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TTU Math2450 Calculus3 Secs 12.7 - 12.8

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    PROFESSOR: I know you have
    encountered difficulties
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    on the last few problems,
    maybe four, maybe five, maybe
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    the last 10, I don't know.
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    But today, I want to--
    we have plenty of time.
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    We still have time
    for chapter 13,
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    and plenty of time
    for the final review.
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    I can afford to spend two or
    three hours just reviewing
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    chapter 12, if I wanted to.
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    All right, so I have this
    question from one of you saying
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    what part of the problem is
    that in terms of a two point
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    integral.
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    We have a solid
    bounded by z equals 3x,
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    and z equals x squared,
    and is a plane.
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    And can anybody tell
    me what this is?
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    Just out of curiosity,
    you don't have to know.
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    STUDENT: It's a parabola.
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    PROFESSOR: It would
    be a parabola,
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    if we were in
    [INTERPOSING VOICES]
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    if we were in 2D.
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    So the parabola is missing
    the y, and y could be anybody.
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    So it's a parabola
    that's shifted along y.
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    It's going to give you
    a cylindrical surface.
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    It's like something used
    for drainage, I don't know.
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    Water, like a valve.
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    So this is what it is,
    a cylindrical surface.
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    And you know that z must be
    between x squared and 3x.
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    How do you know which one is
    bigger, which one is smaller?
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    You should think about it.
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    When you draw, you
    draw like that.
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    Do these guys intersect?
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    We are in the xz plane.
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    Do these guys intersect?
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    x squared equals
    3x intersect where?
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    They intersect at 0, and at 3.
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    x1 is 0, and x2 is 3.
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    So when I want to draw this,
    I would say that indeed, it's
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    a bounded domain.
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    If it where unbounded, it
    wouldn't ask for the volume,
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    because the volume
    would be nothing.
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    So this thing must
    be a bounded domain.
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    x cannot go on, this
    is the infinite part.
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    So we are thinking of just this
    striped piece of a domain x
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    here, where this piece is
    between z equals x squared,
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    then z equals 3x.
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    This is 0 origin, and this is 3.
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    So at 3, they meet again.
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    Are you guys with me?
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    At 3 o'clock they meet again.
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    I'm just kidding, x
    doesn't have to be time.
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    It's a special coordinate.
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    And y is looking at you,
    and is going towards you.
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    Well, if it's toward like
    that, it's probably not
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    positively oriented.
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    So y should come from you,
    and go into the board,
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    and then keep going in that
    direction for the frame
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    to be positive oriented.
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    Positively oriented means x like
    that, y like this, z like that.
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    So k must be the
    crossproduct between i and j.
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    i cross j must be k.
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    If I use the right hand
    rule, and I go y like that,
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    that means I changed
    the orientation.
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    So the y, you have to imagine
    the y coming from you, going
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    perpendicular to
    the board, then keep
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    going inside the
    board infinitely much.
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    Now, if we were to
    play with Play-Doh,
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    and we were on the other side of
    that, like Alice in the mirror,
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    we would have the y in the
    mirror world, going between 0
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    and 2, inside the board.
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    If I were to draw
    this piece of cake,
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    I start dreaming
    again, I apologize.
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    But I'm dreaming of very
    nice bounded pieces of solids
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    that would be made of cheese.
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    This is a perfect example where
    you have something like curve
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    or linear shape, and you
    kind of slice the cheese,
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    and that's a piece
    of the Parmesan.
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    OK.
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    So the y here is
    going from 0 to 2.
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    It's sort of the altitude.
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    And this is the piece
    of cake that you
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    were looking-- or the cheese,
    or whatever you're looking at.
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    So what do you put here?
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    You put z between
    x squared and 3x.
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    You put y between--
    y is between 0 and 2.
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    And you Mr. x as the last
    of them, he can go from-- he
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    goes from 0 to 3.
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    So x has the freedom
    to go from 0 to 3.
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    y has the freedom to go
    from flat line to flat line,
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    from between to flat planes--
    from two horizontal planes.
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    But Mr. z is married to
    x, he cannot escape this
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    relationship.
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    So we can only take this z
    with respect between these two
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    values that depend on x.
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    That's all.
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    Now why would we have 1?
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    Because by definition,
    if you remember
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    the volume was the
    triple integral
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    of 1 dv over any
    solid value domain.
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    Right?
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    So whenever you see
    a problem like that,
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    you know how to start it.
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    One triple integrate,
    and that's going to work.
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    Something else that
    gave you a big headache
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    was the ice cream cone.
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    The ice cream cone problem
    gave a big headache
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    to most of my students
    over the past 14 years
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    that I've been teaching Cal 3.
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    It's a beautiful problem.
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    It's one of my
    favorites problems,
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    because it makes me
    think of food again.
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    And not just any food, but
    some nice ice cream cone
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    that's original ice cream, not
    the one you find in a box like
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    Blue Bell or Ben and Jerry's.
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    All right, so how is the
    ice cream cone problem
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    that-- he showed it to me, but
    I forgot the problem number.
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    It was--
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    STUDENT: It's number 20.
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    PROFESSOR: Number?
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    STUDENT: 20.
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    PROFESSOR: Number 20, thanks.
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    And I want the data [INAUDIBLE].
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    I want to test my memory,
    see how many neurons
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    died since last time.
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    Don't tell me.
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    So I think the sphere was
    a radius 2, and the cone
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    that we picked for you,
    we picked it on purpose.
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    So that the results that
    come up for the ice cream
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    cone boundaries will
    be nice and workable.
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    So we can propose some data
    where the ice cream cone will
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    give you really nasty radii.
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    Can I draw it?
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    Hopefully.
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    This ice cream cone is
    based off the waffle cone.
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    I don't like the waffle
    cone, because I'm dreaming.
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    But the problem is, the waffle
    cone is not a finite surface.
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    It's infinite,
    it's a double cone.
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    It's the dream of every binger.
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    So it goes to infinity,
    and to negative infinity,
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    and that's not my problem.
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    My problem is to intersect
    this cone with the sphere,
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    and make it finite.
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    So to make it the
    true waffle cone,
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    I would have to draw a
    sphere of what radius?
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    Root 2.
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    I'll try to draw a
    sphere of root 2,
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    but I cannot
    predict the results.
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    Now I'm going to only
    look at this v1 cone.
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    I don't know what the problem
    wanted, but I'm looking at,
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    do they say in what domain?
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    Above the plane?
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    STUDENT: It just says
    lies above the cone.
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    PROFESSOR: That
    lies above the cone.
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    But look, if I turn my head like
    this, depending on my reference
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    frame, I have
    cervical spondylosis,
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    this is also lying
    above the cone.
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    So the problem is
    a little bit silly,
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    that whoever wrote
    it should have
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    said the sphere lies above a
    cone, for z greater than 0.
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    In the basement,
    it can continue--
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    that's for z-- for z
    less than 0 can continue
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    upside down, and then between
    the sphere and the cone,
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    you'll have another ice
    cream cone outside that.
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    But practically what
    they mean is just do v1
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    and forget about this one.
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    It's not very nicely phrased.
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    Above, beyond.
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    Are we above Australia?
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    That's stupid, right?
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    Because they may say, oh no,
    depends on where you are.
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    We are above you guys.
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    You think you're better
    than us because you
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    are closer to the North Pole.
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    But who made that rule that
    t the North Pole is superior?
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    If you look at the universe,
    who is above, who is beyond?
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    There is no direction.
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    So they would be very offended.
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    I have a friend who
    works in Sydney.
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    She is a brilliant geometer.
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    And I bet if I asked
    her, she would say
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    who says you guys are above?
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    Because it depends on where your
    head is and how you look at it.
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    The planet is the
    same, so would you
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    say that the people
    who are walking closer
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    to the North Pole have
    their body upside down?
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    So it really matters how
    you look, what's above.
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    So assume that above means--
    the word above means positive.
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    And this is the ice cream cone.
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    Now how do I find out
    where to cut the waffle?
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    Because this is the question.
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    I need to know where the
    boundary of the waffle is.
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    I'm not allowed to eat
    anything above that.
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    So that's going
    to be the waffle.
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    And for that, any ideas-- how do
    I get to see what the circle--
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    where the circle will be?
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    STUDENT: Do they
    meet each other?
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    PROFESSOR: They intersect.
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    Excellent, Matthew.
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    Thank you.
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    So intersect the two surfaces
    by setting up a system to solve.
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    Solve the system.
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    And the intersection of the two
    is Mr. z, which is Mr. circle.
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    All right.
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    So what do I do?
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    I'm going to say I have to
    be smart about that one.
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    So if z squared from
    here plugging in,
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    substitute, is the same as
    x squared plus y squared.
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    So that means this is if
    and only if 2x squared
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    plus y squared.
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    2 times x squared
    plus y squared.
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    We have an x squared
    plus y squared,
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    and another x squared
    plus y squared equals 2.
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    You see how nicely the
    problem was picked?
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    It was picked it's going
    to give you some nice data.
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    z equals-- z
    squared equals that.
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    Keep going with if and only if.
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    If you're a math major,
    you will understand
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    why x squared plus
    y squared equals 1.
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    And z squared must be 1.
