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TTU Math2450 Calculus3 Sec 10.2 and 10.4 part 1

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    PROFESSOR: Any
    questions about theory
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    that gave you headaches
    regarding homework
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    you'd like to talk about?
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    Anything related
    to what we covered
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    from chapter nine and today?
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    STUDENT: Can we
    do some problems?
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    PROFESSOR: I can
    fix from problems
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    like the ones in the
    homework, but also I
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    can have you tell me what
    bothers you in the homework.
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    STUDENT: Oh, I have [INAUDIBLE].
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    PROFESSOR: What bothered
    me about my own homework
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    was that I realized that I
    did not remind you something
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    I assume you should
    know, which is
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    the equation of a sphere of
    given center and given radius.
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    And since I trust you so much,
    I said, OK they know about it.
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    And then somebody asked
    me by email what that was,
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    and I said, oh, yeah.
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    I did not review that in class.
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    So review the equation
    in r3 form that's x, y, z
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    of the sphere of radius r and
    center p of coordinates x0, y0,
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    z0.
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    One of you asked me by email,
    does-- of course you do,
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    and then if you know it,
    can you help me-- can you
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    help remind what that was?
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    STUDENT: x minus x0--
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    PROFESSOR: x minus x0 squared
    plus y minus y0 squared
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    plus z minus z0 squared
    equals R squared.
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    OK?
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    When you ask, for
    example, what is
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    the equation of a units sphere,
    what do I mean by unit sphere?
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    STUDENT: Radius--
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    PROFESSOR: Radius 1, and
    center 0, standard unit sphere,
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    will be.
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    There is a notation for that
    in mathematics called s2.
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    I'll tell you why its called s2.
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    x squared plus y squared
    plus z squared equals 1.
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    s2 stands for the dimension.
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    That means the number
    of the-- the number
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    of degrees of freedom.
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    you have on a certain manifold.
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    What is a manifold?
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    It's a geometric structure.
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    I'm not going to
    go into details.
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    It's a geometric structure
    with some special properties.
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    I'm not talking about
    other fields of algebra,
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    anthropology.
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    I'm just talking about geometry
    and calculus math 3, which
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    is multivariable calculus.
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    Now, how do I think
    of degrees of freedom?
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    Look at the table.
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    What freedom do I have to move
    along one of these sticks?
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    I have one degree of
    freedom in the sense
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    that it's given by a
    parameter like time.
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    Right?
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    It's a 1-parameter
    manifold in the sense
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    that maybe I have
    a line, maybe I
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    have the trajectory of the
    parking space in terms of time.
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    The freedom that the bag has
    is to move according to time,
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    and that's considered only
    one degree of freedom.
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    Now if you were on a
    plane or another surface,
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    why would you have more
    than one degrees of freedom?
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    Well, I can move towards
    you, or I can move this way.
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    I can draw a grid the way
    the x and y coordinate.
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    And those are my
    degrees of freedom.
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    Practically, the basis
    IJ gives me that kind
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    of two degrees of freedom.
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    Right?
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    If I'm in three coordinates, I
    have without other constraints,
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    because I could be
    in three coordinates
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    and constrained to be on
    a cylinder, in which case
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    I still have two
    degrees of freedom.
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    But if I am a bug
    who is free to fly,
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    I have the freedom to go with
    three degrees of freedom,
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    right?
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    I have three degrees of
    freedom, but if the bug
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    is moving-- not flying,
    moving on a surface,
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    then he has two
    degrees of freedom.
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    So to again review, lines
    and curves in general
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    are one dimensional
    things, because you
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    have one degree of freedom.
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    Two dimensional
    things are surfaces,
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    three dimensional things are
    spaces, like the Euclidean
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    space, and we are not
    going to go beyond,
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    at least for the time
    being, we are not
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    going to go beyond that.
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    However, where anybody is
    interested in relativity,
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    say or let's say four
    dimensional spaces, or things
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    of x, y, z spatial coordinates
    and t as a fourth coordinate,
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    then we can go into higher
    dimensions, as well.
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    OK.
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    I want to ask you a question.
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    If somebody gives you on
    WeBWorK or outside of WeBWorK,
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    on the first quiz or
    on the final exam,
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    let's say you have
    this equation,
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    x squared plus y squared plus
    z squared plus 2x plus 2y
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    equals 9.
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    What is this identified as?
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    It's a quadric.
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    Why would this be a quadric?
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    Well, there is no x, y, y, z.
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    Those terms are missing.
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    But I have something of the
    type of quadric x squared
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    plus By squared plus
    c squared plus dxy
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    plus exz plus fyz plus, those
    are, oh my God, so many.
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    Degree two.
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    Degree one I would
    have ax plus by plus cz
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    plus a little d constant, and
    whew, that was a long one.
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    Right?
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    Now, is this of the
    type of a project?
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    Yes, it is.
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    Of course there are some terms
    that are missing, good for us.
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    How are you going to try to
    identify the type of quadric
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    by looking at this?
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    As you said very well,
    I think it's-- you say,
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    I think of a sphere, maybe I can
    complete the squares, you said.
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    How do we complete the squares?
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    x squared plus 2x plus
    some missing number,
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    a magic number-- yes sir?
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    STUDENT: So, basically I'll
    have to take x plus 2 times 4
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    will go outside.
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    It's like x min-- x plus 2--
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    PROFESSOR: Why x plus 2?
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    STUDENT: Because it's 2x--
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    STUDENT: It's 2x.
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    PROFESSOR: But if
    I take x plus 2,
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    then that's going to give
    me x squared plus 4x plus 4,
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    so it's not a good idea.
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    STUDENT: On the x plus 1
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    PROFESSOR: x plus 1.
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    So I'm going to complete
    x plus 1 squared.
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    What did I invent
    that wasn't there?
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    STUDENT: 1.
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    PROFESSOR: I invented
    the 1, and I have
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    to compensate for my invention.
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    I added the 1, created
    the 1 out of nothing,
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    so I have to compensate
    by subtracting it.
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    How much is from here to here?
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    Is it exactly the
    thing that I underlined
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    with a wiggly line, a
    light wiggly line thing,
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    plus what is the
    blue wiggly line,
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    the blue wiggly line
    that doesn't show--
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    I have y plus 1 squared, and
    again, I have to compensate
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    for what I invented.
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    I created a 1 out of nothing,
    so this is y squared plus 2y.
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    The z squared is all by himself,
    and he's crying, I'm so lonely,
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    I don't know, there is
    nobody like me over there.
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    So in the end, I can rewrite
    the whole thing as x plus 1
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    squared plus y plus 1
    squared plus z squared, if I
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    want to work them out in
    this format, equals what?
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    STUDENT: 10.
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    PROFESSOR: 11.
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    11 is the square
    root of 11 squared.
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    Like my son said the other day.
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    So that the radius
    would be square foot
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    11 of a sphere of what circle?
