    this determinant
  • 82:02 - 82:06
    and tell me quickly, well, if
    you are taking Linear Algebra,
  • 82:06 - 82:09
    and two of you are, you
    can tell me immediately.
  • 82:09 - 82:14
    STUDENT: So it's r squared
    [? minus ?] 2r squared?
  • 82:14 - 82:15
    STUDENT: It should just be r.
  • 82:15 - 82:16
    MAGDALENA TODA: --just r.
  • 82:16 - 82:16
    STUDENT: r.
  • 82:16 - 82:17
    MAGDALENA TODA: It's just r.
  • 82:17 - 82:19
    You can expand
    along the last row,
  • 82:19 - 82:24
    and you have 1 times the
    determinant over here.
  • 82:24 - 82:26
    The determinant
    over here is just
  • 82:26 - 82:31
    r cosine squared plus r
    sine squared, which is r.
  • 82:31 - 82:34
    So it's r times 1, which is r.
  • 82:34 - 82:38
    Your old friend r, which was the
    Jacobian for polar coordinates,
  • 82:38 - 82:41
    is still the Jacobian for
    cylindrical coordinates.
  • 82:41 - 82:44
    So that's why I'm saying,
    cylindrical coordinates
  • 82:44 - 82:45
    are your friends.
  • 82:45 - 82:47
    They want to be your friends.
  • 82:47 - 82:49
    I will give you an example.
  • 82:49 - 82:52
  • 82:52 - 82:53
    Yes?
  • 82:53 - 82:54
    STUDENT: [INAUDIBLE]
  • 82:54 - 82:55
    MAGDALENA TODA: Sorry, sorry.
  • 82:55 - 82:55
    No, no.
  • 82:55 - 82:59
    We take that eggshell
    from last time.
  • 82:59 - 83:02
    We put it upside down.
  • 83:02 - 83:04
    Only one eggshell, OK?
  • 83:04 - 83:06
    We start with that easy problem.
  • 83:06 - 83:09
    And this is z equals y minus
    x squared minus y squared.
  • 83:09 - 83:12
  • 83:12 - 83:17
    It's half of the egg that we
    built from plastic last time.
  • 83:17 - 83:22
  • 83:22 - 83:31
    And I want to express the
    triple integral of the volume--
  • 83:31 - 83:43
    express triple integral
    of the volume in terms
  • 83:43 - 83:57
    of first, Cartesian coordinates,
    and second, cylindrical
  • 83:57 - 83:57
    coordinates.
  • 83:57 - 84:06
  • 84:06 - 84:11
    And you're going to say, well,
    I have a circular domain, right?
  • 84:11 - 84:16
    The disc is a domain
    inside the circle.
  • 84:16 - 84:22
    So it's a lot more natural to
    use cylindrical coordinates
  • 84:22 - 84:23
    and not Cartesian coordinates.
  • 84:23 - 84:27
    Why do you want us to use
    Cartesian coordinates at all?
  • 84:27 - 84:32
    I just beg you to bear with
    me, and not actually compute
  • 84:32 - 84:34
    the integral in
    Cartesian coordinates,
  • 84:34 - 84:36
    because you're going
    to kill each other
  • 84:36 - 84:41
    in the process about the
    square roots you have inside.
  • 84:41 - 84:44
    So you can go ahead and
    write it, integral over
  • 84:44 - 84:50
    d, of the function on top,
    which is going to be-- well,
  • 84:50 - 84:53
    let's put it in triple form.
  • 84:53 - 84:57
    The egg, e, you're
    going to laugh at me.
  • 84:57 - 84:59
    It's the triple
    integral over the egg.
  • 84:59 - 85:00
    But actually, it's
    triple integral
  • 85:00 - 85:02
    over the half of the
    egg, but I don't know
  • 85:02 - 85:05
    how to denote half of an egg.
  • 85:05 - 85:10
    It's [? all the ?] volume
    of the body inside the egg.
  • 85:10 - 85:13
    1 dV.
  • 85:13 - 85:22
    I can write it as a
    double integral over D--
  • 85:22 - 85:24
    is that clear?
  • 85:24 - 85:27
    of the z function on top.
  • 85:27 - 85:31
    1 minus x squared minus y
    squared minus the function
  • 85:31 - 85:35
    below, which is 0.
  • 85:35 - 85:38
    Which is going to tell me dx dy.
  • 85:38 - 85:42
    Which is also denoted
    [? da. ?] If you're
  • 85:42 - 85:45
    going to do this in
    Cartesian coordinates,
  • 85:45 - 85:47
    well, good luck to you.
  • 85:47 - 85:52
    Because you're going to
    have something like that.
  • 85:52 - 85:57
    Mister x says I want to
    go between minus 1 and 1.
  • 85:57 - 86:01
  • 86:01 - 86:04
    And that's x.
  • 86:04 - 86:07
    He wants to go all the
    way between minus 1 and 1.
  • 86:07 - 86:11
    And meanwhile, y says,
    but I'm restricted by you,
  • 86:11 - 86:13
    because I'm in a marriage.
  • 86:13 - 86:17
    x squared plus y
    squared equals 1,
  • 86:17 - 86:20
    so y goes between square
    root 1 minus x squared
  • 86:20 - 86:24
    and minus square root
    1 minus x squared.
  • 86:24 - 86:27
    So he goes, look how ugly I am.
  • 86:27 - 86:31
    Minus square root
    1 minus x squared
  • 86:31 - 86:33
    plus square root
    1 minus x squared.
  • 86:33 - 86:37
    And then you have to put
    the integrand, 1 minus x
  • 86:37 - 86:40
    squared minus y squared.
  • 86:40 - 86:42
    And then you go dx dy.
  • 86:42 - 86:47
  • 86:47 - 86:51
    So it's not the best thing.
  • 86:51 - 86:53
    It's not the most
    beautiful thing.
  • 86:53 - 86:56
    Now, you say, but
    I'm going to write it
  • 86:56 - 87:00
    in cylindrical coordinates, and
    you will see how beautiful it's
  • 87:00 - 87:03
    going to become, and I agree.
  • 87:03 - 87:07
    The same thing can be written
    as triple integral over the egg,
  • 87:07 - 87:19
    over the half of the egg,
    1 dV, will be 1, 2, 3.
  • 87:19 - 87:21
    What will be the volume element?
  • 87:21 - 87:23
    Because the volume
    element is not
  • 87:23 - 87:27
    going to be-- when I switch
    to polar-- not going to be dr,
  • 87:27 - 87:30
    d theta, dz.
  • 87:30 - 87:37
    It's going to be r
    rimes dz dr d theta.
  • 87:37 - 87:40
    Remember that, because
    I've seen students
  • 87:40 - 87:45
    forget this r, the
    Jacobian, all the time.
  • 87:45 - 87:51
    This Jacobian is very
    [? useful. ?] All right.
  • 87:51 - 87:58
    So I'll put here
    1r, dz, dr, d theta.
  • 87:58 - 88:02
    Mister z says, I know I'm going
    from the bottom to the top,
  • 88:02 - 88:04
    from the bottom to the top.
  • 88:04 - 88:07
    So z goes, I'm
    between 0 and whoever
  • 88:07 - 88:11
    you gave me, 1 minus x
    squared minus y squared.
  • 88:11 - 88:12
    And he's happy about that.
  • 88:12 - 88:17
    It doesn't look so ugly.
  • 88:17 - 88:22
    And now r and theta say, well,
    we are sort of independent.
  • 88:22 - 88:28
    r is always between 0
    and 1 in my picture,
  • 88:28 - 88:32
    because I have the unit disc
    on the bottom, on the floor.
  • 88:32 - 88:35
    And theta is between
    0 and 2 pi, because I
  • 88:35 - 88:37
    have a complete rotation.
  • 88:37 - 88:42
    If this were chocolate
    cake, or just something
  • 88:42 - 88:46
    made of-- something
    good, some mayo tower,
  • 88:46 - 88:49
    or something, cheese tower.