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    Well so, we really
    get two solutions,
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    the one close to the South
    Pole, and the one close
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    to the North Pole,
    because I'm going
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    to have z equals plus minus 1.
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    Where's the North Pole?
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    The North Pole would be
    0, 0, square root of 2.
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    The South Pole would be 0,
    0, minus square root of 2.
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    And my plain here is
    cut at which altitude?
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    z equals 1.
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    And I have another plane here,
    and an imaginary intersection
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    that I'm not going to talk
    about today. z equals minus y.
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    I don't care about the mirror
    image of the-- with respect
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    to the equator of the cone.
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    All right, good.
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    So we know who this
    guy is, we know
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    that he is-- I have a
    red marker, and a green,
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    and a blue.
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    I cannot live without colors.
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    Life is ugly enough.
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    Let's try to make it colorful.
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    x squared plus y
    squared, equals 1.
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    We are happy, because
    that's a nice, simple circle
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    of radius 1.
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    Now you have to think
    in which coordinate
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    you can write this problem.
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    And I'm going to
    beg of you to help
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    me review the material for
    the final and for the midterm.
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    Then again, on the midterm, I'm
    not going to put this problem.
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    So for the final, do
    expect something like that.
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    We may have, instead of
    the cone in the book,
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    you'll have a paraboloid
    and a sphere intersecting.
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    It's sort of the same thing, but
    instead of the ice cream cone,
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    you have the valley
    full of cream.
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    I cannot stop, right?
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    So if you do the volume
    like I told you before,
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    you simply have
    [INTERPOSING VOICES]
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    No, I'll do the volume first.
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    I know you have
    the surface there,
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    but what-- I'm doing the
    volume because I have plans,
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    and I didn't want
    to say what plans.
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    You forgot what I said, right?
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    So suppose somebody's
    asking you for the volume.
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    The volume-- how much
    ice cream you have inside
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    depends on that very much.
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    And I'd like you to
    remember that the v is
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    piratically against
    the ybc, right?
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    Right until the Cartesian
    coordinates would be a killer,
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    we try to write it
    in either cylindrical
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    or spherical to make
    our life easier.
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    If I want to make my life
    easier, first in cylindrical
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    coordinates, and then in
    spherical coordinates.
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    Could you help me
    find the limit points?
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    And then we'll do the surface.
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    Just remind me, OK?
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    [INTERPOSING VOICES]
    The volume of the-- OK.
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    The volume occupied
    by the ice cream.
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    The ice cream is between
    this plastic cap,
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    that is the sphere.
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    We cover it for
    hygiene purposes.
  • 17:05 - 17:11
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    So for cylindrical coordinates,
    rho and theta are really nice.
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    We don't worry about them yet.
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    But z should be between?
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    OK.
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    Really, 0?
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    So because it's
    between the ice cream
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    the cone-- do you
    think the waffle
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    cone-- what's the equation
    of the waffle cone?
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    And how do you get to the
    equation of the waffle cone?
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    The waffle cone meant--
    oh guys, help me.
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    z equals-- now you
    take the square root
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    of x squared plus y squared,
    because the other one would
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    be here.
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    The imaginary one, z equals
    minus the square root
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    of x squared plus y squared.
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    Forget about the
    world in the basement.
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    So you take z to
    the square root of,
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    with a plus, plus y squared.
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    In cylindrical coordinates,
    what does this mean?
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    In cylindrical coordinates?
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    STUDENT: It equals r.
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    PROFESSOR: This
    equals r, very good.
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    He's thinking faster.
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    Do you guys
    understand why he said
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    x squared plus y
    squared, if we work
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    with polar coordinates--
    which is cylindrical
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    coordinates it's the same
    thing-- polar coordinates
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    and cylindrical coordinates.
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    x squared plus y squared
    would be little r squared.
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    Under the square
    root would be r.
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    So you'll see, we're between r.
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    And now, another hard part.
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    What is the z equals plus square
    root of-- What was it, guys?
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    STUDENT: So are we taking
    the volume of all of the ice
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    cream inside the cone?
  • 18:58 - 19:03
    PROFESSOR: So between the
    cone, ice cream lies here.
  • 19:03 - 19:05
    Ice cream chips,
    chocolate chips,
  • 19:05 - 19:07
    between the cone and the sphere.
  • 19:07 - 19:09
  • 19:09 - 19:13
    The sphere is the bottom
    function, the lower function.
  • 19:13 - 19:14
    Is that good?
  • 19:14 - 19:16
    STUDENT: 2 minus r squared.
  • 19:16 - 19:21
    PROFESSOR: So I have the square
    root of 2 minus r squared.
  • 19:21 - 19:24
    I don't like the
    square root, I hate it.
  • 19:24 - 19:25
    Can I do it with it?
  • 19:25 - 19:27
    Yes, I can.
  • 19:27 - 19:29
    Maybe I can apply the
    use of solution later.
  • 19:29 - 19:31
    Don't worry about
    me, I'll make it.
  • 19:31 - 19:35
    I will live better if I didn't
    have any ugly things like that.
  • 19:35 - 19:36
    So let's see what we have.
  • 19:36 - 19:38
    Theta.
  • 19:38 - 19:41
    Your cone is not just sliced
    cone, it's all the cone.
  • 19:41 - 19:44
    So you have 0 to 2 pi.
  • 19:44 - 19:46
    One revolution,
    complete revolution.
  • 19:46 - 19:50
    How about rho?
  • 19:50 - 19:51
    Rho is limited.
  • 19:51 - 19:53
    Rho is what lies in the
    plane in terms of radius.
  • 19:53 - 19:57
  • 19:57 - 19:58
    0, 2?
  • 19:58 - 20:01
    How much is from here to here?
  • 20:01 - 20:05
    How much is from here to here?
  • 20:05 - 20:08
    Didn't we do it x squared
    plus y squared equals 1?
  • 20:08 - 20:10
    So what is this radius
    from here to here?
  • 20:10 - 20:11
    1.
  • 20:11 - 20:13
    And what is this radius
    from here to here?
  • 20:13 - 20:13
    1.
  • 20:13 - 20:15
    So the projection
    of this ice cream
  • 20:15 - 20:19
    cone-- if you had the
    eye of god is here,
  • 20:19 - 20:22
    sun, you have a
    shadow on the ground,
  • 20:22 - 20:26
    coming from your ice cream
    cone, and this is the shadow.
  • 20:26 - 20:29
    Your shadow is simply
    a disk of radius 1.
  • 20:29 - 20:31
    Good, that's the
    projection you have.
  • 20:31 - 20:34
    So Mr. rho is between 0 and 1.
  • 20:34 - 20:39
    For polar coordinates,
    it's not so ugly actually.
  • 20:39 - 20:40
    0 to 2 pi.
  • 20:40 - 20:43
    0 to 1.
  • 20:43 - 20:47
    r to square root of
    2 minus r squared.
  • 20:47 - 20:53
    Instead of r, it's
    OK to react with rho.
  • 20:53 - 20:55
    And here's the
    big j coordinates.
  • 20:55 - 20:58
    I'm going to erase
    j, don't write j.
  • 20:58 - 21:00
    Jacobian in general is Jacobian.
  • 21:00 - 21:03
    The one that does the
    transformation between
  • 21:03 - 21:04
    coordinates to
    other coordinates.
  • 21:04 - 21:06
    Let me finish on that.
  • 21:06 - 21:09
    How about this one?
  • 21:09 - 21:12
    This is simply r, very good.
  • 21:12 - 21:13
    Your old friend.
  • 21:13 - 21:17
    So you [INAUDIBLE]
    the dz d, theta,
  • 21:17 - 21:25
    dr, d is your [INAUDIBLE]
    It's not easy there.
  • 21:25 - 21:28
    If I were to continue--
    maybe on the final-- OK
  • 21:28 - 21:30
    I'm talking too much, as usual.
  • 21:30 - 21:34
    Maybe on whatever test
    you're going to have,
  • 21:34 - 21:40
    this kind of stuff, with
    a formulation saying you
  • 21:40 - 21:43
    do not have to compute it.
  • 21:43 - 21:46
    But if you wanted to compute it,
    would it be hard from 0 to 1,
  • 21:46 - 21:52
    from 0 to 2 pi, and say
    forgot the stinky pi?
  • 21:52 - 21:56
    Take the 2 pi out to
    make your life easier.
  • 21:56 - 21:59
    Because the theta isn't
    depending from-- there
  • 21:59 - 22:01
    is no theta inside.
  • 22:01 - 22:04
    So take the 2 pi
    out, and then you
  • 22:04 - 22:10
    have an integral from 0 to
    1, and integral from-- now.
  • 22:10 - 22:11
    R got out for a walk.
  • 22:11 - 22:14
    This is r going out for a walk.
  • 22:14 - 22:17
    Integral of 1 with
    respect to dz.
  • 22:17 - 22:22
    So z is taken between r and
    root of 2 minus r squared.
  • 22:22 - 22:23
    Right?
  • 22:23 - 22:27
    So I would have to write
    here the 1 on top minus the 1
  • 22:27 - 22:30
    on the bottom, which is a
    little bit of a headache for me.
  • 22:30 - 22:35
    I'm looking at it,
    I'm getting angry.
  • 22:35 - 22:39
    Now, times the r that
    went out for a walk.