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    What is the-- or the
    sphere of what center?
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    STUDENT: Minus 1--
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    PROFESSOR: Minus
    1, minus 1, and 0.
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    So I don't want to insult you.
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    Of course you know how
    to complete squares.
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    However, I have discovered in an
    upper level class at some point
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    that my students didn't know
    how to complete squares, which
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    was very, very heartbreaking.
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    All right, now.
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    Any questions regarding--
    while I have a few of yours,
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    I'm going to wait
    a little bit longer
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    until I give
    everybody the chance
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    to complete the extra credit.
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    I have the question
    by email saying,
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    you mentioned that
    genius guy in your class.
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    This is a 1-sheeted hyperboloid.
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    x squared plus y squared minus
    z squared minus 1 equals 0.
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    The question was, by
    email, how in the world,
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    did he figure out what the two
    families of generatrices are?
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    So you have one family
    and another family,
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    and both together generate
    the 1-sheeted hyperboloid.
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    Let me give you a little
    bit more of a hint,
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    but I'm still going to stop.
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    So last time I said, he
    noticed you can root together
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    the y squared minus 1 and the
    x squared minus z squared,
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    and you can separate them.
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    So you're going to have x
    squared minus z squared equals
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    1 minus y squared.
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    You can't hide the
    difference of two squares
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    as product of sum
    and difference.
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    x plus z times x minus z equals
    1 plus y times 1 minus y.
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    So how can you
    eventually arrange stuff
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    to be giving due
    to the lines that
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    are sitting on the surface?
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    The lines that are
    sitting on the surface
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    are infinitely many,
    and I would like
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    at least a 1-parameter
    family of such lines.
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    You can have choices.
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    One of the choices
    would be-- this
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    is a product, of
    two numbers, right?
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    So you can write it as an
    equality of two fractions.
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    So you would have something
    like x plus z on top, x minus
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    z below.
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    Observe that you are
    creating singularities here.
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    So you have to take x minus
    z case equals 0 separately,
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    and then you have, let's
    say you have 1 minus y here,
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    and 1 plus y here.
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    What else do you have to impose
    when you impose x minus z
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    equals 0.
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    You cannot have 7 over 0.
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    That is undefined.
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    but if you have 0 over
    0, that's still possible.
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    So whenever you take x
    minus z equals 0 separately,
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    that will imply that the
    numerator corresponding to it
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    will also have to be 0.
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    And together these
    guys are friends.
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    What are they?
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    2--
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    STUDENT: A system of equations.
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    PROFESSOR: It's a
    system of equations.
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    They both represent planes, and
    the intersection of two planes
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    is a line.
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    It's a particular line, which
    is part of the family-- which
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    is part of a family.
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    OK.
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    Now, on the other hand, in case
    you have 1 plus y equals 0--
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    so if it happens that you
    have this extreme case
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    that the denominator
    will be 0, you absolutely
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    have to impose x plus z to be 0,
    and then you have another life.
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    It's not easy for
    me to draw those,
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    but I could if you
    asked me privately
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    to draw those and show you
    what the lines look like.
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    OK?
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    All right.
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    So you have two special lines
    that are part of that picture.
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    They are embedded
    in the surface.
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    How do you find a
    family of planes?
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    Oh my god, I only
    had one choice,
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    but I could have
    yet another choice
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    of how to pick the parameters.
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    Let's take lambda to be
    a real number parameter.
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    And lambda could be
    anything-- if lambda is 0,
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    what have I got to have, guys?
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    STUDENT: The top.
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    PROFESSOR: The top
    guys will be 0,
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    and I still have 1 minus y
    equals 0, a plane, intersected
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    with x plus z equals 0,
    another plane, so still a line.
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    So lambda equals 0 will give
    me yet another line, which
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    is not written big.
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    Are you guys with me?
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    Could lambda ever
    go to infinity?
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    Lambda wants to go to
    infinity, and when does lambda
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    go to infinity?
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    STUDENT: When the
    bottoms would equal 0--
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    PROFESSOR: When both
    the bottoms would be 0.
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    So this is-- I can call it L
    infinity, the line of infinity.
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    You see?
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    But still those
    would be two planes.
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    There's an intersection,
    it's a line.
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    OK.
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    Can we write this family--
    just one family of lines?
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    A line is always an intersection
    of two planes, right?
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    So which are the planes
    that I'm talking about?
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    x plus z equals
    lambda times 1 plus y.
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    This is not in the book,
    because, oh my God, this is
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    too hard for the book, right?
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    But it's a nice example to
    look at in an honors class.
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    1 minus y equals
    lambda times x minus z.
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    It's not in the book.
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    It's not in any book that I know
    of at the level of calculus.
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    All right, OK.
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    What are these animals?
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    The first animal is a plane.
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    The second animal is a plane.
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    How many planes
    are in the picture?
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    For each lambda, you have a--
    for each lambda value in R,
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    you have a couple of planes
    that intersect along your line.
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    This is the line L lambda.
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    And shut up, Magdalena,
    you told people too much.
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    If you still want them to do
    this for 2 extra credit points,
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    give them the chance
    to finish the exercise.
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    So I zip my lips, but
    only after I ask you,
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    how do you think
    you are going to get
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    the other family of rulers?
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    The ruling guys are
    two families, you see?
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    So this family is
    going in one direction.
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    How am I going to
    get two families?
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    I have another choice
    that-- how did I take this?
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    More or less, I made my choice.
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    Just like having two
    people that would
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    be prospective job candidates.
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    You pick one of them.
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    STUDENT: Now, we can put 1
    minus y in the denominator.
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    The denominator in
    place of 1 plus y.
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    PROFESSOR: So I could have
    done-- I could have taken this,
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    and put 1 plus y here,
    and 1 minus y here.
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    I'm going to let
    you do the rest,
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    and get the second
    family of generators
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    for the whole surface.
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    That's enough.
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    You're not missing your credit.
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    Just, you wanted help,
    and I helped you.
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    And I'm not mad whatsoever
    when you ask me things.
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    The email I got sounded like--
    says, this is not in the book,
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    or in any book, or
    on the internet.
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    How shall I approach this?
  • 18:49 - 18:51
    How shall I start thinking
    about this problem?
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    This is a completely
    legitimate question.
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    How do I start on this problem?
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    OK.
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    On the homework-- maybe it's
    too easy-- you have two or three
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    examples involving spheres.
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    Those will be too easy for you.
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    I only gave you a very thin
    among of homework this time.
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    You Have plenty of time until
    Monday at 1:30 or something PM.
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  • 19:19 - 19:21
    I would like to draw
    a little bit more,
  • 19:21 - 19:25
    because in this homework
    and the next homework,
  • 19:25 - 19:33
    I'm building something special
    called the Frenet Trihedron.