  • 88:49 - 88:53
    And I wanted to cut it in
    half or cut it in a quarter,
  • 88:53 - 88:55
    I would be very careful
    about the theta.
  • 88:55 - 89:00
    For example, this is chocolate,
    and I cut it as a quarter.
  • 89:00 - 89:03
    I have to say, just
    the first octant.
  • 89:03 - 89:07
    So you see the piece of the
    cake that would be in the first
  • 89:07 - 89:08
    octant-- now,
    [? our coordinate ?]
  • 89:08 - 89:09
    [? here ?].
  • 89:09 - 89:13
    So for that kind of problem,
    you would have to say,
  • 89:13 - 89:19
    r is between 0 and 1, but
    theta would be between 0 and pi
  • 89:19 - 89:21
    over 2.
  • 89:21 - 89:22
    Are you guys with me?
  • 89:22 - 89:25
    So you were lucky, in
    this case, that you have
  • 89:25 - 89:26
    a full rotation all around.
  • 89:26 - 89:28
    You eat the entire cake.
  • 89:28 - 89:32
    But in other problems,
    you may have a half
  • 89:32 - 89:35
    of a cake, a quarter of a cake.
  • 89:35 - 89:37
    Yes, sir?
  • 89:37 - 89:44
    STUDENT: Why is it dx dy
    down there on the area?
  • 89:44 - 89:45
    MAGDALENA TODA: dy dx.
  • 89:45 - 89:48
    You are very smart,
    and I appreciate that.
  • 89:48 - 89:50
    Thank you.
  • 89:50 - 89:53
    In a regular class--
    oh, I'm not even saying.
  • 89:53 - 89:55
    I made the same mistake one
    time, just right in class,
  • 89:55 - 89:57
    and nobody notices.
  • 89:57 - 90:00
    I noticed later, but
    it was a little late.
  • 90:00 - 90:01
    Thanks [INAUDIBLE].
  • 90:01 - 90:07
    So this is y integration
    first, x integration.
  • 90:07 - 90:09
    Good.
  • 90:09 - 90:12
    Let's see about that.
  • 90:12 - 90:13
    What am I going to do with that?
  • 90:13 - 90:17
    That worries me, because
    this looks like it
  • 90:17 - 90:19
    has nothing to do there.
  • 90:19 - 90:21
    Everything should be
    in z, r, and theta,
  • 90:21 - 90:25
    and this guy is 1
    minus r squared.
  • 90:25 - 90:28
    Otherwise, he doesn't
    belong in there.
  • 90:28 - 90:31
    So I have to write it down.
  • 90:31 - 90:40
    0 to 2 pi, 0 to 1, 0 to 1 minus
    r squared, r, dz, dr, d theta.
  • 90:40 - 90:41
    Is it hard to do?
  • 90:41 - 90:42
    Is it hard to solve?
  • 90:42 - 90:45
  • 90:45 - 90:46
    Shouldn't be.
  • 90:46 - 90:47
    Why?
  • 90:47 - 90:50
    Well, let's go from the
    inside to the outside.
  • 90:50 - 90:55
    First of all, what is the
    beautiful thing about this?
  • 90:55 - 90:59
    As soon as I'm done
    with this integration,
  • 90:59 - 91:04
    I have a product of
    functions in theta and r
  • 91:04 - 91:06
    that are independent.
  • 91:06 - 91:08
    So let me write it down.
  • 91:08 - 91:13
    Integral from 0 to 2 pi,
    integral from 0 to 1,
  • 91:13 - 91:17
    and I decide, I'm all for it.
  • 91:17 - 91:20
    I'll have integral of r dz.
  • 91:20 - 91:24
    But z has nothing to do with
    r, so he says, well, I'm z,
  • 91:24 - 91:24
    you're r.
  • 91:24 - 91:27
    We are independent.
  • 91:27 - 91:30
    r is like a constant
    for the time being.
  • 91:30 - 91:35
    He can even go here and wait.
  • 91:35 - 91:38
    And then the integral
    you have, it goes out.
  • 91:38 - 91:39
    He gets out.
  • 91:39 - 91:39
    You see, guys?
  • 91:39 - 91:40
    He gets out.
  • 91:40 - 91:46
    And then, you have 1,
    integral of 1, this is z,
  • 91:46 - 91:52
    z between-- I'm taking
    this alone-- between 0 down
  • 91:52 - 91:55
    and 1 minus r squared up.
  • 91:55 - 91:57
    I could have
    written this faster,
  • 91:57 - 91:59
    but that's not the point.
  • 91:59 - 92:05
    So this will be integrated
    with respect to r and theta
  • 92:05 - 92:06
    in the end.
  • 92:06 - 92:09
  • 92:09 - 92:10
    So, again, what did I do?
  • 92:10 - 92:12
    I said that was the r.
  • 92:12 - 92:15
    But the r, when I integrate
    with z, they're independent.
  • 92:15 - 92:17
    So r gets out.
  • 92:17 - 92:18
    Integral of 1 is z.
  • 92:18 - 92:24
    z between these two guys
    is 1 minus r squared.
  • 92:24 - 92:26
    I'm going to write it out.
  • 92:26 - 92:30
  • 92:30 - 92:33
    Integral from 0 to 2 pi.
  • 92:33 - 92:36
    Integral from 0 to 1.
  • 92:36 - 92:39
    Your old friend,
    y minus r squared,
  • 92:39 - 92:43
    times your old
    friend r, dr d theta.
  • 92:43 - 92:44
    Is this hard?
  • 92:44 - 92:46
    Come on, this is not hard.
  • 92:46 - 92:51
    This is a piece of cake,
    a piece of chocolate cake.
  • 92:51 - 92:53
    Right?
  • 92:53 - 92:55
    So, what is this?
  • 92:55 - 92:57
    It's the integral
    of r minus r cubed.
  • 92:57 - 93:01
  • 93:01 - 93:03
    What is your luck here?
  • 93:03 - 93:05
    Theta is not in the picture.
  • 93:05 - 93:08
    So theta says, I'm going
    to go out for a walk.
  • 93:08 - 93:12
    You guys finish integration
    in r, I'm by myself.
  • 93:12 - 93:15
    0 to 2 pi d theta.
  • 93:15 - 93:19
    Say bye, bye, because theta is
    not contained in the integrand.
  • 93:19 - 93:26
    And then you go integral from
    0 to 1, r minus r cubed dr.
  • 93:26 - 93:33
    And now, we have two beautiful,
    simple integrals from Calc I
  • 93:33 - 93:36
    that we should be able
    to solve in no time.
  • 93:36 - 93:40
    I'm too lazy to write,
    again, the anti-derivative,
  • 93:40 - 93:47
    which would be, r squared over
    2 minus r to the 4 over 4.
  • 93:47 - 93:49
    What do I get her in the end?
  • 93:49 - 93:51
    STUDENT: [INAUDIBLE]
  • 93:51 - 93:54
    MAGDALENA TODA: 1/2
    minus 1 over 4, right?
  • 93:54 - 93:56
    So I have 1/4.
  • 93:56 - 93:57
    Did you say the same thing?
  • 93:57 - 93:58
    STUDENT: I said 1/4.
  • 93:58 - 94:01
    MAGDALENA TODA: It's
    the same thing, 1/4.
  • 94:01 - 94:03
    And this is?
  • 94:03 - 94:03
    STUDENT: 2 pi.
  • 94:03 - 94:04
    MAGDALENA TODA: 2 pi.
  • 94:04 - 94:08
    So in the end, I allow
    him to write it like that.
  • 94:08 - 94:11
    Of course-- but you'll
    say, well, it's silly.
  • 94:11 - 94:13
    I should be able to simplify.
  • 94:13 - 94:15
    Well, go ahead and simplify.
  • 94:15 - 94:16
    How much do we get?