  • 22:39 - 22:42
  • 22:42 - 22:45
    So practically, the
    0 is solved, and I
  • 22:45 - 22:50
    have the dr. And from 0 to 1.
  • 22:50 - 22:53
  • 22:53 - 22:55
    So I took care or who?
  • 22:55 - 22:58
    I took care of the
    integral with respect to z.
  • 22:58 - 23:00
    This is r here.
  • 23:00 - 23:03
    This was done first.
  • 23:03 - 23:06
    And you gave me that
    between those two.
  • 23:06 - 23:07
    So I got that.
  • 23:07 - 23:12
    Times the r, between 0 and 1,
    with respect to r, and then
  • 23:12 - 23:14
    the 2 pi gets outside.
  • 23:14 - 23:17
    Now, if I split this
    into two integrals,
  • 23:17 - 23:18
    it's going to be easy, right?
  • 23:18 - 23:21
    Because I go--
    the first integral
  • 23:21 - 23:24
    will be r times square
    root of 2 minus r squared.
  • 23:24 - 23:26
    How can you do such an integral?
  • 23:26 - 23:27
    We do substitution.
  • 23:27 - 23:33
    For example, your u would
    b 2 minus r squared.
  • 23:33 - 23:34
    Can you keep going?
  • 23:34 - 23:37
    The second integral
    is a piece of cake.
  • 23:37 - 23:39
    A piece of ice cream.
  • 23:39 - 23:41
    The integral of r squared.
  • 23:41 - 23:44
    r cubed over 3,
    between 0 and 1, 1/3.
  • 23:44 - 23:50
    So we can still solve the ice
    cream cone volume like that.
  • 23:50 - 23:51
    Do I like it?
  • 23:51 - 23:51
    No.
  • 23:51 - 23:56
    Can you suspect why
    I don't like it?
  • 23:56 - 23:57
    Oh, by the way.
  • 23:57 - 24:00
    Suppose you got to
    this on the final,
  • 24:00 - 24:05
    how much do you get
    for-- you mess up
  • 24:05 - 24:08
    the algebra, how
    much do you get?
  • 24:08 - 24:18
  • 24:18 - 24:21
    You say, I can do
    that in my sleep,
  • 24:21 - 24:28
    u equals 2 minus r squared, u
    equals minus 2r, I can go on.
  • 24:28 - 24:32
    Even if you mess up the
    algebra, you get most of it.
  • 24:32 - 24:34
    Why don't I like it?
  • 24:34 - 24:36
    Because it involves
    work, and I'm lazy.
  • 24:36 - 24:43
    So can I find a
    better way to do it?
  • 24:43 - 24:46
    Can I get use
    spherical coordinates?
  • 24:46 - 24:48
    And how do I use
    spherical coordinates?
  • 24:48 - 24:51
    So let me see how I do that.
  • 24:51 - 24:54
    In spherical coordinates,
    it should be easier.
  • 24:54 - 25:00
  • 25:00 - 25:04
    Remember that for
    mathematicians, they
  • 25:04 - 25:07
    include this course Cal
    3 multivariable calculus.
  • 25:07 - 25:10
    We are not studying geography.
  • 25:10 - 25:15
    So for us, a lot can happen
    between minus 90 and plus 90
  • 25:15 - 25:20
    degrees, but it measures
    from the North Pole,
  • 25:20 - 25:22
    because we believe
    in Santa Clause.
  • 25:22 - 25:24
    Always remember that.
  • 25:24 - 25:29
    So we go all the way from
    0 degrees to 180 degrees.
  • 25:29 - 25:34
    So your-- in principle--
    your latitude
  • 25:34 - 25:40
    will go from 0 to
    all the way to pi.
  • 25:40 - 25:43
    But it doesn't, because
    it gets stuck here.
  • 25:43 - 25:46
    What is the latitude
    of the ice cream cone?
  • 25:46 - 25:51
    So what is the pi angle
    for this ice cream cone?
  • 25:51 - 25:54
  • 25:54 - 25:56
    It's a 45 degree angle.
  • 25:56 - 25:59
    That is true.
  • 25:59 - 26:05
    For anything like that-- I'm
    looking again at this cone.
  • 26:05 - 26:07
    z squared equals x
    squared plus y squared.
  • 26:07 - 26:11
  • 26:11 - 26:14
    I just want to talk a
    little bit about that.
  • 26:14 - 26:23
    So if you have x and
    y, this is the x.
  • 26:23 - 26:26
    This is x, you have to use
    your imagination on me.
  • 26:26 - 26:33
    And the hypotenuse would be
    x squared plus y squared.
  • 26:33 - 26:36
    And this is the z.
  • 26:36 - 26:45
    And then, I draw
    what is in between.
  • 26:45 - 26:48
    This has to be 45 degrees.
  • 26:48 - 26:50
    Can you see what's going on?
  • 26:50 - 26:58
    So theta has to be
    between 0 and what?
  • 26:58 - 27:00
    STUDENT: 2 pi.
  • 27:00 - 27:01
    PROFESSOR: Yes, you
    are smarter than me.
  • 27:01 - 27:03
    That was the longitude.
  • 27:03 - 27:03
    Thank you.
  • 27:03 - 27:06
    I'm sorry, I meant to
    write the latitude.
  • 27:06 - 27:11
    Phi is between 0 and pi/4.
  • 27:11 - 27:14
    How about the radius?
  • 27:14 - 27:17
    Are you afraid of the radius?
  • 27:17 - 27:18
    No.
  • 27:18 - 27:19
    Why?
  • 27:19 - 27:21
    The radius is your friend.
  • 27:21 - 27:24
    It was not your friend before.
  • 27:24 - 27:25
    Look how wobbly it is.
  • 27:25 - 27:30
    But in this case, the radius
    goes all the way from 0
  • 27:30 - 27:34
    to a finite value,
    which is exactly
  • 27:34 - 27:38
    the radius of the sphere.
  • 27:38 - 27:43
    Because you have rays of light
    coming from the source origin,
  • 27:43 - 27:49
    and they bounce
    against this profile,
  • 27:49 - 27:52
    which is the profile
    of the sphere, which
  • 27:52 - 27:54
    has radius square root of 2.
  • 27:54 - 27:58
    So life is good for
    you in this case.
  • 27:58 - 28:01
    Are you guys with me?
  • 28:01 - 28:02
    Should it be easy?
  • 28:02 - 28:06
    Yes, it should be easy to
    write that in the integral,
  • 28:06 - 28:08
    if you know how to write it.
  • 28:08 - 28:09
    So you have.
  • 28:09 - 28:10
    OK.
  • 28:10 - 28:11
    What do you want to do first?
  • 28:11 - 28:14
    It doesn't matter that you
    apply Fubini's theorem.
  • 28:14 - 28:19
    You have fixed limits.
  • 28:19 - 28:28
    You have 0 to 2 pi, 0 to
    pi/4, 0 to square root 2.
  • 28:28 - 28:32
    Inside, there must be a
    Jacobian that you know by heart,
  • 28:32 - 28:36
    and I'm asking you to learn
    it by heart before the final,
  • 28:36 - 28:38
    if not for now, but
    maybe before the final.
  • 28:38 - 28:43
    But by now, you should
    know it by heart.
  • 28:43 - 28:44
    Thank you so much, Matthew.
  • 28:44 - 28:45
    Yes.
  • 28:45 - 28:49
    You don't have much to memorize,
    but this is one of the things
  • 28:49 - 28:52
    that I told you I did not
    memorize it, I was a freshman,
  • 28:52 - 28:55
    I was stubborn and silly.
  • 28:55 - 28:58
    So I have to compute what?
  • 28:58 - 29:00
    I have to compute the Jacobian.
  • 29:00 - 29:05
    Imagine what work you have
    when you're limited in time.
  • 29:05 - 29:09
    dx, dr. dx, d theta.
  • 29:09 - 29:11
    dx, d phi.
  • 29:11 - 29:13
    I thought I was
    about to kill myself.
  • 29:13 - 29:23
    dy, dr. dy, d theta. dy, d
    phi, and finally, dz, dr. dz,
  • 29:23 - 29:25
    d theta.
  • 29:25 - 29:27
    dz d phi.
  • 29:27 - 29:29
    And I did this.
  • 29:29 - 29:32
    And I thought I was about to
    just collapse and not finish
  • 29:32 - 29:33
    my exam.
  • 29:33 - 29:37
    I finished my exam, but since
    then, I didn't remember that.
  • 29:37 - 29:39
    I had to compute it.
  • 29:39 - 29:42
    It took me 10 minutes
    to compute the Jacobian.
  • 29:42 - 29:46
    So this is r squared, psi, phi.
  • 29:46 - 29:50
    If you have nothing better
    to do, you can do that.
  • 29:50 - 29:52
  • 29:52 - 29:57
    Do you remember what the
    spherical coordinates were, out
  • 29:57 - 29:58
    of curiosity?
  • 29:58 - 30:00
    Who remembers that?
  • 30:00 - 30:03
    There are some
    pre-med majors here,
  • 30:03 - 30:05
    who probably remember that.
  • 30:05 - 30:10
    So when you have a phi here,
    you have r-- sine or cosine?
  • 30:10 - 30:11
    Cosine.
  • 30:11 - 30:13
    r cosine phi.