  • 19:33 - 19:37
    And I told you a little bit
    about this Frenet Trihedron,
  • 19:37 - 19:40
    but I didn't tell you much.
  • 19:40 - 19:43
  • 19:43 - 19:46
    Many textbooks in
    multivariable calculus
  • 19:46 - 19:49
    don't say much about it,
    which I think is a shame.
  • 19:49 - 19:53
  • 19:53 - 19:57
    You have a position
    vector that gives you
  • 19:57 - 19:59
    the equation of a regular curve.
  • 19:59 - 20:06
  • 20:06 - 20:08
    x of t, y of t, z of t.
  • 20:08 - 20:10
    Again, what was a regular curve?
  • 20:10 - 20:14
    I'm just doing review of
    what we did last time.
  • 20:14 - 20:17
    A very nice curve
    that is differentiable
  • 20:17 - 20:22
    and whose derivative is
    continuous everywhere
  • 20:22 - 20:23
    on the interval.
  • 20:23 - 20:31
    But moreover, the r prime
    of t never becomes 0.
  • 20:31 - 20:36
    So continuously differentiable,
    and r prime of t
  • 20:36 - 20:41
    never becomes 0 for any--
    do you know this name,
  • 20:41 - 20:43
    any for every or for any?
  • 20:43 - 20:44
    OK.
  • 20:44 - 20:47
    This is the symbolistics
    of mathematics.
  • 20:47 - 20:50
    You know because you
    are as nerdy as me.
  • 20:50 - 20:52
    But everybody else doesn't.
  • 20:52 - 20:54
    You guys will learn.
  • 20:54 - 20:56
    This is what
    mathematicians like.
  • 20:56 - 21:00
    You see, mathematicians hate
    writing lots of words down.
  • 21:00 - 21:05
    If we liked writing essays
    and lots of blah, blah, blah,
  • 21:05 - 21:07
    we would do something else.
  • 21:07 - 21:09
    We wouldn't do mathematics.
  • 21:09 - 21:11
    We would do debates,
    we would do politics,
  • 21:11 - 21:14
    we would do other things.
  • 21:14 - 21:17
    Mathematicians like
    ideas, but when
  • 21:17 - 21:19
    it comes to writing
    them down, they
  • 21:19 - 21:23
    want to right them down in
    the most compact way possible.
  • 21:23 - 21:26
    That's why they created
    sort of their own language,
  • 21:26 - 21:31
    and they have all sorts
    of logical quantifiers.
  • 21:31 - 21:34
    And it's like your
    secret language
  • 21:34 - 21:37
    when it comes to your
    less nerdy friends.
  • 21:37 - 21:45
    So you go for every--
    for any or for every--
  • 21:45 - 21:46
    do you know this sign?
  • 21:46 - 21:49
  • 21:49 - 21:50
    There exists.
  • 21:50 - 21:55
  • 21:55 - 21:57
    And do you know this thing?
  • 21:57 - 22:01
    Because one of the-- huh?
  • 22:01 - 22:03
    STUDENT: Is that factorial?
  • 22:03 - 22:05
    PROFESSOR: Factorial,
    but in logic,
  • 22:05 - 22:09
    that means there exists
    a unique-- a unique.
  • 22:09 - 22:11
    So there exists a unique.
  • 22:11 - 22:15
    There exists a unique number.
  • 22:15 - 22:19
    There is a unique number.
  • 22:19 - 22:21
    So we have our own language.
  • 22:21 - 22:24
    Of course, empty set,
    everybody knows that.
  • 22:24 - 22:28
    And it's used in
    mathematical logic a lot.
  • 22:28 - 22:33
    You know most of the symbols
    from unit intersection,
  • 22:33 - 22:35
    or, and.
  • 22:35 - 22:39
    I'm going to use some
    of those as well.
  • 22:39 - 22:40
    Coming back to the
    Frenet Trihedron,
  • 22:40 - 22:44
    we have that velocity
    vector at every point.
  • 22:44 - 22:45
    We are happy with it.
  • 22:45 - 22:49
    We have our prime of t
    that is referred from 0.
  • 22:49 - 22:51
    I said I want to
    make it uniform,
  • 22:51 - 22:54
    and then I divided
    by the magnitude,
  • 22:54 - 22:58
    and I have this wonderful t
    vector we just talked about.
  • 22:58 - 23:04
    Mr. t is r prime over the
    magnitude of r prime, which
  • 23:04 - 23:07
    is called it's peak right?
  • 23:07 - 23:10
    We divide by its peak.
  • 23:10 - 23:13
    What's the name of t, again?
  • 23:13 - 23:14
    STUDENT: Tangent unit--
  • 23:14 - 23:16
    PROFESSOR: Tangent
    unit vector, very good.
  • 23:16 - 23:20
    How did you remember
    that so quickly?
  • 23:20 - 23:22
    Tangent unit vector.
  • 23:22 - 23:28
    There is also another
    guy who is famous.
  • 23:28 - 23:33
    I wanted to make him
    green, but let's see
  • 23:33 - 23:35
    if I can make him blue.
  • 23:35 - 23:42
    t is defined-- should I
    write the f on top of here?
  • 23:42 - 23:44
    Do you know what that is?
  • 23:44 - 23:46
    STUDENT: I thought n
    was the normal vector.
  • 23:46 - 23:48
    PROFESSOR: t prime
    divided by the length of--
  • 23:48 - 23:49
    STUDENT: Wait.
  • 23:49 - 23:53
    I thought the vector
    n was the normal.
  • 23:53 - 23:56
    PROFESSOR: n-- there
    are many normals.
  • 23:56 - 24:01
    It's a very good thing, because
    we don't say that in the book.
  • 24:01 - 24:05
    OK, this is the t along my r.
  • 24:05 - 24:09
    Now when I go through a point,
    this is the normal plane,
  • 24:09 - 24:10
    right?
  • 24:10 - 24:15
    There are many normals to
    the surface-- to the curve.
  • 24:15 - 24:16
    Which one am I taking?
  • 24:16 - 24:20
    All of them are perpendicular
    to the direction, right?
  • 24:20 - 24:20
    STUDENT: tf.
  • 24:20 - 24:22
    PROFESSOR: So I take
    this one, or this one,
  • 24:22 - 24:25
    or this one, or this one, or
    this one, or this one, there.
  • 24:25 - 24:27
    I have to make up my mind.
  • 24:27 - 24:31
    And that's how people came up
    with the so-called principal
  • 24:31 - 24:33
    unit normal.
  • 24:33 - 24:36
    And this is the one
    I'm talking about.
  • 24:36 - 24:39
    And you are right, it is normal.
  • 24:39 - 24:42
    Principal unit normal.
  • 24:42 - 24:45
    Remember this very
    well for your exam,
  • 24:45 - 24:48
    because it's a very
    important notion.
  • 24:48 - 24:50
    How do I get to that?