  • 94:16 - 94:17
    STUDENT: It's 5/2.
  • 94:17 - 94:19
    MAGDALENA TODA: 5/2.
  • 94:19 - 94:22
    So this says that the
    volume of the chocolate
  • 94:22 - 94:25
    cake-- now I'm dreaming, now
    it's not an eggshell that's
  • 94:25 - 94:28
    empty in the middle
    anymore, it's just
  • 94:28 - 94:32
    a chocolate cake all
    round up and made
  • 94:32 - 94:38
    in the shape of a paraboloid,
    or some hill made of chocolate
  • 94:38 - 94:41
    mousse that I made.
  • 94:41 - 94:45
    So 5 over 2 will be
    the volume of that.
  • 94:45 - 94:46
    Is this a hard problem?
  • 94:46 - 94:47
    It shouldn't be.
  • 94:47 - 94:50
    If you think about
    it, it's nothing new.
  • 94:50 - 94:54
    It's all polar coordinates
    and nothing else.
  • 94:54 - 94:56
    But you may want to
    see one more like that.
  • 94:56 - 94:59
    Do you want to see another
    one like that, or not?
  • 94:59 - 95:00
    Yes?
  • 95:00 - 95:04
    STUDENT: I did the same, but I
    couldn't get the right answer
  • 95:04 - 95:06
    in the homework.
  • 95:06 - 95:08
    Because the first
    level is in Cartesian,
  • 95:08 - 95:10
    and then you have to change
    to spherical, and then--
  • 95:10 - 95:13
    MAGDALENA TODA: Algebra is
    a problem for all of us.
  • 95:13 - 95:17
    Did you remember to include the
    r, and do everything slowly?
  • 95:17 - 95:17
    STUDENT: Yes.
  • 95:17 - 95:21
    My issue was the [? borders. ?]
  • 95:21 - 95:23
    MAGDALENA TODA: The
    boundaries, the midpoints?
  • 95:23 - 95:27
    STUDENT: --it's not-- if I
    put the 0, it's not right.
  • 95:27 - 95:28
    So--
  • 95:28 - 95:30
    MAGDALENA TODA:
    Well, send it to me.
  • 95:30 - 95:34
    Send it to me from WeBWorK,
    and we will see what I can do.
  • 95:34 - 95:36
    It's still unsolved?
  • 95:36 - 95:39
    OK, I'll help you on it.
  • 95:39 - 95:40
    All right.
  • 95:40 - 95:42
    So, let's move on.
  • 95:42 - 95:45
    STUDENT: Yeah, I
    tried [? 5 and 4. ?]
  • 95:45 - 95:46
    MAGDALENA TODA: --to something.
  • 95:46 - 95:48
    Let's move on to
    something trivial.
  • 95:48 - 95:51
    You are going to say, come on,
    Magdalena, this is trivial.
  • 95:51 - 95:52
    I don't want to do this.
  • 95:52 - 95:58
    Of course I know we'll
    find it really easy,
  • 95:58 - 96:02
    the volume of the can of
    Pepsi Cola or whatever.
  • 96:02 - 96:10
    It's a cylinder of
    radius r and height h,
  • 96:10 - 96:12
    and I want to set
    up the integral
  • 96:12 - 96:15
    to compute the volume
    of the cylinder
  • 96:15 - 96:18
    in cylindrical coordinates.
  • 96:18 - 96:24
    So problem 2 for
    cylindrical coordinates
  • 96:24 - 96:30
    to compute the
    volume of a cylinder.
  • 96:30 - 96:34
  • 96:34 - 96:37
    Did we know that from before?
  • 96:37 - 96:39
    I have my helper, here.
  • 96:39 - 96:41
    He has [INAUDIBLE].
  • 96:41 - 96:42
    You all know him.
  • 96:42 - 96:42
    Area of the--
  • 96:42 - 96:44
    STUDENT: Volume [INAUDIBLE]
  • 96:44 - 96:44
    MAGDALENA TODA: --base.
  • 96:44 - 96:45
    STUDENT: The area of
    the base, I'm sorry.
  • 96:45 - 96:47
    MAGDALENA TODA:
    --times the height,
  • 96:47 - 96:52
    which will be pi r
    squared h, right?
  • 96:52 - 96:55
    This is what we should get
    when we compute the integral.
  • 96:55 - 96:58
    If we don't, that means
    we messed up somewhere.
  • 96:58 - 97:00
    STUDENT: Wow.
  • 97:00 - 97:02
    Well get pi r squared z.
  • 97:02 - 97:05
    MAGDALENA TODA: Let's put big
    R, because I reserved little r
  • 97:05 - 97:10
    for the variable
    between 0 and big R
  • 97:10 - 97:11
    for the polar coordinates.
  • 97:11 - 97:17
    So this is big R,
    and this is little h.
  • 97:17 - 97:20
    And this is your domain.
  • 97:20 - 97:24
    So how do you write cylinder?
  • 97:24 - 97:31
    Well, let's say the
    body inside is called c.
  • 97:31 - 97:34
    I have triple
    integral over c of 1.
  • 97:34 - 97:39
  • 97:39 - 97:40
    dz, dy, dx.
  • 97:40 - 97:44
  • 97:44 - 97:48
    Of course, we won't do this
    in cylindrical coordinates,
  • 97:48 - 97:59
    so this dV becomes
    r, dr, d theta, dz.
  • 97:59 - 98:02
  • 98:02 - 98:06
    So I will have to do
    it in proper order.
  • 98:06 - 98:13
    r dz first, dz, dr, d
    theta, because-- well, it
  • 98:13 - 98:15
    doesn't matter in
    this case, z is still
  • 98:15 - 98:17
    between some fixed values.
  • 98:17 - 98:21
    z is between 0 and h.
  • 98:21 - 98:25
    Again, if this were a
    plane or another surface,
  • 98:25 - 98:28
    you would write it as a variable
    function of two variables.
  • 98:28 - 98:32
    Then you have r between 0 and r.
  • 98:32 - 98:37
    You have theta
    between 0 and 2 pi.
  • 98:37 - 98:39
    I could give you on
    the final something,
  • 98:39 - 98:42
    a quarter of a salami.
  • 98:42 - 98:45
    Just cut the salami
    on the first octant,
  • 98:45 - 98:51
    and get the same problem
    as this, but instead
  • 98:51 - 98:56
    of theta from 0 to 2 pi, you
    would have theta from 0 to pi
  • 98:56 - 98:59
    over 2.
  • 98:59 - 99:02
    So, is this hard?
  • 99:02 - 99:04
    It shouldn't be hard.
  • 99:04 - 99:05
    r, again, gets out.
  • 99:05 - 99:06
    He says, I'm out of her.
  • 99:06 - 99:08
    I have nothing to do with z.
  • 99:08 - 99:11
    So z is by himself.
  • 99:11 - 99:17
    Z by himself gets integral of
    1 dz, z. z between 0 and h.
  • 99:17 - 99:20
    So h is by himself.
  • 99:20 - 99:30
    So I have, again, integral,
    integral 0 to 2 pi, 0 to big R.
  • 99:30 - 99:34
    And here, I have h.
  • 99:34 - 99:35
    Are you guys with me?
  • 99:35 - 99:37
    Are you following?
  • 99:37 - 99:42
    dr d theta.
  • 99:42 - 99:43
    STUDENT: h should [INAUDIBLE]
  • 99:43 - 99:46
  • 99:46 - 99:48
    MAGDALENA TODA: And
    the r-- I forgot.
  • 99:48 - 99:51
    You see how easy it is
    to forget. r is here,
  • 99:51 - 99:54
    but I forgot it here.
  • 99:54 - 99:54
    r is here.
  • 99:54 - 99:58
    He was hiding behind the
    bush, so I pulled him back
  • 99:58 - 100:02
    in the picture, because I need
    to integrate with respect to r.
  • 100:02 - 100:06
    Now, fortunately for
    us, this is easy.