  • 30:13 - 30:18
    And then r sine phi
    for both times what?
  • 30:18 - 30:21
    The first one comes
    from theta, like that.
  • 30:21 - 30:24
    It's going to be cosine
    theta, and sine theta.
  • 30:24 - 30:30
    Well imagine me taking these
    functions and differentiating,
  • 30:30 - 30:31
    partial derivatives.
  • 30:31 - 30:38
    And after I differentiated down,
    compute the 3 by 3 determining.
  • 30:38 - 30:42
    It's an error, no matter how
    good you are at computing.
  • 30:42 - 30:46
    So don't do that,
    just memorize it.
  • 30:46 - 30:48
    Don't do like I did.
  • 30:48 - 30:50
    And then you have d what?
  • 30:50 - 30:54
    dr, d phi, d theta.
  • 30:54 - 30:57
  • 30:57 - 31:03
    Now what is the volume
    of the ice cream cone?
  • 31:03 - 31:06
    Let me erase.
  • 31:06 - 31:07
    This shouldn't be hard.
  • 31:07 - 31:10
    This is the type
    of problem where
  • 31:10 - 31:15
    you have a product of
    functions of several variables.
  • 31:15 - 31:22
    You can separate as a product
    of three independent integrals
  • 31:22 - 31:25
    as a consequence of
    Fubini's theorem.
  • 31:25 - 31:29
    So you have integral from,
    integral from, integral from.
  • 31:29 - 31:30
    Who's your friend?
  • 31:30 - 31:31
    Who do you like the most?
  • 31:31 - 31:31
    STUDENT: Theta.
  • 31:31 - 31:34
    PROFESSOR: You like
    theta the most?
  • 31:34 - 31:37
    Because it comes
    from Santa Clause?
  • 31:37 - 31:38
    No, the theta doesn't.
  • 31:38 - 31:43
    This is the easiest step.
  • 31:43 - 31:45
    So that's why you
    like it, because it's
  • 31:45 - 31:46
    the easiest to deal with.
  • 31:46 - 31:48
    How about phi?
  • 31:48 - 31:51
    Sine phi, d phi.
  • 31:51 - 31:56
    I agree with you,
    it's not so easy,
  • 31:56 - 31:58
    but it's going to be a
    piece of cake anyway.
  • 31:58 - 32:04
    How about this one, 0
    to root 2 r squared dr.
  • 32:04 - 32:07
    Is this guy hard to do?
  • 32:07 - 32:14
    r cubed over 3 will give
    me root 2 cubed over 3.
  • 32:14 - 32:16
    How much is that, by the way?
  • 32:16 - 32:19
    2 root 2 over 3.
  • 32:19 - 32:22
    Oh bless your heart,
    that's not so hard.
  • 32:22 - 32:24
    This is not a problem.
  • 32:24 - 32:26
    How about that?
  • 32:26 - 32:29
  • 32:29 - 32:29
    What do you have?
  • 32:29 - 32:33
    What is the integral of sine?
  • 32:33 - 32:34
    Negative cosine.
  • 32:34 - 32:42
    So you have minus cosine phi
    between pi/4 up and 0 down.
  • 32:42 - 32:44
    Good luck to you.
  • 32:44 - 32:48
    Well, the first guy.
  • 32:48 - 32:50
    Good, minus root 2 over 2.
  • 32:50 - 32:53
    Minus, second guy?
  • 32:53 - 32:56
    Minus, minus 1.
  • 32:56 - 32:57
    Don't fall into the trap.
  • 32:57 - 32:59
    Pay attention to the signs.
  • 32:59 - 33:01
    Don't mess up,
    because that's where
  • 33:01 - 33:07
    you can hurt your grade by
    messing up with minus signs.
  • 33:07 - 33:16
    So this is 1 plus 1,
    1 minus root 2 over 2.
  • 33:16 - 33:23
  • 33:23 - 33:26
    And finally, let's see what
    that is, the whole thing being.
  • 33:26 - 33:29
  • 33:29 - 33:31
    Can we write it nicely?
  • 33:31 - 33:34
    What's 2 times-- 4.
  • 33:34 - 33:41
    4, root 2 over 3 pi.
  • 33:41 - 33:42
    The first and the last.
  • 33:42 - 33:47
    4 times 2, pi/3 times this
    nasty guy 1 minus root 2.
  • 33:47 - 33:52
    I don't like it, let's
    make it look better.
  • 33:52 - 33:53
    Well OK, you can
    give me this answer,
  • 33:53 - 33:56
    of course you'll get 100%.
  • 33:56 - 33:58
    But am I happy with it?
  • 33:58 - 34:00
    If you were to publish
    this in a journal,
  • 34:00 - 34:02
    how would you simplify?
  • 34:02 - 34:04
    This is dry.
  • 34:04 - 34:08
    OK so what do you have?
  • 34:08 - 34:11
    1 is 2/2.
  • 34:11 - 34:22
    2 minus root 2 pi,
    4 and 2 simplify.
  • 34:22 - 34:23
    Are you guys with me?
  • 34:23 - 34:27
    There is a 2 down, and a 4
    up, so I'm going to have a 2
  • 34:27 - 34:30
    and another 2, all over 3.
  • 34:30 - 34:33
  • 34:33 - 34:36
    So I have 2 and 2 pi,
    times 2 minus root 2.
  • 34:36 - 34:38
    Do you like it like that?
  • 34:38 - 34:38
    I don't.
  • 34:38 - 34:39
    So what do you do next?
  • 34:39 - 34:44
  • 34:44 - 34:46
    I can even pull
    the root 2 inside.
  • 34:46 - 34:52
    So I go 4 root 2, minus what?
  • 34:52 - 34:57
    Minus 4, because this is
    2 times 3 is 4, pi over--
  • 34:57 - 34:58
    Do you like it?
  • 34:58 - 35:02
    Still I don't,
    because I'm stubborn.
  • 35:02 - 35:07
    4 root 2 minus 1 over 3 is
    the most beautiful form.
  • 35:07 - 35:10
    So I'll try to brush
    it up, and put it
  • 35:10 - 35:13
    in the most elegant form.
  • 35:13 - 35:16
  • 35:16 - 35:18
    It doesn't matter.
  • 35:18 - 35:22
    If you want to give
    me a correct answer,
  • 35:22 - 35:23
    any form it would be OK.
  • 35:23 - 35:24
    Yes?
  • 35:24 - 35:25
    STUDENT: If it was
    slightly different,
  • 35:25 - 35:31
    how would we find phi for the
    limits in the second part?
  • 35:31 - 35:32
    PROFESSOR: If you have a what?
  • 35:32 - 35:36
    STUDENT: How would we find
    phi if it wasn't obvious,
  • 35:36 - 35:38
    if it wasn't x
    squared, or c squared?
  • 35:38 - 35:41
    PROFESSOR: If it wasn't
    a 45 degree angle?
  • 35:41 - 35:41
    [INAUDIBLE]
  • 35:41 - 35:45
  • 35:45 - 35:48
    It's not so bad, you
    need a calculator.
  • 35:48 - 35:56
    Assume that I would have given
    you the sphere of radius 7,
  • 35:56 - 36:00
    or square root of 7,
    intersecting with this cone.
  • 36:00 - 36:03
    Then to compute
    that phi, you would
  • 36:03 - 36:06
    have needed to intersect
    the two surfaces
  • 36:06 - 36:10
    and then compute it, maybe
    look at tangent inverse.
  • 36:10 - 36:14
    Compute phi with
    tangent inverse.
  • 36:14 - 36:15
    And you will have tangent
    inverse of a number.
  • 36:15 - 36:19
    Well, you cannot put tangent
    inverse of a number everywhere,
  • 36:19 - 36:21
    it's not nice.
  • 36:21 - 36:24
    So what you would
    do is in the end,
  • 36:24 - 36:26
    you would do it with
    a calculator, come up
  • 36:26 - 36:30
    with a nice truncated
    result with 5 decimals,
  • 36:30 - 36:34
    or 10 decimals, whatever the
    calculator will give you.
  • 36:34 - 36:35
    OK?
  • 36:35 - 36:38
  • 36:38 - 36:39
    Or, you can do it with MathLab.
  • 36:39 - 36:42
  • 36:42 - 36:47
    You can do it with scientific
    software, for sure.
  • 36:47 - 36:52
    Let's do what I-- Ryan
    you said this was a what?
  • 36:52 - 36:54
    STUDENT: Number 20
    is for surface area.
  • 36:54 - 36:55
    PROFESSOR: OK.
  • 36:55 - 36:58
    So, it's-- read it to me again.
  • 36:58 - 37:02
    What does it say?
  • 37:02 - 37:03
    I'm coming to you.
  • 37:03 - 37:06
  • 37:06 - 37:10
    It says, find the surface area
    of the part of the sphere that
  • 37:10 - 37:14
    lies where you have 64.
  • 37:14 - 37:19
    This is all because
    of [INAUDIBLE]
  • 37:19 - 37:21
    But yours is not
    very even, right?
  • 37:21 - 37:27
  • 37:27 - 37:29
    You shouldn't have bad results.
  • 37:29 - 37:30
    And guess what?
  • 37:30 - 37:34
    If you do, you use
    your calculator
  • 37:34 - 37:38
    to find out the upper limit
    of the angle for the volume.