  • 24:50 - 24:54
    I take t, I differentiate
    it, and I divide
  • 24:54 - 24:59
    by the lengths of t prime.
  • 24:59 - 25:07
    Now, can you prove to me
    that indeed this fellow
  • 25:07 - 25:10
    is perpendicular to t?
  • 25:10 - 25:12
    Can you do that?
  • 25:12 - 25:14
    STUDENT: That n is
    perpendicular to t?
  • 25:14 - 25:16
    PROFESSOR: Mm-hmm.
  • 25:16 - 25:18
    So a little exercise.
  • 25:18 - 25:23
  • 25:23 - 25:31
    Prove that-- Prove that I don't
    have a good marker anymore.
  • 25:31 - 25:38
    Prove that n, the unit
    principal vector field,
  • 25:38 - 25:45
    is perpendicular-- you
    see, I'm a mathematician.
  • 25:45 - 25:49
    I swear, I hate to write down
    the whole word perpendicular.
  • 25:49 - 25:52
    I would love to
    say, perpendicular.
  • 25:52 - 25:58
    That's how I write perpendicular
    really fast-- to t fore
  • 25:58 - 26:01
    every value of t.
  • 26:01 - 26:03
    For every value of t.
  • 26:03 - 26:04
    OK.
  • 26:04 - 26:06
    How in the world can I do that?
  • 26:06 - 26:09
    I have to think about it.
  • 26:09 - 26:12
    This is hard.
  • 26:12 - 26:13
    Wish me luck.
  • 26:13 - 26:16
    So do I know
    anything about Mr. t?
  • 26:16 - 26:18
    What do I know about Mr. t?
  • 26:18 - 26:20
    I'll take it and I'll
    differentiate it later.
  • 26:20 - 26:25
    It Mr. t is magic in the
    sense that he's a unit vector.
  • 26:25 - 26:28
    I'm going to write that down.
  • 26:28 - 26:32
    t in absolute value equals 1.
  • 26:32 - 26:33
    It's beautiful.
  • 26:33 - 26:37
    If I squared that-- and
    you're going to say,
  • 26:37 - 26:39
    why would you want
    to square that?
  • 26:39 - 26:40
    You're going to see in a minute.
  • 26:40 - 26:43
    If I squared that,
    then I'm going
  • 26:43 - 26:51
    to have the dot product
    between t and itself equals 1.
  • 26:51 - 26:53
  • 26:53 - 26:57
    Can somebody tell me why the
    dot product between t and itself
  • 26:57 - 27:01
    is the square of a length of t?
  • 27:01 - 27:05
    What's the definition
    of the dot product?
  • 27:05 - 27:08
    Magnitude of the first
    vector, times the magnitude
  • 27:08 - 27:11
    of the second vector--
    there i am already--
  • 27:11 - 27:15
    times the cosine of the
    angle between the two vectors
  • 27:15 - 27:17
    Duh, that's 0.
  • 27:17 - 27:20
    So cosine of 0 is 1, I'm done.
  • 27:20 - 27:21
    Right?
  • 27:21 - 27:27
    Now, I have a vector function
    times a vector function--
  • 27:27 - 27:31
    this is crazy, right-- equals 1.
  • 27:31 - 27:34
    I'm going to go ahead
    and differentiate.
  • 27:34 - 27:38
    Keep in mind that
    this is a product.
  • 27:38 - 27:40
    What's the product?
  • 27:40 - 27:42
    One of my professors,
    colleagues,
  • 27:42 - 27:45
    was telling me, now,
    let's be serious.
  • 27:45 - 27:49
    In five years, how many
    of your engineering majors
  • 27:49 - 27:51
    will remember the product?
  • 27:51 - 27:53
    I really was
    thinking about this.
  • 27:53 - 27:57
    I hope everybody, if
    they were my students,
  • 27:57 - 27:59
    because we are going to
    have enough practice.
  • 27:59 - 28:02
    So the prime rule in
    Calc 1 said that if you
  • 28:02 - 28:05
    have f of t times g of
    t, you have a product.
  • 28:05 - 28:08
    You prime that product,
    and never write
  • 28:08 - 28:13
    f prime times g prime unless you
    want me to call you around 2 AM
  • 28:13 - 28:15
    to say you should never do that.
  • 28:15 - 28:20
  • 28:20 - 28:24
    So how does the
    product rule work?
  • 28:24 - 28:28
    The first one prime
    times the second unprime
  • 28:28 - 28:32
    plus the first one unprime
    times the second prime.
  • 28:32 - 28:35
    My students know
    the product rule.
  • 28:35 - 28:37
    I don't care if the rest
    of the world doesn't.
  • 28:37 - 28:40
    I don't care about any
    community college who
  • 28:40 - 28:43
    would say, I don't want the
    product rule to be known,
  • 28:43 - 28:45
    you can differentiate
    with a calculator.
  • 28:45 - 28:46
    That's a no, no, no.
  • 28:46 - 28:50
    You don't know calculus if you
    don't know the product rule.
  • 28:50 - 28:53
    So the product rule is
    a blessing from God.
  • 28:53 - 28:58
    It helps everywhere in physics,
    in mechanics, in engineering.
  • 28:58 - 29:01
    It really helps in
    differential geometry
  • 29:01 - 29:04
    with the directional
    derivative, the Lie derivative.
  • 29:04 - 29:08
    It helps you understand all
    the upper level mathematics.
  • 29:08 - 29:12
    Now here you have t prime,
    the first prime times
  • 29:12 - 29:16
    the second unprime, plus the
    first unprime times the second
  • 29:16 - 29:17
    prime.
  • 29:17 - 29:21
    It's the same as for
    regular scalar functions.
  • 29:21 - 29:24
    What's the derivative of 1?
  • 29:24 - 29:24
    STUDENT: 0.
  • 29:24 - 29:26
    PROFESSOR: 0.
  • 29:26 - 29:27
    Look at this guy!
  • 29:27 - 29:29
    Doesn't he look funny?
  • 29:29 - 29:33
    It is the dot product community.
  • 29:33 - 29:34
    Yes it is, by definition.
  • 29:34 - 29:40
    So you have twice T
    times T prime equals 0.
  • 29:40 - 29:44
    This 2 is-- stinking
    guy, let's divide by 2.
  • 29:44 - 29:45
    Forget about that.
  • 29:45 - 29:47
    What does this say?
  • 29:47 - 29:54
    The dot product of T times--
    I mean by T prime is 0.
  • 29:54 - 29:57
    When are two vectors
    giving you dot product 0?
  • 29:57 - 29:59
    STUDENT: When they're
    perpendicular.
  • 29:59 - 30:00
  • 30:00 - 30:02
    PROFESSOR: So if both
    of them are non-zero,
  • 30:02 - 30:03
    they have to be like that.
  • 30:03 - 30:06
    They have to be like this,
    perpendicular, right?