  • 100:06 - 100:08
    It's a piece of cake.
  • 100:08 - 100:09
    What is a constant
    for everybody?
  • 100:09 - 100:11
    Little h.
  • 100:11 - 100:13
    He goes out in a hurry.
  • 100:13 - 100:15
    He says, I'm hurrying out.
  • 100:15 - 100:17
    I have h out.
  • 100:17 - 100:19
    But then you have
    a double integral
  • 100:19 - 100:23
    of a product of two
    functions in one variable.
  • 100:23 - 100:28
    So you have one integral in
    r only, which is this one.
  • 100:28 - 100:30
    Are you guys with me?
  • 100:30 - 100:36
    And one integral in theta only,
    which is integral of 1 d theta.
  • 100:36 - 100:40
    Can you tell me the limit
    points for the integrals?
  • 100:40 - 100:40
    STUDENT: 0, r.
  • 100:40 - 100:41
    STUDENT: 0 and r.
  • 100:41 - 100:43
    MAGDALENA TODA: 0
    and r for this guy,
  • 100:43 - 100:44
    STUDENT: And 0 and 2 pi.
  • 100:44 - 100:48
    MAGDALENA TODA: And 0
    to 1 pi for that guy.
  • 100:48 - 100:52
    And now, it should be easy.
  • 100:52 - 100:54
    Am I getting the right answer?
  • 100:54 - 100:56
    Was this the [? guy ?] and why?
  • 100:56 - 101:03
    Because I have h r
    squared over 2 times 2 pi.
  • 101:03 - 101:12
    2 goes away, so I've got exactly
    h times r squared times pi.
  • 101:12 - 101:14
    Which was the volume
    of the cylinder
  • 101:14 - 101:18
    that our teachers gave to us
    in K-12 with no explanation.
  • 101:18 - 101:21
    They said, well, you
    have to understand,
  • 101:21 - 101:24
    it's basically, if you
    believe that the disc has
  • 101:24 - 101:30
    area pi r squared, you multiply
    that, it'll make 8 sheets, 8
  • 101:30 - 101:31
    tiny sheets of that.
  • 101:31 - 101:33
    Then you multiply,
    and that's how
  • 101:33 - 101:38
    we understood the
    notion of a volume,
  • 101:38 - 101:40
    by repeating those
    cross-sections.
  • 101:40 - 101:41
    You have an altitude
    of h, and you
  • 101:41 - 101:43
    have cross-section
    after cross-section
  • 101:43 - 101:44
    after cross-section.
  • 101:44 - 101:49
    But still you have to
    believe the area of the disc.
  • 101:49 - 101:53
    How did we believe the area of
    the disc when we were little?
  • 101:53 - 101:55
    I remember I didn't believe it.
  • 101:55 - 101:59
    My teacher in fourth grade came
    up with some graphing paper.
  • 101:59 - 102:02
    And we went ahead
    and compared what
  • 102:02 - 102:07
    I got from the little tiny
    squares and the actual formula,
  • 102:07 - 102:10
    and it was hard
    for me to believe.
  • 102:10 - 102:13
    But I was surprised
    that I couldn't
  • 102:13 - 102:19
    find an explanation for my
    pi r squared formula, even
  • 102:19 - 102:20
    in middle school.
  • 102:20 - 102:24
    And then I started high school,
    and still no explanation
  • 102:24 - 102:25
    for that.
  • 102:25 - 102:27
    So I was very
    confused, I was like,
  • 102:27 - 102:31
    is math more like history, where
    we have to memorize everything
  • 102:31 - 102:33
    and believe everything?
  • 102:33 - 102:37
    But thank God for
    calculus, as you said.
  • 102:37 - 102:40
    In college, I
    understood, finally,
  • 102:40 - 102:45
    why the area of the
    disc is pi r squared.
  • 102:45 - 102:50
    OK, let's move on to our
    friend that I announced today
  • 102:50 - 102:55
    with lots of advertisement.
  • 102:55 - 102:56
    Yes, sir?
  • 102:56 - 103:00
    STUDENT: What happens if
    you ask the area [INAUDIBLE]
  • 103:00 - 103:01
    between x and y plane?
  • 103:01 - 103:02
    MAGDALENA TODA: Between?
  • 103:02 - 103:05
    STUDENT: x and y plane.
  • 103:05 - 103:08
    What happens in that?
  • 103:08 - 103:09
    [INAUDIBLE]
  • 103:09 - 103:10
    MAGDALENA TODA:
    Between which plane?
  • 103:10 - 103:13
    STUDENT: x and y.
  • 103:13 - 103:14
    MAGDALENA TODA: x and y plane?
  • 103:14 - 103:18
    STUDENT: Let's
    say z and y plane.
  • 103:18 - 103:19
    MAGDALENA TODA: z
    and y-- which planes?
  • 103:19 - 103:20
    STUDENT: This--
  • 103:20 - 103:23
    MAGDALENA TODA: z equals y?
  • 103:23 - 103:25
    You mean x equals y is a plane.
  • 103:25 - 103:26
    STUDENT: Yeah.
  • 103:26 - 103:27
    MAGDALENA TODA:
    You can ask, well,
  • 103:27 - 103:36
    yeah-- let's say I'm asking the
    volume of the slice of the cake
  • 103:36 - 103:41
    that is between
    x equals y plane,
  • 103:41 - 103:49
    and this plane, x equals
    0, and z equals something.
  • 103:49 - 103:52
    Flat.
  • 103:52 - 104:00
    Then I have to think of,
    again-- so theta, right?
  • 104:00 - 104:03
    I have to take out a 4.
  • 104:03 - 104:06
    0 to 5 or 4, and
    measure differently
  • 104:06 - 104:09
    when I measure the angle, right?
  • 104:09 - 104:11
    We will see some
    sorts of measurements
  • 104:11 - 104:13
    for angles that
    will surprise you.
  • 104:13 - 104:25
    When we look at
    geography on an atlas,
  • 104:25 - 104:33
    we all those latitude and
    longitude coordinates,
  • 104:33 - 104:37
    but nobody ever told us
    about the angles very well.
  • 104:37 - 104:43
    How do we actually define
    longitude and latitude?
  • 104:43 - 104:46
    Well, between mathematicians and
    people who work in geography,
  • 104:46 - 104:49
    there is a consensus.
  • 104:49 - 104:53
    Longitude is this thing that
    you measure around the equator.
  • 104:53 - 104:55
    That is the angle.
  • 104:55 - 104:56
    For people in
    geography, it starts
  • 104:56 - 104:59
    at the Greenwich Village.
  • 104:59 - 105:03
    I mean, the meridian passes
    through Greenwich Village.
  • 105:03 - 105:05
    I went there out of curiosity.
  • 105:05 - 105:06
    And there is nothing there.
  • 105:06 - 105:11
    It's just like a suburb
    of London, or something.
  • 105:11 - 105:16
    It goes through-- so
    meridian 0 goes through that.
  • 105:16 - 105:20
    That's where you
    measure theta equal 0.
  • 105:20 - 105:25
    And you go around up to
    say that equals 2 pi.
  • 105:25 - 105:29
    And how many meridians
    do we actually have?
  • 105:29 - 105:32
    STUDENT: There are 24.
  • 105:32 - 105:35
    MAGDALENA TODA: So when we
    them 1 degree apart, there
  • 105:35 - 105:38
    should be 360 things like that.
  • 105:38 - 105:39
    STUDENT: [INAUDIBLE]
  • 105:39 - 105:40
    MAGDALENA TODA: What?
  • 105:40 - 105:40
    STUDENT: Yeah.
  • 105:40 - 105:41
    MAGDALENA TODA: Huh?
  • 105:41 - 105:43
    STUDENT: Yes, but how
    many do we define as--
  • 105:43 - 105:44
    MAGDALENA TODA: Yeah.