  • 37:38 - 37:40
    OK.
  • 37:40 - 37:47
    So now, you say oh
    my god, this is ugly.
  • 37:47 - 37:49
    I agree with you, it's not nice.
  • 37:49 - 37:56
  • 37:56 - 38:03
    You have square root of 2 minus
    x squared minus y squared.
  • 38:03 - 38:10
    And when you compute the
    surface area of the cap-- cup,
  • 38:10 - 38:13
    cap means spherical cap.
  • 38:13 - 38:16
    A little hat that
    looks like this?
  • 38:16 - 38:18
    That's why it's called cap.
  • 38:18 - 38:21
    That will integrate
    over the disk d.
  • 38:21 - 38:35
  • 38:35 - 38:40
    Square root of 1
    plus f of x squared
  • 38:40 - 38:49
    plus f of y squared, dx da.
  • 38:49 - 38:52
    Is that the only
    way you can do this?
  • 38:52 - 38:53
    No.
  • 38:53 - 38:57
    You can actually do it with
    parametrization of a sphere,
  • 38:57 - 39:01
    and you have the
    element limit over here.
  • 39:01 - 39:05
    So that might be easier.
  • 39:05 - 39:08
  • 39:08 - 39:09
    Yeah.
  • 39:09 - 39:10
    You can also do it in homework.
  • 39:10 - 39:15
    But what if you went up there--
    let's see, how hard is life?
  • 39:15 - 39:18
    How hard would it be
    to do it like this?
  • 39:18 - 39:21
  • 39:21 - 39:23
    That's good.
  • 39:23 - 39:25
    First of all, let's
    think everything
  • 39:25 - 39:27
    that's under the square root.
  • 39:27 - 39:28
    And write it down.
  • 39:28 - 39:30
    1 plus.
  • 39:30 - 39:33
    Now, computing this problem
    with respect to x and you say,
  • 39:33 - 39:35
    oh my god, that's hard.
  • 39:35 - 39:36
    No, it's not.
  • 39:36 - 39:39
    If you want to do the
    hard one, and most of you
  • 39:39 - 39:41
    were, and you have
    that professors who
  • 39:41 - 39:45
    gave you enough practice,
    what did you have done?
  • 39:45 - 39:47
    Chain rule.
  • 39:47 - 39:52
    On the bottom, you have
    this nasty guy twice.
  • 39:52 - 39:56
    But on the top, your minus 2x.
  • 39:56 - 40:00
    So when you simplify
    your life becomes easier.
  • 40:00 - 40:03
  • 40:03 - 40:06
    And you will square it.
  • 40:06 - 40:10
    Are you guys with me,
    have I lost you yet?
  • 40:10 - 40:13
    And then the same thing in y.
  • 40:13 - 40:19
    Minus 2y, over 2 square root 2
    minus x square minus y squared,
  • 40:19 - 40:20
    square it.
  • 40:20 - 40:25
  • 40:25 - 40:28
    Some things cancel out.
  • 40:28 - 40:31
    So let's be patient
    and see what we have.
  • 40:31 - 40:34
  • 40:34 - 40:38
    First of all, 1 is not going to
    give you trouble, because let
  • 40:38 - 40:42
    write 1 as this over itself.
  • 40:42 - 40:46
    Plus, minus squared
    is plus, thank god.
  • 40:46 - 40:51
    x squared over 2 minus x squared
    minus y squared plus y squared
  • 40:51 - 40:58
    over 2 minus x squared
    minus y squared.
  • 40:58 - 41:01
    And these guys go for a walk.
  • 41:01 - 41:09
    Minus x squared, minus y
    squared, plus y squared.
  • 41:09 - 41:12
  • 41:12 - 41:15
    They disappear
    together in the dark.
  • 41:15 - 41:20
    So you have 2 over 2 minus
    x squared minus y squared.
  • 41:20 - 41:29
  • 41:29 - 41:31
    OK let's try to do that.
  • 41:31 - 41:34
  • 41:34 - 41:36
    Guys, I have to erase.
  • 41:36 - 41:37
    I will erase.
  • 41:37 - 41:43
  • 41:43 - 41:47
    So what you see
    here, some people
  • 41:47 - 41:51
    call it ds, and use the
    element of area on the surface.
  • 41:51 - 41:58
  • 41:58 - 42:04
    It's like the area of
    a small surface patch.
  • 42:04 - 42:08
  • 42:08 - 42:09
    So the curve linear squared.
  • 42:09 - 42:14
  • 42:14 - 42:15
    Alright.
  • 42:15 - 42:22
    So area of the cup will be--
    now you say, well over the d,
  • 42:22 - 42:24
    let me think.
  • 42:24 - 42:28
    d represents those
    xy's with a property
  • 42:28 - 42:36
    that x squared plus y squared
    was between what and what?
  • 42:36 - 42:42
    0 and 1, because
    that was our, the
  • 42:42 - 42:47
    predicted domain on the
    shadow on the ground.
  • 42:47 - 42:48
    OK, that was this.
  • 42:48 - 42:52
  • 42:52 - 42:56
    And as you look at it, I have
    to put it on the square root.
  • 42:56 - 42:59
    Don't be afraid of
    it, because it's not
  • 42:59 - 43:03
    much up here than you thought.
  • 43:03 - 43:05
    And let's solve this together.
  • 43:05 - 43:11
    What is your luck that this is
    a symmetric polynomial index,
  • 43:11 - 43:15
    and why x squared plus y squared
    that you can rewrite as r
  • 43:15 - 43:17
    squared, polar coordinates?
  • 43:17 - 43:20
    And Ryan asked, can I
    do polar coordinates?
  • 43:20 - 43:22
    That's exactly what
    you're going to do.
  • 43:22 - 43:25
    You didn't know, unless
    your intuition is strong.
  • 43:25 - 43:27
    Yes?
  • 43:27 - 43:27
    Alex tell me.
  • 43:27 - 43:30
    STUDENT: I was going to ask,
    if you could have done that
  • 43:30 - 43:35
    by taking the r plane and
    multiplying that by 2 pi r?
  • 43:35 - 43:37
    PROFESSOR: Yeah,
    you can do that.
  • 43:37 - 43:39
  • 43:39 - 43:41
    Well, that is a way to do that.
  • 43:41 - 43:43
    So practically, he's
    asking-- I don't
  • 43:43 - 43:48
    know if you guys
    remember, in Cal 2,
  • 43:48 - 43:51
    you have the surface
    of revolution, right?
  • 43:51 - 43:54
    And if you knew the
    length of an arc,
  • 43:54 - 43:57
    you would be able
    to revolve that arc.
  • 43:57 - 43:58
    This is the cap.
  • 43:58 - 44:01
    And you take one of the
    meridians of the hat,
  • 44:01 - 44:04
    and revolve it, can
    redo with a form,
  • 44:04 - 44:09
    like you did the washer
    and dryer method.
  • 44:09 - 44:10
    It always amuses me.
  • 44:10 - 44:15
    Yes, you could have
    done that from Cal 2.
  • 44:15 - 44:17
    Computing the area of
    the cap as a surface
  • 44:17 - 44:23
    of revolution, chapter-- c'mon,
    I'm a co-author of this book.
  • 44:23 - 44:28
    Chapter 7?
  • 44:28 - 44:29
    What chapter?
  • 44:29 - 44:30
    Chapter 6?
  • 44:30 - 44:32
    No.
  • 44:32 - 44:34
    The washer and dryer?
  • 44:34 - 44:36
    Chapter 6, right?
  • 44:36 - 44:36
    OK.
  • 44:36 - 44:39
    But now we already
    have three, and we
  • 44:39 - 44:42
    don't want to remember Cal 2
    because it was a nightmare.
  • 44:42 - 44:44
    Several of you told
    me that this is
  • 44:44 - 44:48
    easier, these things are
    generally easier than Cal 2,
  • 44:48 - 44:51
    because Cal 2 was headache.
  • 44:51 - 44:56
    And what seemed to be giving
    you most of the headache
  • 44:56 - 44:59
    was a salad of
    different ingredients
  • 44:59 - 45:01
    that seemed to be unrelated.
  • 45:01 - 45:03
    Which I agree.
  • 45:03 - 45:12
    You have arcing, washer,
    slices, then Greek substitution,
  • 45:12 - 45:13
    the partial fractions.
  • 45:13 - 45:15
    All sorts of things and
    series and sequences.
  • 45:15 - 45:19
    And they are little
    things that don't quite
  • 45:19 - 45:22
    follow one from another.
  • 45:22 - 45:25
    They are a little bit unrelated.
  • 45:25 - 45:27
    OK, how do you do that?
  • 45:27 - 45:31
    You have to help me because
    that was the idea, that now you
  • 45:31 - 45:32
    can help me, right?
  • 45:32 - 45:34
    Square root of
  • 45:34 - 45:39
    STUDENT: 2 over 2 minus r
    squared, times r, dr d theta.
  • 45:39 - 45:44
  • 45:44 - 45:47
    PROFESSOR: And do we like it?
  • 45:47 - 45:51
    No, but we have to continue.
  • 45:51 - 45:55
    0 to 1, this is 0 to 2 pi.