  • 30:06 - 30:12
    So it follows that t has to
    be perpendicular to T prime.
  • 30:12 - 30:16
    And now, that's why n
    is perpendicular to t.
  • 30:16 - 30:19
    But, because n is
    collinear to t prime.
  • 30:19 - 30:20
    Hello.
  • 30:20 - 30:22
    n is collinear to t prime.
  • 30:22 - 30:26
    So this is t prime.
  • 30:26 - 30:28
    Is t prime unitary?
  • 30:28 - 30:29
    I'm going to measure it.
  • 30:29 - 30:31
    No it's not.
  • 30:31 - 30:32
    t prime.
  • 30:32 - 30:34
    So if I want to
    make it unitary, I'm
  • 30:34 - 30:36
    going to chop my-- no,
    I'm not going to chop.
  • 30:36 - 30:40
    I just take it, t prime,
    and divide by its magnitude.
  • 30:40 - 30:43
    Then I'm going to get that
    vector n, which is unitary.
  • 30:43 - 30:48
    So from here it follows that t
    and n are indeed perpendicular,
  • 30:48 - 30:53
    and your colleague over there
    said, hey, it has to be normal.
  • 30:53 - 30:55
    That's perpendicular
    to t, but which one?
  • 30:55 - 30:58
    A special one, because
    I have many normals.
  • 30:58 - 31:02
    Now, this special one is
    easy to find like that.
  • 31:02 - 31:06
    Where shall I put here--
    I'll draw him very nicely.
  • 31:06 - 31:09
  • 31:09 - 31:10
    I'll draw him.
  • 31:10 - 31:13
    Now you guys have to
    imagine-- am I drawing
  • 31:13 - 31:15
    well enough for you?
  • 31:15 - 31:16
    I don't even know.
  • 31:16 - 31:18
    t and n should be perpendicular.
  • 31:18 - 31:22
    Can you imagine them having that
    90 degree angle between them?
  • 31:22 - 31:22
    OK.
  • 31:22 - 31:27
    Now there is a magic one that
    you don't even have to define.
  • 31:27 - 31:29
    And yes sir?
  • 31:29 - 31:31
    STUDENT: In this
    thing, can [INAUDIBLE]
  • 31:31 - 31:34
    this T vector [INAUDIBLE]
    written by the definition
  • 31:34 - 31:36
    thing?
  • 31:36 - 31:38
    PROFESSOR: No.
  • 31:38 - 31:39
    STUDENT: N vector
    times the magnitude
  • 31:39 - 31:42
    of t vector derivative?
  • 31:42 - 31:47
    PROFESSOR: So
    technically you have
  • 31:47 - 31:51
    t prime would be the
    magnitude of t prime times n.
  • 31:51 - 31:52
    STUDENT: Yes.
  • 31:52 - 31:54
    PROFESSOR: But keep in mind
    that sometimes is tricky,
  • 31:54 - 31:57
    because this is, in
    general, not a constant.
  • 31:57 - 31:59
    Always keep it in mind,
    it's not a constant.
  • 31:59 - 32:02
    We'll have some examples later.
  • 32:02 - 32:05
    There is a magic
    guy called binormal.
  • 32:05 - 32:10
    That binormal is the
    normal to both t and n.
  • 32:10 - 32:12
    And he's defined as
    t plus n because it's
  • 32:12 - 32:14
    normal to both of them.
  • 32:14 - 32:18
    So I'm going to write this
    b vector is t cross n.
  • 32:18 - 32:22
    Now I'm asking you to draw it.
  • 32:22 - 32:24
    Can anybody come to
    the board and draw it
  • 32:24 - 32:27
    for 0.01 extra credit?
  • 32:27 - 32:30
    Yes, sir?
  • 32:30 - 32:31
    STUDENT: [INAUDIBLE]
  • 32:31 - 32:35
    PROFESSOR: Draw that on the
    picture like t and n, t and n,
  • 32:35 - 32:38
    t is the-- who the heck
    is t? t is the red one,
  • 32:38 - 32:41
    and blue is the n.
  • 32:41 - 32:43
    So does it go down or up?
  • 32:43 - 32:46
    We should be perpendicular
    to both of them.
  • 32:46 - 32:49
    Is b unitary or not?
  • 32:49 - 32:52
    If you have two unit vectors,
    will the cross product
  • 32:52 - 32:53
    be a unit vector?
  • 32:53 - 32:56
  • 32:56 - 33:00
    Only if the two vectors
    are perpendicular,
  • 33:00 - 33:05
    it is going to be, right?
  • 33:05 - 33:12
    So you have-- well, I
    think it goes that--
  • 33:12 - 33:14
    in which direction does it go?
  • 33:14 - 33:15
    Because
  • 33:15 - 33:16
    STUDENT: It should
    not be how we have it.
  • 33:16 - 33:17
    PROFESSOR: No, no, no.
  • 33:17 - 33:18
    Because this is--
  • 33:18 - 33:19
    STUDENT: Yeah.
  • 33:19 - 33:20
    I'm using--
  • 33:20 - 33:23
    PROFESSOR: So t
    goes over n, so I'm
  • 33:23 - 33:27
    going to try-- it is
    like that, sort of.
  • 33:27 - 33:29
    STUDENT: Into the chord?
  • 33:29 - 33:31
    PROFESSOR: So again, it's
    not very clear because
  • 33:31 - 33:34
    of my stinking art, here.
  • 33:34 - 33:36
    It's really not nice art.
  • 33:36 - 33:40
    t, and this is n.
  • 33:40 - 33:44
    And if I go t going over n.
  • 33:44 - 33:48
    T going over n goes up or down?
  • 33:48 - 33:48
    STUDENT: Down.
  • 33:48 - 33:49
    PROFESSOR: Goes down.
  • 33:49 - 33:52
    So it's going to look
    more like this, feet.
  • 33:52 - 33:55
    Now guys, when we--
    thank you so much.
  • 33:55 - 33:58
    So you've like a
    0.01 extra credit.
  • 33:58 - 34:01
    OK.
  • 34:01 - 34:03
    Tangent, normal, and
    binormal form a corner.
  • 34:03 - 34:04
    Yes, sir?
  • 34:04 - 34:07
    STUDENT: Is rt-- rt is
    the function at the--
  • 34:07 - 34:09
    for the flag that's flying?
  • 34:09 - 34:12
    PROFESSOR: The r of t
    is the position vector
  • 34:12 - 34:15
    of the flag that was
    flying that he was drunk.
  • 34:15 - 34:21
    STUDENT: Why wasn't the
    derivative of it perpendicular?
  • 34:21 - 34:24
    Why isn't t perpendicular to rt?
  • 34:24 - 34:26
    PROFESSOR: If--
    well, good question.
  • 34:26 - 34:29
  • 34:29 - 34:31
    We'll talk about it.