  • 105:44 - 105:48
    In geography, we say 0 degree,
    1 degree, the discretely many 0,
  • 105:48 - 105:50
    1 degree, and so on.
  • 105:50 - 105:57
    So the one that's
    at 180-- OK, it
  • 105:57 - 106:05
    goes 0, 180, is the meridian
    that, if we were to continue,
  • 106:05 - 106:09
    it would go to meridian
    0, past the north pole.
  • 106:09 - 106:09
    All right?
  • 106:09 - 106:12
    So we have this
    notion of longitude
  • 106:12 - 106:15
    that we are going to
    introduce from 0 to 2 pi.
  • 106:15 - 106:17
    And that's fine.
  • 106:17 - 106:19
    But how do you measure latitude?
  • 106:19 - 106:20
    Longitude is up.
  • 106:20 - 106:23
  • 106:23 - 106:32
    Latitude, in geography
    and in mathematics,
  • 106:32 - 106:34
    they may differ a little bit.
  • 106:34 - 106:39
    We can even change our notation
    for latitude sometimes.
  • 106:39 - 106:45
    In geography, always from
    0, the equator, going up.
  • 106:45 - 106:47
    At the North Pole,
    what is your latitude?
  • 106:47 - 106:51
  • 106:51 - 106:52
    STUDENT: It's going
    to be 90 degrees.
  • 106:52 - 106:53
    MAGDALENA TODA: 90 degrees.
  • 106:53 - 106:55
    And how do we say that?
  • 106:55 - 106:59
    STUDENT: [INAUDIBLE] Well, in
    math we say-- I would, too,
  • 106:59 - 107:10
    but-- Now we say North, 90
    degrees North in geography.
  • 107:10 - 107:12
    For a mathematician,
    it's not like that.
  • 107:12 - 107:13
    Mathematicians are crazy people.
  • 107:13 - 107:17
    The go minus pi over
    2, which is minus 90.
  • 107:17 - 107:20
    The geography guy
    says 90 degrees South.
  • 107:20 - 107:24
  • 107:24 - 107:25
    OK?
  • 107:25 - 107:29
    What latitude are
    we here in Lubbock?
  • 107:29 - 107:30
    Do we know?
  • 107:30 - 107:34
  • 107:34 - 107:35
    Come on, you know.
  • 107:35 - 107:37
    STUDENT: 32.
  • 107:37 - 107:38
    33.
  • 107:38 - 107:39
    MAGDALENA TODA: Something.
  • 107:39 - 107:41
    33, I thought, but
    maybe I'm wrong.
  • 107:41 - 107:42
    Something like that.
  • 107:42 - 107:43
    STUDENT: 32.8.
  • 107:43 - 107:44
    MAGDALENA TODA: 32.8.
  • 107:44 - 107:46
    I don't know.
  • 107:46 - 107:53
    In any case, when
    we measure latitude,
  • 107:53 - 107:57
    we should always start-- if we
    are normal, we should always
  • 107:57 - 107:59
    start at the equator,
    because that's
  • 107:59 - 108:01
    how we did it in school, right?
  • 108:01 - 108:04
    To go this way and this way.
  • 108:04 - 108:05
    Mathematicians don't.
  • 108:05 - 108:07
    They say, no, I'm
    going like this.
  • 108:07 - 108:13
    I'm going from minus pi
    over 2 to 0 and 2 pi over 2.
  • 108:13 - 108:15
    That's one way to do it.
  • 108:15 - 108:17
    One way.
  • 108:17 - 108:21
    Minus pi over 2 to
    0 and pi over 2.
  • 108:21 - 108:24
    But here in calculus, we
    are absolutely not normal.
  • 108:24 - 108:27
    So we have another way
    of defining latitude.
  • 108:27 - 108:31
    We say latitude
    from the North Pole.
  • 108:31 - 108:36
    Latitude from the North
    Pole I know how to spell it.
  • 108:36 - 108:40
  • 108:40 - 108:42
    So we measure like this.
  • 108:42 - 108:43
    Look at me.
  • 108:43 - 108:45
    You are going to be amused,
    because you will see that we
  • 108:45 - 108:47
    are crazy, which is true.
  • 108:47 - 108:53
    But this is already
    accepted as the notation.
  • 108:53 - 109:00
    So we go like that
    all the way to 180.
  • 109:00 - 109:04
    So this-- the North
    Pole would be-- so what
  • 109:04 - 109:07
    is the angle for the point p?
  • 109:07 - 109:10
    The angle for the
    point p of latitude--
  • 109:10 - 109:14
    not theta, theta was the
    larger-- let's call it phi.
  • 109:14 - 109:22
    Phi is between 0
    degrees and 180 degrees,
  • 109:22 - 109:25
    which is the South Pole.
  • 109:25 - 109:27
    So we measure-- I think
    because mathematicians still
  • 109:27 - 109:33
    believe in Santa, I don't know--
    they go from the North Pole, 0,
  • 109:33 - 109:37
    90, 180.
  • 109:37 - 109:42
    So this is the angle phi
    that we are defining.
  • 109:42 - 109:44
    Let me show you on a picture
    what the spherical coordinates
  • 109:44 - 109:47
    are, the way we are
    going to use them.
  • 109:47 - 109:54
    So I take a big
    sphere-- a big sphere.
  • 109:54 - 109:59
  • 109:59 - 110:08
    And these are the axes
    the way you know them.
  • 110:08 - 110:14
    This is x-axis, this is y-axis,
    and z-axis, and the origin.
  • 110:14 - 110:18
    And you pick your favorite
    point somewhere on the sphere.
  • 110:18 - 110:22
    And you say, I want to see
    what spherical coordinates are.
  • 110:22 - 110:26
    Those spherical coordinates
    are three coordinates, r theta,
  • 110:26 - 110:28
    and phi.
  • 110:28 - 110:34
    r is the radius from p to o.
  • 110:34 - 110:37
  • 110:37 - 110:44
    Theta is the longitude, and phi
    is the latitude from the North
  • 110:44 - 110:45
    Pole.
  • 110:45 - 110:50
  • 110:50 - 110:51
    OK.
  • 110:51 - 110:52
    So let me draw.
  • 110:52 - 110:55
    Let's take this red,
    and let's draw op.
  • 110:55 - 111:00
  • 111:00 - 111:03
    This is r.
  • 111:03 - 111:05
    But then we say, well, I could
    still be inside the sphere.
  • 111:05 - 111:07
    Yes, you can still
    be inside the sphere.
  • 111:07 - 111:10
    It could be anywhere
    you want in space.
  • 111:10 - 111:16
    Then, how do you measure the
    latitude and the longitude?
  • 111:16 - 111:21
    First of all, to measure,
    let's go from p down,
  • 111:21 - 111:23
    and that's going to
    be p prime somewhere.
  • 111:23 - 111:26
  • 111:26 - 111:30
    Then I'm going to
    say that's op prime.
  • 111:30 - 111:34
    And then I will project on
    the x-axis and the y-axis.
  • 111:34 - 111:38
    So I'm putting 90-degree
    angle, 90-degree angle.
  • 111:38 - 111:41
    This is the x coordinate,
    this is the y coordinate,
  • 111:41 - 111:46
    and this is-- how do
    I do the z coordinate?
  • 111:46 - 111:48
    Through the point
    p, I should draw
  • 111:48 - 111:55
    a plane that's horizontal,
    until that horizontal plane is
  • 111:55 - 111:59
    going to cut the axis z.
  • 111:59 - 112:00
    I'm going to do that.
  • 112:00 - 112:06
    And then what I get is something
    that finishes my rectangle.
  • 112:06 - 112:08
    I have a 90-degree, 90-degree,
    90-degree, 90-degree.
  • 112:08 - 112:13
  • 112:13 - 112:15
    And this is z.
  • 112:15 - 112:16
    This is z.
  • 112:16 - 112:21
    So we have to write down
    everybody, x, y, and z,
  • 112:21 - 112:25
    in terms of r theta and phi.