  • 45:55 - 46:03
    I can get rid of the 2 pi,
    and put it here and say, OK.
  • 46:03 - 46:12
    I should be as good as taking
    out square root of 2 from here.
  • 46:12 - 46:15
  • 46:15 - 46:18
    He goes out for a walk.
  • 46:18 - 46:25
    And then I have integral 1 over
    this long line of fraction.
  • 46:25 - 46:31
  • 46:31 - 46:36
    STUDENT: And that would be 2r
    so that the r will cancel out.
  • 46:36 - 46:42
    PROFESSOR: So r dr, if
    u is 2 minus r squared,
  • 46:42 - 46:43
    the u is minus.
  • 46:43 - 46:48
    I have to pay attention, so
    I don't mess up the signs.
  • 46:48 - 46:51
    So rdr is a block.
  • 46:51 - 46:55
    And this block is
    simply minus du/2.
  • 46:55 - 47:03
    So I write it here,
    minus 1/2, du/2.
  • 47:03 - 47:08
  • 47:08 - 47:11
    Don't be nervous
    about this minus,
  • 47:11 - 47:13
    because it's not going to
    give me a minus result,
  • 47:13 - 47:15
    a negative result.
    If it did, that means
  • 47:15 - 47:18
    that I was drunk when I
    did it, because I will
  • 47:18 - 47:21
    get the area of the cap as
    a negative number, which
  • 47:21 - 47:23
    is impossible.
  • 47:23 - 47:26
    But it's going to happen
    when I change the limits.
  • 47:26 - 47:26
    Yes?
  • 47:26 - 47:28
    STUDENT: Where did that
    last one come from?
  • 47:28 - 47:30
    PROFESSOR: From this one.
  • 47:30 - 47:34
    [INTERPOSING VOICES]
    Oh, I put too many.
  • 47:34 - 47:38
    So this guy is
    this guy, which is
  • 47:38 - 47:40
    this guy minus the [INAUDIBLE].
  • 47:40 - 47:43
  • 47:43 - 47:49
    Now, do you want me to go
    ahead and cancel this out?
  • 47:49 - 47:50
    Right?
  • 47:50 - 47:51
    OK.
  • 47:51 - 47:55
    I have squared 2 pi.
  • 47:55 - 47:57
    I did not get the
    endpoints, you have
  • 47:57 - 47:58
    to help me put the endpoints.
  • 47:58 - 48:02
  • 48:02 - 48:05
    From 2 down.
  • 48:05 - 48:06
    To 1.
  • 48:06 - 48:07
    Which is crazy, right?
  • 48:07 - 48:09
    Because 2 is bigger than 1.
  • 48:09 - 48:13
    That's exactly where the next
    minus is going to come from.
  • 48:13 - 48:18
    So integral from 2 to 1 is
    minus integral from 1 to 2.
  • 48:18 - 48:20
    So I shouldn't be
    worried, because I already
  • 48:20 - 48:24
    have the minus out, with the
    minus that's going to come out,
  • 48:24 - 48:25
    I'm going to have a
    positive variable.
  • 48:25 - 48:28
  • 48:28 - 48:29
    Square root 2 pi.
  • 48:29 - 48:33
  • 48:33 - 48:37
    Somebody was smarter than
    me and said Magdalene,
  • 48:37 - 48:39
    I think Alex-- was it you?
  • 48:39 - 48:44
    You said, why don't you
    take advantage of the fact
  • 48:44 - 48:48
    that you already have 1 over
    2 square root u and integrate?
  • 48:48 - 48:51
    And that is going
    to be squared u.
  • 48:51 - 48:53
    Can you understand?
  • 48:53 - 48:54
    Who said that?
  • 48:54 - 48:57
    I heard a voice, it
    was not in my head.
  • 48:57 - 48:58
    I'm Innocent.
  • 48:58 - 49:02
    I heard a voice that told
    me, if you are smart,
  • 49:02 - 49:05
    you would understand
    to pull out the minus.
  • 49:05 - 49:10
    You would understand
    that this exactly
  • 49:10 - 49:13
    is the derivative
    of square root of u.
  • 49:13 - 49:16
    And I will be faster than
    you, because you have just
  • 49:16 - 49:21
    computed made between 1 and 2.
  • 49:21 - 49:22
    Some people aren't too smart.
  • 49:22 - 49:23
    I didn't think of that.
  • 49:23 - 49:27
    Now I've been thing about that.
  • 49:27 - 49:31
    Why cancel out the 2
    when you can [INAUDIBLE].
  • 49:31 - 49:35
    So you have a minus out.
  • 49:35 - 49:39
    STUDENT: There still needs to
    be a 2 on the outside, right?
  • 49:39 - 49:41
    PROFESSOR: Yes, I have
    to put 2 together.
  • 49:41 - 49:43
    Minus 2 and 2.
  • 49:43 - 49:46
    2 pi, that's a collective thing.
  • 49:46 - 49:50
    Squared and cubed
    between 1 and 2.
  • 49:50 - 49:51
    Do I like this?
  • 49:51 - 49:55
    No, but you tell me
    what is in the bracket.
  • 49:55 - 49:59
    How much u minus 12, 13.
  • 49:59 - 50:03
    1 minus square root of
    2 is a negative number.
  • 50:03 - 50:06
    But with the minus outside,
    I"m going to fix it.
  • 50:06 - 50:08
    And I'm going to get
    something really ugly.
  • 50:08 - 50:16
  • 50:16 - 50:18
    Yeah.
  • 50:18 - 50:21
    So when I'm multiplying sides,
    this by that, I get 4, right?
  • 50:21 - 50:23
    Guys?
  • 50:23 - 50:24
    I get a 4.
  • 50:24 - 50:29
    This guy and this guy, minus,
    minus, plus 2, 2 times 2 is 4.
  • 50:29 - 50:35
    And then minus, to make
    it look better, 2 root 2.
  • 50:35 - 50:38
    And multiply out.
  • 50:38 - 50:40
    Minus root 2 and the pi.
  • 50:40 - 50:44
    Now, I don't care
    where you stop.
  • 50:44 - 50:47
    I swear that if you stop
    here, you'll still get 100%.
  • 50:47 - 50:51
    Because what I care about is
    not to see a nice simplified
  • 50:51 - 50:52
    result, so much.
  • 50:52 - 50:54
    I won't go over your work.
  • 50:54 - 50:57
    But to see that
    you understood how
  • 50:57 - 51:00
    you solve this kind of problem.
  • 51:00 - 51:02
    It's not the sign
    of intelligence
  • 51:02 - 51:07
    being able to simplify
    answers very much.
  • 51:07 - 51:12
    But the method in itself, why
    and how, what the steps are,
  • 51:12 - 51:15
    that shows knowledge
    and intelligence.
  • 51:15 - 51:19
  • 51:19 - 51:20
    Have I mess up?
  • 51:20 - 51:21
    I don't think so.
  • 51:21 - 51:25
    STUDENT: Does the order matter,
    of the dr d theta, or dx/dy,
  • 51:25 - 51:29
    does that matter which
    order you put them in?
  • 51:29 - 51:30
    PROFESSOR: In this case, no.
  • 51:30 - 51:31
    STUDENT: Or over here?
  • 51:31 - 51:33
    PROFESSOR: In this
    case, no again.
  • 51:33 - 51:36
    But if you were
    to swap them, you
  • 51:36 - 51:40
    would have to swap
    the values as well.
  • 51:40 - 51:41
    Why is that?
  • 51:41 - 51:43
    That's a very good question.
  • 51:43 - 51:46
    He's right, but why is that?
  • 51:46 - 51:49
    It doesn't matter, why?
  • 51:49 - 51:50
    In general, it matters.
  • 51:50 - 51:54
  • 51:54 - 52:02
    They have to be from a given
    number to a given number.
  • 52:02 - 52:05
    It's not like reversing--
    when you reverse
  • 52:05 - 52:08
    the order of integrals,
    it's usually harder,
  • 52:08 - 52:11
    because you have to draw
    the vertical strips.
  • 52:11 - 52:13
    And you have it
    between two functions.
  • 52:13 - 52:16
    And then from vertical strips,
    you go to horizontal strips,
  • 52:16 - 52:18
    and you have other
    two functions.
  • 52:18 - 52:21
    So you always have to think
    how to change the function.
  • 52:21 - 52:24
    Here, you don't have
    to think at all.
  • 52:24 - 52:28
    You have a function
    that depends on r only.
  • 52:28 - 52:29
    There is no theta
    in the picture.
  • 52:29 - 52:32
    Plus these two
    are fixed numbers.
  • 52:32 - 52:35
    You can reverse the
    integration in your sleep.
  • 52:35 - 52:37
    OK, you get the same thing.
  • 52:37 - 52:40
    All you have to do is
    swap these two guys,
  • 52:40 - 52:42
    and swap-- the 0 is the same.
  • 52:42 - 52:45
    So I swap these two guys.
  • 52:45 - 52:49
    STUDENT: How did you
    take the 2 pi out?
  • 52:49 - 52:51
    PROFESSOR: What did I do?
  • 52:51 - 52:53
    How did I take this out?
  • 52:53 - 52:56
    STUDENT: No, the 2 pi.
  • 52:56 - 52:57
    PROFESSOR: Oh, the 2 pi?