  • 34:31 - 34:35
    If the length of r
    would be a constant,
  • 34:35 - 34:39
    can we prove that r and r
    prime are perpendicular?
  • 34:39 - 34:41
    Let's do that as
    another exercise.
  • 34:41 - 34:43
    All right?
  • 34:43 - 34:46
    So tnb looks like a corner.
  • 34:46 - 34:52
    Look at the corner that the
    video cannot see over there.
  • 34:52 - 34:54
    TN and B are mutually octagonal.
  • 34:54 - 34:56
  • 34:56 - 34:58
    I'm going to draw them.
  • 34:58 - 35:01
    This is an arbitrary
    point on a curve,
  • 35:01 - 35:04
    and this is t, which is
    always tangent to the curve,
  • 35:04 - 35:06
    and this is n.
  • 35:06 - 35:08
    Let's say that's the
    unit principle normal.
  • 35:08 - 35:11
    And t cross n will
    go, again, down.
  • 35:11 - 35:12
    I don't know.
  • 35:12 - 35:15
    I have an obsession
    with me going down.
  • 35:15 - 35:16
    This is called the
    Frenet Trihedron.
  • 35:16 - 35:20
  • 35:20 - 35:23
    And I have a proposal
    for a problem
  • 35:23 - 35:35
    that maybe I should give
    my students in the future.
  • 35:35 - 35:46
    Show that for a circle,
    playing in space, I don't know.
  • 35:46 - 36:07
    The position vector and the
    velocity vector are always how?
  • 36:07 - 36:08
    Friends.
  • 36:08 - 36:09
    Let's say friends.
  • 36:09 - 36:12
    No, come on, I'm kidding.
  • 36:12 - 36:13
    How are they?
  • 36:13 - 36:15
    STUDENT: Perpendicular.
  • 36:15 - 36:17
    PROFESSOR: How do you do that?
  • 36:17 - 36:18
    Is it hard?
  • 36:18 - 36:21
    We should be smart
    enough to do that, right?
  • 36:21 - 36:22
    I have a circle.
  • 36:22 - 36:26
    That circle has what-- what
    is the property of a circle?
  • 36:26 - 36:30
    Euclid defined that-- this is
    one of the axioms of Euclid.
  • 36:30 - 36:32
    Does anybody know which axiom?
  • 36:32 - 36:36
    That there exists
    such a set of points
  • 36:36 - 36:39
    that are all at the same
    distance from a given point
  • 36:39 - 36:41
    called center.
  • 36:41 - 36:43
    So that is a circle, right?
  • 36:43 - 36:44
    That's what Mr. Euclid said.
  • 36:44 - 36:45
    He was a genius.
  • 36:45 - 36:52
    So no matter where I put that
    circle, I can take r of t
  • 36:52 - 36:55
    in magnitude measured
    from the origin
  • 36:55 - 36:57
    from the center of the circle.
  • 36:57 - 37:01
    Keep in mind, always the
    center of the circle.
  • 37:01 - 37:06
    I put it at the origin of the
    space-- origin of the universe.
  • 37:06 - 37:08
    No, origin of the
    space, actually.
  • 37:08 - 37:13
    R of T magnitude
    would be a constant.
  • 37:13 - 37:14
    Give me a constant, guys.
  • 37:14 - 37:14
    OK?
  • 37:14 - 37:16
    It doesn't matter.
  • 37:16 - 37:18
    Let me draw.
  • 37:18 - 37:20
    I want to draw in plane, OK?
  • 37:20 - 37:26
    Because I'm getting tired.
    x y, and this is r of t,
  • 37:26 - 37:30
    and the magnitude of this r of
    t is the radius of the circle.
  • 37:30 - 37:33
    Right?
  • 37:33 - 37:37
    So let's say, this is
    the radius of the circle.
  • 37:37 - 37:41
  • 37:41 - 37:44
    How in the world do I
    prove the same idea?
  • 37:44 - 37:48
    Who helps me prove
    that r is always
  • 37:48 - 37:51
    perpendicular to r prime?
  • 37:51 - 37:54
    Which way do you want to move,
    counterclockwise or clockwise?
  • 37:54 - 37:55
    STUDENT: Counterclockwise.
  • 37:55 - 37:56
    PROFESSOR: Counterclockwise.
  • 37:56 - 37:58
    Because if you are
    a real scientist,
  • 37:58 - 38:00
    I'm proud of you guys.
  • 38:00 - 38:02
    It's clear from the
    picture that r prime
  • 38:02 - 38:05
    would be perpendicular to r.
  • 38:05 - 38:06
    Why is that?
  • 38:06 - 38:08
    How am I going to do that?
  • 38:08 - 38:12
    Now, mimic everything I--
    don't look at your notes,
  • 38:12 - 38:17
    and try to tell me how
    I show that quickly.
  • 38:17 - 38:18
    What am I going to do?
  • 38:18 - 38:23
    So all I know, all
    that gave me was r of t
  • 38:23 - 38:28
    equals k in magnitude constant.
  • 38:28 - 38:31
    For every t, this same constant.
  • 38:31 - 38:32
    What's next?
  • 38:32 - 38:35
    What do I want to do next?
  • 38:35 - 38:36
    STUDENT: Square it?
  • 38:36 - 38:38
    PROFESSOR: Square
    it, differentiate it.
  • 38:38 - 38:40
    I can also go ahead
    and differentiate it
  • 38:40 - 38:42
    without squaring
    it, but that's going
  • 38:42 - 38:47
    to be a little bit of more pain.
  • 38:47 - 38:52
    So square it, differentiate it.
  • 38:52 - 38:53
    I'm too lazy.
  • 38:53 - 38:56
    When I differentiate,
    what am I going to get?
  • 38:56 - 39:05
    From the product rule, twice
    r dot r primed of t equals 0.
  • 39:05 - 39:07
    Well, I'm done.
  • 39:07 - 39:12
    Because it means that for
    every t that radius-- not
  • 39:12 - 39:13
    the radius, guys, I'm sorry.
  • 39:13 - 39:17
    The position vector will be
    perpendicular to the velocity
  • 39:17 - 39:18
    vector.
  • 39:18 - 39:22
    Now, if I draw the
    trajectory of my drunken flag
  • 39:22 - 39:25
    this [INAUDIBLE]
    is not true, right?
  • 39:25 - 39:27
    This is crazy.
  • 39:27 - 39:30
    Of course this is r,
    and this is r prime,
  • 39:30 - 39:36
    and there is an arbitrary
    angle between r and r prime.
  • 39:36 - 39:38
    The good thing is that
    the arbitrary angle always
  • 39:38 - 39:41
    exists, and is
    continuous as a function.
  • 39:41 - 39:43
    I never have that
    angle disappear.
  • 39:43 - 39:47
    That's way I want that
    prime never to become 0.