  • 112:25 - 112:28
    This is going to be
    just trigonometry.
  • 112:28 - 112:30
    We are going to get a
    little bit of a headache,
  • 112:30 - 112:34
    but I know that you
    are going to help me.
  • 112:34 - 112:39
    So the latitude measured
    from the North Pole
  • 112:39 - 112:45
    is this angle, this
    angle phi, which
  • 112:45 - 112:48
    is the same thing
    as this angle phi.
  • 112:48 - 112:50
  • 112:50 - 112:52
    And where is the angle theta?
  • 112:52 - 112:59
    I need a line-- this is
    line color, and I have here.
  • 112:59 - 113:02
  • 113:02 - 113:04
    That's theta.
  • 113:04 - 113:06
    So somebody needs to help me.
  • 113:06 - 113:08
    The easiest is z.
  • 113:08 - 113:11
    Why is z the easiest
    to write down?
  • 113:11 - 113:14
    Because-- It's going to come
    from the Pythagorean theorem,
  • 113:14 - 113:19
    for whatever
    trigonometric angle phi.
  • 113:19 - 113:22
    I have a 90-degree.
  • 113:22 - 113:25
    This is the triangle.
  • 113:25 - 113:28
    What do you think
    z is going to be?
  • 113:28 - 113:31
  • 113:31 - 113:32
    I'm going to go 90.
  • 113:32 - 113:37
    In this triangle, I
    have an angle phi.
  • 113:37 - 113:41
    And z is the adjacent.
  • 113:41 - 113:44
    Phi is the hypotenuse.
  • 113:44 - 113:47
    So let me write down.
  • 113:47 - 113:50
    z is r cosine phi.
  • 113:50 - 113:51
    Yes, in this case.
  • 113:51 - 114:00
  • 114:00 - 114:01
    Why is that?
  • 114:01 - 114:07
    Because I'll take z over
    r, and that's cosine phi.
  • 114:07 - 114:09
    z over r is cosine phi.
  • 114:09 - 114:12
    It's the adjacent
    over the hypotenuse.
  • 114:12 - 114:13
    All right, that was easy.
  • 114:13 - 114:16
    But the problem is, how
    do I get to x and y?
  • 114:16 - 114:20
    Now, unless I find
    the protection,
  • 114:20 - 114:27
    I need you to give me the
    line op prime measure.
  • 114:27 - 114:30
    This is the hard--
    not hard, but-- It's
  • 114:30 - 114:33
    from this other triangle.
  • 114:33 - 114:39
    I'm going to fill it
    in red dots everywhere.
  • 114:39 - 114:48
  • 114:48 - 114:51
    STUDENT: That lined
    line is r the sine of 5.
  • 114:51 - 114:52
    MAGDALENA TODA: r sine 5.
  • 114:52 - 114:53
    Why is that?
  • 114:53 - 114:59
    Because sine of phi will
    be exactly the-- where
  • 114:59 - 115:01
    is the 90-degree angle here?
  • 115:01 - 115:05
    So the sine phi will be the
    opposite over hypotenuse.
  • 115:05 - 115:06
    Say it again.
  • 115:06 - 115:07
    Opposite over hypotenuse.
  • 115:07 - 115:09
    And that's the 90-degree angle.
  • 115:09 - 115:10
    So good.
  • 115:10 - 115:14
    So it's op prime over r.
  • 115:14 - 115:14
    Good.
  • 115:14 - 115:16
    But now, I have to go on,
    because the [? lined ?]
  • 115:16 - 115:19
    guy is not the end of the game.
  • 115:19 - 115:22
    The end of the game is x and y.
  • 115:22 - 115:32
    So x is op prime cosine theta,
    and y op prime sine theta.
  • 115:32 - 115:33
    Who can tell me why?
  • 115:33 - 115:36
  • 115:36 - 115:39
    STUDENT: Because x
    is your adjacent,
  • 115:39 - 115:40
    and y is your opposite.
  • 115:40 - 115:41
    MAGDALENA TODA: Right.
  • 115:41 - 115:44
    Because this is also
    a 90-degree angle.
  • 115:44 - 115:50
    So I have a right triangle,
    and if I take the angle theta,
  • 115:50 - 115:53
    this is the adjacent
    for the angle theta.
  • 115:53 - 116:00
    So cosine theta is x over r, x
    over op prime, the hypotenuse.
  • 116:00 - 116:04
    So again, let's
    write, x over op prime
  • 116:04 - 116:06
    is going to equal sine theta.
  • 116:06 - 116:10
    y over op prime is
    going to be sine theta.
  • 116:10 - 116:12
    That's why I have those.
  • 116:12 - 116:13
    Good.
  • 116:13 - 116:15
    So can I write x and y?
  • 116:15 - 116:18
    X will be-- now comes a
    little bit of headache.
  • 116:18 - 116:23
    op prime is r sine
    phi, cosine theta.
  • 116:23 - 116:29
    r sine phi, cosine theta.
  • 116:29 - 116:38
    Y equals r sine phi sine theta,
    and z equals r cosine phi.
  • 116:38 - 116:40
    Good.
  • 116:40 - 116:44
    These are the famous
    cylindrical-- spherical
  • 116:44 - 116:44
    coordinates.
  • 116:44 - 116:47
  • 116:47 - 116:51
    Spherical coordinate
    transformation.
  • 116:51 - 116:53
    So what does this
    transformation do?
  • 116:53 - 117:00
    This transformation takes
    the r, phi, and theta,
  • 117:00 - 117:04
    and moves them into
    the image x, y, z.
  • 117:04 - 117:08
    So this is the transformation
    I was talking about.
  • 117:08 - 117:10
    STUDENT: Doesn't it
    go from x, y, z to r--
  • 117:10 - 117:12
    MAGDALENA TODA: It goes back.
  • 117:12 - 117:15
    So you have a
    one-to-one function.
  • 117:15 - 117:19
    You have an inverse, and
    the inverse is also c1.
  • 117:19 - 117:23
    They are both c1 functions.
  • 117:23 - 117:24
    The inverse.
  • 117:24 - 117:25
    Who is the inverse?
  • 117:25 - 117:27
    I don't know, guys.
  • 117:27 - 117:30
    OK, I'll only give you one piece
    of information that's crucial,
  • 117:30 - 117:33
    and you'll have to find
    phi and theta, which
  • 117:33 - 117:35
    are not hard to find.
  • 117:35 - 117:38
    Who is r?
  • 117:38 - 117:41
    STUDENT: r is still x
    squared plus y squared.
  • 117:41 - 117:46
    MAGDALENA TODA: r is x squared,
    plus y squared, plus z squared,
  • 117:46 - 117:48
    under square root.
  • 117:48 - 117:49
    Let's see why that is.
  • 117:49 - 117:52
    You may not believe
    me, but I'll do it.
  • 117:52 - 118:00
    So assume that you square x
    squared plus y squared, right?
  • 118:00 - 118:05
    Then you have r squared
    sine phi squared.
  • 118:05 - 118:08
    But the square of this plus
    the square of that collapse
  • 118:08 - 118:11
    and will become a 1
    when you add them up.
  • 118:11 - 118:15
    So When you add up x
    squared plus y squared,
  • 118:15 - 118:17
    this goes away and
    becomes 1, and you have
  • 118:17 - 118:20
    r squared sine squared phi.
  • 118:20 - 118:24
    Now, if you make z
    squared, who is the square?
  • 118:24 - 118:27
    R squared cosine squared phi.
  • 118:27 - 118:29
    Add them all up.
  • 118:29 - 118:32
    x squared plus y
    squared plus z squared
  • 118:32 - 118:37
    equals little r squared.
  • 118:37 - 118:41
    So now we are ready to
    prove the volume of a ball.
  • 118:41 - 118:44
    We have this ball of radius r.