  • 52:57 - 52:58
    OK.
  • 52:58 - 53:00
    Let me show you it better
    here, because we've
  • 53:00 - 53:03
    discussed about this before.
  • 53:03 - 53:07
    When you have
    integral from a to b,
  • 53:07 - 53:11
    or integral from c to
    d of a function or r
  • 53:11 - 53:19
    and a function of
    theta, what do you go?
  • 53:19 - 53:20
    There is a theorem
    that says that--
  • 53:20 - 53:22
    and thanks for this
    theorem and the fact
  • 53:22 - 53:23
    that they're separable.
  • 53:23 - 53:26
    The variables are
    separated in this product.
  • 53:26 - 53:31
    This is the product between
    integral from a to b,
  • 53:31 - 53:34
    here of theta to
    theta, and integral
  • 53:34 - 53:38
    from c to d, f of r/dr.
    They are nothing to one
  • 53:38 - 53:40
    another but a product.
  • 53:40 - 53:41
    So what do you do?
  • 53:41 - 53:47
    You say this is integral
    of 1, from 0 to pi d theta,
  • 53:47 - 53:49
    times the other guy.
  • 53:49 - 53:53
    So this is 2 pi.
  • 53:53 - 53:57
    When theta doesn't appear
    inside, it's a blessing.
  • 53:57 - 54:00
    But if and if there
    is, I have a question.
  • 54:00 - 54:01
    What if theta appeared inside?
  • 54:01 - 54:04
  • 54:04 - 54:06
    Theta doesn't appear
    inside by himself.
  • 54:06 - 54:09
    He appears inside
    of a trig function.
  • 54:09 - 54:14
    So assume you have cosine
    theta here times r.
  • 54:14 - 54:18
    You would have pulled
    cosine theta out,
  • 54:18 - 54:21
    and integrated cosine
    theta, that would be easy.
  • 54:21 - 54:26
    And if you have a problem like
    that, you would have gotten 0.
  • 54:26 - 54:29
    Because integral of
    course of cosine theta
  • 54:29 - 54:33
    would be sine of theta, and
    then theta between 0 and 2
  • 54:33 - 54:37
    pi is sine of theta between,
    which would give you 0.
  • 54:37 - 54:40
    It happened to me,
    many times in the exam.
  • 54:40 - 54:41
    It was a blessing.
  • 54:41 - 54:45
    I was 19, and I was so happy.
  • 54:45 - 54:48
    Professors wanted to
    see only the answer.
  • 54:48 - 54:52
    Because in Romania,
    it's different.
  • 54:52 - 54:55
    You come take a written
    exam, and the professor
  • 54:55 - 54:58
    has five hours to grade it.
  • 54:58 - 55:02
    The same day, two hours later,
    you have the oral examination.
  • 55:02 - 55:05
    You pick up a ticket,
    on the ticket,
  • 55:05 - 55:08
    you see three things to
    solve, four things to solve.
  • 55:08 - 55:09
    You go take a seat.
  • 55:09 - 55:13
    And while the professor and
    the assistant grade the exam,
  • 55:13 - 55:17
    you actually think
    of your oral exam.
  • 55:17 - 55:21
    When you come and present
    your results on the board,
  • 55:21 - 55:23
    they tell you,
    you messed up, you
  • 55:23 - 55:27
    got a 60% on this sticking exam.
  • 55:27 - 55:28
    This is how it goes.
  • 55:28 - 55:32
    Or, on the contrary, hey,
    listen, you got a 95%
  • 55:32 - 55:34
    on the written part, OK?
  • 55:34 - 55:37
    I don't want to see
    what you have there,
  • 55:37 - 55:38
    it really looks good.
  • 55:38 - 55:40
    I don't want to see
    it, it's clear to me
  • 55:40 - 55:41
    that you know what you're doing.
  • 55:41 - 55:45
    So it's a different
    kind of examination.
  • 55:45 - 55:48
    I hear that Princeton
    does that, I wonder
  • 55:48 - 55:49
    how are all the exams here.
  • 55:49 - 55:52
    I don't think people
    are ready for them yet.
  • 55:52 - 55:54
    But at Princeton they
    do a lot, all the same.
  • 55:54 - 55:59
    They make a hat, and take a
    [INAUDIBLE], put tickets in it.
  • 55:59 - 56:02
    And the teacher comes,
    and closes his eyes
  • 56:02 - 56:06
    and picks a ticket,
    and says oh my god, I
  • 56:06 - 56:08
    got proof of Fubini's theorem.
  • 56:08 - 56:11
    And do these three
    triple integrals.
  • 56:11 - 56:15
    This is a type of oral
    exam that you would have.
  • 56:15 - 56:19
    But if you know that,
    because you studied,
  • 56:19 - 56:23
    you're not afraid
    to present them.
  • 56:23 - 56:26
    But you have to present them,
    and you have a limited time.
  • 56:26 - 56:30
    Because there are other 30
    students in the classroom.
  • 56:30 - 56:32
    You only have five minutes.
  • 56:32 - 56:37
    And I only pick-- I want to
    see your work on all of them.
  • 56:37 - 56:38
    And I'll teach
    you how to present
  • 56:38 - 56:40
    on this problem on the board.
  • 56:40 - 56:42
    And then you have five
    minutes to present.
  • 56:42 - 56:47
    If you are really
    embarrassed and you
  • 56:47 - 56:50
    don't want to speak in public,
    then you have a problem.
  • 56:50 - 56:53
    I've had many fears--
    and in other countries--
  • 56:53 - 56:56
    I heard that in England,
    they have the same system.
  • 56:56 - 56:59
    There are people who are too
    shy to show their results,
  • 56:59 - 57:02
    or too shy to talk.
  • 57:02 - 57:05
    And then they start stuttering.
  • 57:05 - 57:07
    But they have to do it.
  • 57:07 - 57:10
    There is no excuse,
    they don't care if you
  • 57:10 - 57:13
    have problems with your speech.
  • 57:13 - 57:19
    So I asked the people I
    knew and I went to London,
  • 57:19 - 57:22
    and they said most people
    will stutter in there.
  • 57:22 - 57:24
    I was so scared.
  • 57:24 - 57:26
    Most people who stutter
    in our oral exams
  • 57:26 - 57:29
    are people who
    spend too much time
  • 57:29 - 57:32
    in the pub the previous day.
  • 57:32 - 57:36
    Pubs were everywhere and I saw
    lots of students in the pubs.
  • 57:36 - 57:40
    I went to University of Durham--
    this is where Harry Potter was
  • 57:40 - 57:42
    filmed, by the way.
  • 57:42 - 57:45
    I saw the castle, which
    is a student dorm.
  • 57:45 - 57:48
    You pay something
    like 500 pounds.
  • 57:48 - 57:52
    Which would be like $100?
  • 57:52 - 57:54
    $1,000?
  • 57:54 - 58:01
    Less, because I think it's
    7.50, something like $800.
  • 58:01 - 58:04
    It used to be that the
    pound was double the dollar.
  • 58:04 - 58:05
    [INTERPOSING VOICES]
  • 58:05 - 58:10
  • 58:10 - 58:16
    So you could stay in that
    dorm for $800 per month.
  • 58:16 - 58:21
    And you've got the same table
    where they ate in the movie.
  • 58:21 - 58:23
    It was really nice.
  • 58:23 - 58:27
    But the University of
    Durham is a isolated castle,
  • 58:27 - 58:30
    the cathedral,
    everything is very old,
  • 58:30 - 58:32
    from the 11th
    century, 12th century.
  • 58:32 - 58:37
    But if you go into the
    city, it's full of pubs.
  • 58:37 - 58:39
    Who is in the pubs?
  • 58:39 - 58:41
    The calculus students.
  • 58:41 - 58:43
    This is where they
    do their homework.
  • 58:43 - 58:48
    And it amazes me how
    they don't get drunk.
  • 58:48 - 58:50
    I'm not used to alcohol,
    because I don't drink.
  • 58:50 - 58:52
    Well they are used to it.
  • 58:52 - 58:57
    So they may nicely can do
    their homework, beautifully,
  • 58:57 - 59:01
    next to a big draft
    of Guinness like that.
  • 59:01 - 59:05
    And still makes sense when
    they write the solution.
  • 59:05 - 59:07
    They don't miss a minus
    sign, they're amazing.
  • 59:07 - 59:10
  • 59:10 - 59:13
    Alright, is this hard?
  • 59:13 - 59:18
    If you are interested, you
    can ask about study abroad.
  • 59:18 - 59:20
    We don't have big
    business with England,
  • 59:20 - 59:22
    but you could go to Seville.
  • 59:22 - 59:26
    There are some programs
    in the summer where
  • 59:26 - 59:29
    one of our professors teaches
    differential equations like I
  • 59:29 - 59:31
    told you about.
  • 59:31 - 59:34
    He teaches differential
    equations this summer
  • 59:34 - 59:34
    in Seville.
  • 59:34 - 59:40
  • 59:40 - 59:44
    I think you can still
    add in the next two days.
  • 59:44 - 59:47
    Some of you did,
    some of you didn't.
  • 59:47 - 59:49
    All right.
  • 59:49 - 59:53
    Any questions about
    other problems?
  • 59:53 - 59:58
    I have to apologize,
    I played the game
  • 59:58 - 60:01
    without telling you the truth.