  • 39:47 - 39:49
    Because if the bag was
    stopping its motion,
  • 39:49 - 39:54
    goodbye angle, goodbye
    analysis, right?
  • 39:54 - 39:55
    OK.
  • 39:55 - 39:56
    Very nice.
  • 39:56 - 39:57
    So don't give me more ideas.
  • 39:57 - 40:00
    You smart people, if
    you give me more ideas,
  • 40:00 - 40:03
    I'm going to come up with
    all sorts of problems.
  • 40:03 - 40:05
    And this is actually one
    of the first problems
  • 40:05 - 40:09
    you learn in a graduate
    level geometry class.
  • 40:09 - 40:14
  • 40:14 - 40:17
    Let me give you another
    piece of information
  • 40:17 - 40:20
    that you're going
    to love, which could
  • 40:20 - 40:22
    be one of those
    types of combined
  • 40:22 - 40:25
    problems on a final
    exam or midterm,
  • 40:25 - 40:30
    A, B, C, D, E. The
    curvature of a curve
  • 40:30 - 40:34
    is a measure of how
    the curve will bend.
  • 40:34 - 40:36
    Say what?
  • 40:36 - 40:46
    The curvature of a
    curve is a measure
  • 40:46 - 40:49
    of the bending of that curve.
  • 40:49 - 40:59
  • 40:59 - 41:04
    By definition, you have
    to take it like that.
  • 41:04 - 41:21
    If the curve is parameterized
    in arc length-- somebody
  • 41:21 - 41:23
    remind me what that is.
  • 41:23 - 41:25
    What does it mean?
  • 41:25 - 41:32
    That is r of s such
    that-- what does it mean,
  • 41:32 - 41:34
    parameterizing arc length--
  • 41:34 - 41:35
    STUDENT: r prime of s.
  • 41:35 - 41:37
    PROFESSOR: r primed of
    s in magnitude is 1.
  • 41:37 - 41:38
    The speed 1.
  • 41:38 - 41:39
    It's a speed 1 curve.
  • 41:39 - 41:43
  • 41:43 - 42:01
    Then, the curvature of this
    curve is defined as k of s
  • 42:01 - 42:06
    equals the magnitude of
    the acceleration vector
  • 42:06 - 42:09
    will respect the S.
    Say what, Magdalena?
  • 42:09 - 42:13
    I can also write
    it magnitude of d--
  • 42:13 - 42:17
    oh my gosh, second derivative
    with respect s of r.
  • 42:17 - 42:20
    I'll do it right now. d2r ds2.
  • 42:20 - 42:22
    And I know you get
    a headache when
  • 42:22 - 42:26
    I solve, when I write that,
    because you are not used to it.
  • 42:26 - 42:33
    A quick and beautiful example
    that can be on the homework,
  • 42:33 - 42:39
    and would also be on the
    exam, maybe on all the exams,
  • 42:39 - 42:42
    I don't know.
  • 42:42 - 42:48
    Compute the curvature of a
    circle of radius a Say what?
  • 42:48 - 43:03
    Compute the curvature of a
    circle of radius a And you say,
  • 43:03 - 43:04
    wait a minute.
  • 43:04 - 43:07
    For a circle of
    radius a in plane--
  • 43:07 - 43:09
    why can I assume it's in plane?
  • 43:09 - 43:13
    Because if the circle
    is a planar curve,
  • 43:13 - 43:16
    I can always assume
    it to be in plane.
  • 43:16 - 43:19
    And it has radius a I
    can find infinitely many
  • 43:19 - 43:20
    parameterizations.
  • 43:20 - 43:23
    So what, am I crazy?
  • 43:23 - 43:25
    Well, yes, I am, but
    that's another story.
  • 43:25 - 43:28
    Now, if I want to
    parameterize, I
  • 43:28 - 43:31
    have to parameterize
    in arc length.
  • 43:31 - 43:34
    If I do anything else,
    that means I'm stupid.
  • 43:34 - 43:39
    So, r of s will be what?
  • 43:39 - 43:41
    Can somebody tell me
    how I parameterize
  • 43:41 - 43:46
    a curve in arc length
    for a-- what is this guy?
  • 43:46 - 43:49
    A circle of radius a.
  • 43:49 - 43:51
    Yeah, I cannot do it.
  • 43:51 - 43:52
    I'm not smart enough.
  • 43:52 - 43:59
    So I'll say R of T will be
    a cosine t, a sine t and 0.
  • 43:59 - 44:03
    And here I stop, because
    I had a headache.
  • 44:03 - 44:09
    t is from 0 to 2 pi, and
    I think this a is making
  • 44:09 - 44:15
    my life miserable,
    because it's telling me,
  • 44:15 - 44:17
    you don't have
    speed 1, Magdalena.
  • 44:17 - 44:19
    Drive to Amarillo
    and back, you're
  • 44:19 - 44:22
    not going to get speed 1.
  • 44:22 - 44:23
    Why don't I have speed 1?
  • 44:23 - 44:24
    Think about it.
  • 44:24 - 44:25
    Bear with me.
  • 44:25 - 44:29
    Minus a sine t equals sine t, 0.
  • 44:29 - 44:29
    Bad.
  • 44:29 - 44:31
    What is the speed?
  • 44:31 - 44:33
    a.
  • 44:33 - 44:36
    If you do the math,
    the speed will be a.
  • 44:36 - 44:40
    So length of our
    prime of t will be a.
  • 44:40 - 44:41
    Somebody help me.
  • 44:41 - 44:42
    Get me out of trouble.
  • 44:42 - 44:43
    Who is this?
  • 44:43 - 44:45
    I want to do it in arc length.
  • 44:45 - 44:48
    Otherwise, how can
    I do the curvature?
  • 44:48 - 44:51
    So somebody tell
    me how to get to s.
  • 44:51 - 44:52
    What the heck is that?
  • 44:52 - 44:59
    s of t is integral from
    0 to t of-- who tells me?
  • 44:59 - 45:00
    The speed, right?
  • 45:00 - 45:04
    Was it not the displacement,
    the arc length traveled along,
  • 45:04 - 45:08
    and the curve is integral
    in time of the speed.
  • 45:08 - 45:12
  • 45:12 - 45:13
    OK?
  • 45:13 - 45:16
    So I have-- what is that?
  • 45:16 - 45:18
    Speed is?
  • 45:18 - 45:18
    STUDENT: Um--
  • 45:18 - 45:19
    PROFESSOR: a.
  • 45:19 - 45:23
    So a time t, am I right,
    guys? s is a times t.
  • 45:23 - 45:25
    So what do I have to do?
  • 45:25 - 45:31
    Take Mr. t, shake his hand,
    and replace him with s over a.
  • 45:31 - 45:32
    OK.
  • 45:32 - 45:40
    So instead of r of t, I'll say--
    what other letters do I have?
  • 45:40 - 45:40
    Not r.