  • 118:44 - 118:49
  • 118:49 - 118:53
    Find the volume of this ball
    with any kind of coordinates
  • 118:53 - 118:54
    you think.
  • 118:54 - 118:57
    But now, you say, OK, if you do
    cylindrical coordinates, good
  • 118:57 - 118:58
    luck to you.
  • 118:58 - 119:03
    It's going to be, we'll
    stay here until midnight
  • 119:03 - 119:06
    computing the volume.
  • 119:06 - 119:08
    Let's try both,
    and let's see how
  • 119:08 - 119:10
    they differ from one another.
  • 119:10 - 119:11
    How hard they are--
  • 119:11 - 119:12
    STUDENT: Can you do Cartesian?
  • 119:12 - 119:13
    MAGDALENA TODA: Hmm?
  • 119:13 - 119:14
    STUDENT: Are you
    going to do Cartesian?
  • 119:14 - 119:15
    MAGDALENA TODA: I'll
    write Cartesian,
  • 119:15 - 119:18
    but I'll write Cartesian,
    I'll write cylindrical.
  • 119:18 - 119:19
    I'm not going to
    use them, though.
  • 119:19 - 119:22
    I'm going to say goodbye
    to them, and in the end,
  • 119:22 - 119:23
    I'm going to use spherical.
  • 119:23 - 119:27
    Now, the beautiful thing about
    the Jacobian for spherical
  • 119:27 - 119:30
    is that it has to be memorized.
  • 119:30 - 119:34
    Because for you to write
    it down as a determinant,
  • 119:34 - 119:43
    dx dr, dx d phi, dx d theta, and
    there are six more like that,
  • 119:43 - 119:44
    it takes forever.
  • 119:44 - 119:47
    So it's better that I
    tell you what it is.
  • 119:47 - 119:52
    I compute it a few times, and
    we get r squared sine phi.
  • 119:52 - 119:57
    So what is the volume of a
    sphere, the volume of the ball?
  • 119:57 - 120:02
    I can write a triple integral
    of 1 dV over the ball
  • 120:02 - 120:08
    B. Let's call this ball
    B. Script, beautiful B.
  • 120:08 - 120:13
    And that will take care of
    the-- this is dx, dy, dz, right?
  • 120:13 - 120:15
    That's the first formula.
  • 120:15 - 120:16
    I cannot use it.
  • 120:16 - 120:18
    It's going to be a mess.
  • 120:18 - 120:23
    Now, let's try this written
    at least in cylindrical
  • 120:23 - 120:24
    coordinates.
  • 120:24 - 120:27
    You will still see
    that is not easy.
  • 120:27 - 120:36
    When we write it in
    cylindrical coordinates,
  • 120:36 - 120:41
    I'm going to have cylindrical
    coordinates, [? still. ?]
  • 120:41 - 120:42
    It's going to be what?
  • 120:42 - 120:49
    It's going to be an r,
    and then dz, dr, d theta.
  • 120:49 - 120:54
    And z, well, we can
    do what [INAUDIBLE]
  • 120:54 - 120:58
    said, mapping several of them.
  • 120:58 - 121:01
    When you have a symmetric
    object, you split it in half,
  • 121:01 - 121:02
    and you say double the area.
  • 121:02 - 121:04
    We can always do that.
  • 121:04 - 121:08
    Or you could go from
    the Southern Hemisphere
  • 121:08 - 121:11
    to the Northern Hemisphere,
    and you practically
  • 121:11 - 121:12
    get the same thing.
  • 121:12 - 121:15
    Now, for the ball
    we have here, you
  • 121:15 - 121:17
    have x squared,
    plus y squared, plus
  • 121:17 - 121:23
    z squared equals-- what was the
    radius of the ball? r squared.
  • 121:23 - 121:24
    OK.
  • 121:24 - 121:26
    I don't like it, but that's OK.
  • 121:26 - 121:31
    z will have to go
    between what and what?
  • 121:31 - 121:35
    Between two nasty square
    roots and a minus.
  • 121:35 - 121:38
    r squared minus x
    squared, minus y squared,
  • 121:38 - 121:44
    and r squared minus x squared
    minus y squared with minus.
  • 121:44 - 121:45
    Do I like it?
  • 121:45 - 121:46
    No.
  • 121:46 - 121:48
    But at least--
    that's in Cartesian.
  • 121:48 - 121:50
    At least in polar
    coordinates, I can
  • 121:50 - 121:56
    say, mister z decides to go from
    minus square root r squared,
  • 121:56 - 121:59
    minus r squared,
    because x squared
  • 121:59 - 122:02
    plus y squared is cylindrical.
  • 122:02 - 122:07
    This is r squared
    in cylindrical.
  • 122:07 - 122:08
    OK?
  • 122:08 - 122:11
    So I would do it like that.
  • 122:11 - 122:19
    Square root r squared minus
    r squared, r from 0 to r,
  • 122:19 - 122:22
    and theta from 0 to 2 pi.
  • 122:22 - 122:25
    And I don't want the headache
    of these square roots,
  • 122:25 - 122:31
    because as soon as I do
    that-- well, I can do it,
  • 122:31 - 122:32
    bit it's obnoxious.
  • 122:32 - 122:35
    I take the z out.
  • 122:35 - 122:40
    z between the 2, I'll take
    z between this and that.
  • 122:40 - 122:44
    So I'll have twice the
    square root times little r.
  • 122:44 - 122:48
    I have to perform some u
    substitution, and to be smart,
  • 122:48 - 122:50
    and I think I can do it.
  • 122:50 - 122:51
    This in cylindrical.
  • 122:51 - 122:55
  • 122:55 - 122:59
    But I want to show you how
    beautiful it is in spherical.
  • 122:59 - 123:04
    In spherical-- what are you
    going to have in spherical?
  • 123:04 - 123:09
    In spherical, you have
    this, the ball in spherical.
  • 123:09 - 123:15
  • 123:15 - 123:19
    1, 2, 3 of 1.
  • 123:19 - 123:21
    1 times the Jacobian.
  • 123:21 - 123:23
    Who is the Jacobian?
    r squared sine phi.
  • 123:23 - 123:26
  • 123:26 - 123:28
    Good.
  • 123:28 - 123:30
    What else?
  • 123:30 - 123:33
    Anything else you want,
    dr, d phi, d theta,
  • 123:33 - 123:35
    they are all between
    fixed endpoints.
  • 123:35 - 123:36
    So you are really lucky.
  • 123:36 - 123:38
    Why are you lucky?
  • 123:38 - 123:41
    Because all these guys,
    r, phi, and theta,
  • 123:41 - 123:45
    are between fixed
    endpoints for a ball.
  • 123:45 - 123:46
    Do we know those endpoints?
  • 123:46 - 123:48
    Well, we better.
  • 123:48 - 123:51
    If we don't, then
    we are not with it.
  • 123:51 - 124:01
    So r for the ball goes little
    r from 0 all the way to r.
  • 124:01 - 124:02
    Good.
  • 124:02 - 124:06
    Now, the latitude
    measured from Santa Claus.
  • 124:06 - 124:08
    That is the question.
  • 124:08 - 124:10
    It's phi, right?
  • 124:10 - 124:18
    It's from 0 to the
    South Pole, phi.
  • 124:18 - 124:20
    And theta is from
  • 124:20 - 124:21
    STUDENT: 0 to 2 pi.
  • 124:21 - 124:22
    MAGDALENA TODA: 0 to 2 pi.
  • 124:22 - 124:25
    From the Greenwich
    meridian all the way back.
  • 124:25 - 124:27
    Good.
  • 124:27 - 124:29
    So now we are ready.
  • 124:29 - 124:34
    Now it's a blessing, because
    we apply the Fubini theorem,
  • 124:34 - 124:37
    and all the endpoints
    being fixed,
  • 124:37 - 124:40
    I can separate this
    integral into a product
  • 124:40 - 124:43
    of three integrals that
    are all independent.
  • 124:43 - 124:47
    And I'm going to ask you
    to tell me what those are.
  • 124:47 - 124:50
  • 124:50 - 124:51
    Yes, sir?
  • 124:51 - 124:54
    STUDENT: Why don't we
    just go from 0 to pi?
  • 124:54 - 124:57
    MAGDALENA TODA: Because--
    you mean for phi?
  • 124:57 - 125:01
    OK, phi is the latitude
    measured from the North Pole.
  • 125:01 - 125:04
    That's why I said Santa Claus.
  • 125:04 - 125:07
    Because mathematicians,
    many of them,
  • 125:07 - 125:10
    are split into two categories.
  • 125:10 - 125:15
    Some say, I measure
    latitude between 0 and pi,
  • 125:15 - 125:20
    and 0 minus pi over 2, so I can
    go all the way between minus pi
  • 125:20 - 125:22
    over 2 to pi.
  • 125:22 - 125:26
    But some say, no,
    I don't like is.
  • 125:26 - 125:31
    I measure the phi
    from 0, because it's
  • 125:31 - 125:33
    easier for the picture.
  • 125:33 - 125:37
    And I measure phi from North
    Pole all the way to the South
  • 125:37 - 125:41
    Pole, and the latitude goes
    all the way to pi, to 180.
  • 125:41 - 125:45
    Now, for me, it was
    easier, because I
  • 125:45 - 125:47
    was able to draw
    this picture, and I
  • 125:47 - 125:51
    was able to write those
    formulas very easily.
  • 125:51 - 125:54
    Now, for those integrals, can
    you tell me, the first one
  • 125:54 - 125:55
    in r, can you tell?
  • 125:55 - 125:58
    Who can tell me the r?
  • 125:58 - 125:59
    STUDENT: 0, r, r squared u.
  • 125:59 - 126:01
    MAGDALENA TODA: Very good.
  • 126:01 - 126:03
    So that's the only thing
    that's a little bit hard.
  • 126:03 - 126:05
    Everything is the same.
  • 126:05 - 126:12
    The integral from--
    sine phi d phi from
  • 126:12 - 126:13
    STUDENT: 0 to pi.
  • 126:13 - 126:15
    MAGDALENA TODA: 0 to pi.
  • 126:15 - 126:17
    And finally, integral from 0 to
  • 126:17 - 126:18
    STUDENT: 2 pi.
  • 126:18 - 126:21
    MAGDALENA TODA: 2 pi.
  • 126:21 - 126:25
    Of 1 d theta, and you
    say that's just 2 pi.
  • 126:25 - 126:26
    I know.
  • 126:26 - 126:27
    That is the beauty of it.
  • 126:27 - 126:29
    It's 2 pi.
  • 126:29 - 126:33
    So that simplifies a
    little bit my life.
  • 126:33 - 126:35
    How about the first fellow?
  • 126:35 - 126:36
    I know you love
    the picture, right?
  • 126:36 - 126:38
    You love this picture.
  • 126:38 - 126:41
    But I need to say goodbye to it.
  • 126:41 - 126:42
    OK.
  • 126:42 - 126:44
    So I'll erase it.
  • 126:44 - 126:48
  • 126:48 - 126:55
    And I have r cubed over 3. r
    cubed over 3 starts showing
  • 126:55 - 126:58
    the meaning of
    the volume formula
  • 126:58 - 127:00
    that you knew from high school.
  • 127:00 - 127:04
  • 127:04 - 127:10
    So this guy becomes
    r cubed over 3
  • 127:10 - 127:13
    means big R cubed over 3 here.
  • 127:13 - 127:16
    The first guy.
  • 127:16 - 127:20
    This first guy is
    this first guy.
  • 127:20 - 127:25
    This guy, not a problem.
  • 127:25 - 127:29
    Integral of sine phi
    is minus cosine phi.
  • 127:29 - 127:34
    And that, you have to measure
    that between 0 and phi.
  • 127:34 - 127:36
    So you have to do it a
    little bit carefully.
  • 127:36 - 127:40
    One time, I had a student
    who got 0 on that.
  • 127:40 - 127:42
    After he plugged in
    here, he got a 0,
  • 127:42 - 127:44
    so he came up with
    this new theorem
  • 127:44 - 127:47
    that the volume
    of the ball was 0,
  • 127:47 - 127:49
    no matter what the
    radius was for him.
  • 127:49 - 127:51
    But he didn't realize
    what was going on.
  • 127:51 - 127:54
    So you realize what
    his mistake was.
  • 127:54 - 127:56
    He didn't get the signs right.
  • 127:56 - 127:58
    So minus cosine of pi.
  • 127:58 - 127:59
    What's cosine of pi?
  • 127:59 - 128:00
    STUDENT: Negative 1.
  • 128:00 - 128:01
    MAGDALENA TODA: Negative 1.
  • 128:01 - 128:06
    With a minus, it's minus
    minus 1, which is plus 1.
  • 128:06 - 128:08
    Right?
  • 128:08 - 128:10
    But then you have
    minus, and he wrote 1,
  • 128:10 - 128:13
    and this is where
    the mistake was.
  • 128:13 - 128:21
    Minus the other 1 is minus
    cosine of 0, which is minus 1.
  • 128:21 - 128:24
    So you get 2.
  • 128:24 - 128:26
    All right, and
    then, finally, 2 pi.
  • 128:26 - 128:28
    So what did we get here?
  • 128:28 - 128:31
    We got something beautiful.
  • 128:31 - 128:32
    We got--
  • 128:32 - 128:36
  • 128:36 - 128:38
    STUDENT: 4/3 pi r cubed over 3.
  • 128:38 - 128:39
    MAGDALENA TODA: Huh?
  • 128:39 - 128:41
    STUDENT: 4/3 pi r cubed.
  • 128:41 - 128:42
    MAGDALENA TODA: Yeah.
  • 128:42 - 128:46
    We got 4 pi r cubed over 3.
  • 128:46 - 128:50
    This is the thing we knew
    from when we were little.
  • 128:50 - 128:55
    How old were we when our
    teachers told us that they
  • 128:55 - 128:59
    cannot tell us why, but this
    is the volume of a sphere?
  • 128:59 - 129:01
    Were we in ninth grade?
  • 129:01 - 129:03
    Younger?
  • 129:03 - 129:04
    Eight grade?
  • 129:04 - 129:07
    But I don't think I
    was able to memorize.
  • 129:07 - 129:09
    That was one of my problems.
  • 129:09 - 129:11
    I think in eight grade, my
    teacher gave me the formula.
  • 129:11 - 129:14
    But I wasn't able to memorize
    that in eighth grade.
  • 129:14 - 129:18
    And I think in high school,
    I memorized it finally,
  • 129:18 - 129:21
    like when I was 16 or something.
  • 129:21 - 129:26
    So this is 4 pi r cubed over
    3, and it closes that question.
  • 129:26 - 129:29
    Next time, I want to do one
    or two more applications
  • 129:29 - 129:31
    for the spherical coordinates,
    because you're not
  • 129:31 - 129:32
    yet used to them.
  • 129:32 - 129:36
    Maybe I'm going to do a
    mixture of the problems,
  • 129:36 - 129:38
    cylindrical, spherical.
  • 129:38 - 129:39
    You know what to expect.
  • 129:39 - 129:44
    Don't expect
    anything really hard.
  • 129:44 - 129:47
    But it walks you slowly
    through the whole [? deal ?]
  • 129:47 - 129:51
    if you go over the set.
  • 129:51 - 129:52
    OK?
  • 129:52 - 129:55
    enjoy the day, and ask
    me questions if you have.
  • 129:55 - 129:58
    I'll be in my office hours.
  • 129:58 - 130:00
Title:
TTU Math2450 Calculus3 Secs 12.6 - 12.7
Description:

Integration in Rectangular, Cylindrical and Spherical coordinates

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Video Language:
English

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