  • 45:40 - 45:41
    Rho of s.
  • 45:41 - 45:42
    I love rho.
  • 45:42 - 45:44
    Rho is the Greek [INAUDIBLE].
  • 45:44 - 45:46
    Is this finally an arc length?
  • 45:46 - 45:51
    Cosine of-- what
    is t, guys, again?
  • 45:51 - 45:53
    s over a.
  • 45:53 - 45:58
    s over a, a sine
    s over a, and 0.
  • 45:58 - 46:02
    This is the parameterization
    in arc length.
  • 46:02 - 46:08
    This is an arc length
    parameterization of the circle.
  • 46:08 - 46:11
    And then what is this
    definition of curvature?
  • 46:11 - 46:14
    It's here.
  • 46:14 - 46:17
    Do that rho once, twice.
  • 46:17 - 46:20
    Prime it twice,
    and do the length.
  • 46:20 - 46:21
    So rho prime.
  • 46:21 - 46:25
    Oh my God is it hard.
  • 46:25 - 46:29
    a times minus sine of s over a.
  • 46:29 - 46:30
    Am I done, though?
  • 46:30 - 46:31
    Chain rule.
  • 46:31 - 46:32
    Pay attention, Magdalena.
  • 46:32 - 46:34
    Don't screwed up with this one.
  • 46:34 - 46:36
    1 over a.
  • 46:36 - 46:38
    Good.
  • 46:38 - 46:39
    Next.
  • 46:39 - 46:42
    a cosine of s over a.
  • 46:42 - 46:43
    Chain rule.
  • 46:43 - 46:44
    Don't forget,
    multiply by 1 over a.
  • 46:44 - 46:47
    OK, that makes my life easier.
  • 46:47 - 46:48
    We simplify.
  • 46:48 - 46:52
    Thank God a simplifies
    here, a simplifies there,
  • 46:52 - 46:54
    so that is that derivative.
  • 46:54 - 46:56
    What's the second derivative?
  • 46:56 - 47:01
    Rho double prime of s will
    be-- somebody help me, OK?
  • 47:01 - 47:03
    Because this is a
    lot of derivation.
  • 47:03 - 47:03
    STUDENT: --cosine--
  • 47:03 - 47:05
    PROFESSOR: Thank you, sir.
  • 47:05 - 47:07
    Minus cosine of s over a.
  • 47:07 - 47:08
    STUDENT: Times 1 over a.
  • 47:08 - 47:13
    PROFESSOR: Times 1 over a,
    comma, minus sine of s over a.
  • 47:13 - 47:16
    That's all I have left
    in my life, right?
  • 47:16 - 47:20
    Minus sine of s over a times
    1 over a from the chain rule.
  • 47:20 - 47:23
    I have to pay attention and see.
  • 47:23 - 47:24
    What's the magnitude of this?
  • 47:24 - 47:29
    The magnitude of this of this
    animal will be the curvature.
  • 47:29 - 47:30
    Oh, my God.
  • 47:30 - 47:32
    So what is k?
  • 47:32 - 47:35
    k of s will be--
    could somebody tell me
  • 47:35 - 47:40
    what magnitude I get after I
    square all these individuals,
  • 47:40 - 47:43
    sum them up, and take
    the square root of them?
  • 47:43 - 47:44
    STUDENT: [INAUDIBLE]
  • 47:44 - 47:50
    PROFESSOR: Square root
    of 1 over 1 squared.
  • 47:50 - 47:51
    And I get 1 over a.
  • 47:51 - 47:53
    You are too fast for
    me, you teach me that.
  • 47:53 - 47:54
    No, I'm just kidding.
  • 47:54 - 47:56
    I knew it was 1 over a.
  • 47:56 - 47:59
    Now, how did
    engineers know that?
  • 47:59 - 48:02
    Actually, for hundreds of years,
    mathematicians, engineers,
  • 48:02 - 48:04
    and physicists knew that.
  • 48:04 - 48:07
    And that's the last thing
    I want to teach you today.
  • 48:07 - 48:10
    We have two circles.
  • 48:10 - 48:17
    This is of, let's say, radius
    1/2, and this is radius 2.
  • 48:17 - 48:21
    The engineer, mathematician,
    physicist, whoever they are,
  • 48:21 - 48:26
    they knew that the curvature
    is inverse proportional
  • 48:26 - 48:28
    to the radius.
  • 48:28 - 48:30
    That radius is 1/2.
  • 48:30 - 48:34
    The curvature will
    be 2 in this case.
  • 48:34 - 48:38
    The radius is 2, the
    curvature will be 1/2.
  • 48:38 - 48:42
    Does that make sense, this
    inverse proportionality?
  • 48:42 - 48:46
    The bigger the radius,
    the lesser the curvature,
  • 48:46 - 48:48
    that less bent you are.
  • 48:48 - 48:50
    The more fat-- well, OK.
  • 48:50 - 48:53
    I'm not going to say anything
    politically incorrect.
  • 48:53 - 48:59
    So this is really curved because
    the radius is really small.
  • 48:59 - 49:03
    This less curved,
    almost-- at infinity,
  • 49:03 - 49:06
    this curvature
    becomes 0, because
  • 49:06 - 49:09
    at infinity, that radius
    explodes to plus infinity bag
  • 49:09 - 49:10
    theory.
  • 49:10 - 49:14
    Then you have 1 over
    infinity will be 0,
  • 49:14 - 49:19
    and that will be the curvature
    of a circle of infinite radius.
  • 49:19 - 49:20
    Right?
  • 49:20 - 49:23
    So we learned something today.
  • 49:23 - 49:25
    We learned about the
    curvature of a circle, which
  • 49:25 - 49:26
    is something.
  • 49:26 - 49:31
    But this is the same
    way for any curve.
  • 49:31 - 49:32
    You reparameterize.
  • 49:32 - 49:34
    Now you understand why you need
    to reparameterize in arc length
  • 49:34 - 49:36
    s.
  • 49:36 - 49:38
    You take the acceleration
    in arc length.
  • 49:38 - 49:39
    You get the magnitude.
  • 49:39 - 49:42
    That measures how
    bent the curve is.
  • 49:42 - 49:47
    Next time, you're going to
    do how bent the helix is.
  • 49:47 - 49:48
    OK?
  • 49:48 - 49:49
    At every point.
  • 49:49 - 49:51
    Enjoy your WeBWorK homework.
  • 49:51 - 49:55
    Ask me anytime, and
    ask me also Thursday.
  • 49:55 - 49:59
    Do not have a block about
    your homework questions.
  • 49:59 - 50:05
    You can ask me anytime
    by email, or in person.
  • 50:05 - 50:10
Title:
TTU Math2450 Calculus3 Sec 10.2 and 10.4 part 1
Description:

Derivatives of Vector Value Functions

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Video Language:
English
Duration:
50:11

English subtitles

Revisions