  • 60:01 - 60:05
    [INAUDIBLE] he came to
    me last time and said,
  • 60:05 - 60:09
    you never showed
    us this notation.
  • 60:09 - 60:17
    So what if one gives you x
    of u, v equals 2x minus y.
  • 60:17 - 60:22
    y of u, v equals 3x plus y.
  • 60:22 - 60:25
    What the heck is that?
  • 60:25 - 60:27
    He didn't say heck, because
    he's a gentlemen, right?
  • 60:27 - 60:36
    But he said this is the
    notation used in web work,
  • 60:36 - 60:40
    and the book is actually not
    emphasizing it, which is true.
  • 60:40 - 60:46
    The book is emphasizing the
    Jacobian in section 12.8
  • 60:46 - 60:50
    only, which is not covered,
    it's not part of the menu.
  • 60:50 - 60:54
    But the definition, you
    should at least know it.
  • 60:54 - 60:57
    So what would be the
    definition of this animal?
  • 60:57 - 61:01
    You see that we have to take
    the partial derivative of x
  • 61:01 - 61:04
    with respect to u, the partial
    derivative of x with respect
  • 61:04 - 61:08
    to v, the partial derivative
    of y with respect to u,
  • 61:08 - 61:11
    and the partial derivative
    of y with respect to v.
  • 61:11 - 61:14
    And that's exactly what
    it is, indeterminate.
  • 61:14 - 61:15
    Not matrix, but indeterminate.
  • 61:15 - 61:18
  • 61:18 - 61:21
    So do I bother to write it down?
  • 61:21 - 61:23
    If I wanted to write
    down what it is,
  • 61:23 - 61:27
    of course I would write
    it down like that.
  • 61:27 - 61:31
    I don't want to spend
    all my time doing that,
  • 61:31 - 61:34
    because it's such
    an easy problem.
  • 61:34 - 61:36
    What do you have to do?
  • 61:36 - 61:40
    Just compute for such a simple
    transformation in plane.
  • 61:40 - 61:42
  • 61:42 - 61:45
    Actually, if you
    took linear-- again,
  • 61:45 - 61:50
    who is enrolled
    in linear algebra?
  • 61:50 - 61:51
    Only 1, 2, 3?
  • 61:51 - 61:52
    Thought there were only 2.
  • 61:52 - 61:53
    OK.
  • 61:53 - 61:59
    In linear algebra, you
    wrote this differently.
  • 61:59 - 62:06
    You wrote it like this. x and
    y equals matrix multiplication.
  • 62:06 - 62:11
    You have 2, minus
    1, 3, 1, by the way
  • 62:11 - 62:12
    it's obvious the
    determinate of this matrix
  • 62:12 - 62:14
    is different from 0.
  • 62:14 - 62:19
    This is the linear map that you
    are applying to the vector xy.
  • 62:19 - 62:26
    And in your algebra book,
    you're using Larson, am I right?
  • 62:26 - 62:29
  • 62:29 - 62:30
    Larson's book?
  • 62:30 - 62:31
    It's a good book.
  • 62:31 - 62:36
    So you have a of the vector x.
  • 62:36 - 62:43
    a of the vector x
    is the vector v.
  • 62:43 - 62:46
    When you all get to
    see linear algebra,
  • 62:46 - 62:53
    you'll like it more than Cal
    3, because it's more fun.
  • 62:53 - 62:56
    So how do you do this
    matrix multiplication?
  • 62:56 - 62:56
    It's very easy.
  • 62:56 - 62:59
    This time that, minus
    this times this.
  • 62:59 - 63:04
  • 63:04 - 63:07
    So can computers do that?
  • 63:07 - 63:11
    Yes, computers can, if you
    have the right program.
  • 63:11 - 63:14
    And this is the first
    program I learned in C++.
  • 63:14 - 63:16
    No, it was the second program.
  • 63:16 - 63:21
    How to write a little program
    for multiplication of two
  • 63:21 - 63:23
    matrices.
  • 63:23 - 63:28
    The first program I
    had, I learned in C++.
  • 63:28 - 63:31
    It was to build an ATM machine.
  • 63:31 - 63:37
    I hated that, because every time
    I went under 0 with my balance,
  • 63:37 - 63:40
    I would have new word under 0.
  • 63:40 - 63:43
    So I would have to prepare
    for all the possible cases
  • 63:43 - 63:45
    and save.
  • 63:45 - 63:48
    If you don't have
    enough money, whatever.
  • 63:48 - 63:52
    So that was the first
    program we wrote.
  • 63:52 - 63:55
    OK so, what do we have?
  • 63:55 - 64:02
    2 minus 1, 3 and 1.
  • 64:02 - 64:04
    What is the Jacobian
    in this case?
  • 64:04 - 64:06
    It's 2 plus 3, 5.
  • 64:06 - 64:07
    Different from 0.
  • 64:07 - 64:11
  • 64:11 - 64:14
    You have one or two
    problems like that.
  • 64:14 - 64:15
    Three problems.
  • 64:15 - 64:17
    I was really mean.
  • 64:17 - 64:18
    I apologize.
  • 64:18 - 64:20
    But you still have time
    to do those problems
  • 64:20 - 64:21
    in case of the review.
  • 64:21 - 64:24
    STUDENT: So we just take
    the determinate of it?
  • 64:24 - 64:28
    PROFESSOR: And you take the
    determinate of the matrix.
  • 64:28 - 64:30
    And that's you Jacobian.
  • 64:30 - 64:32
    STUDENT: What number is that?
  • 64:32 - 64:35
    PROFESSOR: I don't remember.
  • 64:35 - 64:37
    STUDENT: What if
    it's the u and the v
  • 64:37 - 64:42
    is at the top and x and
    the y at the bottom?
  • 64:42 - 64:43
    PROFESSOR: So the
    determinate will be the same.
  • 64:43 - 64:46
    This is a very good question.
  • 64:46 - 64:47
    Are you guys with me?
  • 64:47 - 64:52
    So he said, what if you have
    your first equation's name
  • 64:52 - 64:53
    would be this one.
  • 64:53 - 64:59
    And you have your equations
    written like that.
  • 64:59 - 65:01
    Right?
  • 65:01 - 65:06
    And so, when you
    look at this, you
  • 65:06 - 65:12
    will go-- it depends how you--
    in which order you do that.
  • 65:12 - 65:19
    I wrote u, v. Sorry.
  • 65:19 - 65:24
    u and v, but you
    understood what I meant.
  • 65:24 - 65:25
    Right?
  • 65:25 - 65:26
    u and v.
  • 65:26 - 65:29
    STUDENT: Can you
    do number three?
  • 65:29 - 65:30
    It was a hard one.
  • 65:30 - 65:31
    PROFESSOR: I will,
    just a second.
  • 65:31 - 65:38
    So d y, x with respect to u,
    v. What would happen, I just I
  • 65:38 - 65:41
    would flip the x and y.
  • 65:41 - 65:42
    What will happen?
  • 65:42 - 65:47
    I get 3, 1, it's still
    the same function.
  • 65:47 - 65:49
    2, and minus 1.
  • 65:49 - 65:52
    Why do I get minus 5?
  • 65:52 - 65:59
  • 65:59 - 66:03
    So imagine guys, what happens
    when you have x and y?
  • 66:03 - 66:07
    If you rotate, you don't
    change the sign of your matrix,
  • 66:07 - 66:08
    or notation.
  • 66:08 - 66:12
    Matrix notation will
    always have [INAUDIBLE].
  • 66:12 - 66:17
    But if you flip it,
    if you swap x and y,
  • 66:17 - 66:22
    you are actually changing
    the sign of the Jacobian,
  • 66:22 - 66:24
    the sign of the matrix.
  • 66:24 - 66:28
    You are changing
    your orientation.
  • 66:28 - 66:31
    That would be a
    hypothetical situation.
  • 66:31 - 66:33
    You are changing
    your orientation.
  • 66:33 - 66:37
    Do you have a number, Ryan?
  • 66:37 - 66:38
    Is it hard?
  • 66:38 - 66:39
    Why is it hard?
  • 66:39 - 66:43
  • 66:43 - 66:46
    Yeah, let me do that.
  • 66:46 - 66:55
  • 66:55 - 66:56
    It's hard enough.
  • 66:56 - 67:00
  • 67:00 - 67:01
    It's computation.
  • 67:01 - 67:26
  • 67:26 - 67:27
    Were you able to do it?
  • 67:27 - 67:32
  • 67:32 - 67:34
    Not yet, right?
  • 67:34 - 67:40
    So this is x, not-- OK.
  • 67:40 - 67:47
    So you can write this also,
    differently, except the y sub
  • 67:47 - 67:52
    u, y sub v. Who
    can tell me-- there
  • 67:52 - 67:56
    are ways to do it
    in a simpler way.
  • 67:56 - 67:59
    But I don't want to tell
    you yet what that way is.
  • 67:59 - 68:01
    And I'll show you next time.
  • 68:01 - 68:03
    What is x sub u?
  • 68:03 - 68:06
  • 68:06 - 68:11
    It shouldn't be so hard
    because it's the quotient rule.
  • 68:11 - 68:16
    You have 4 times u squared
    plus v squared minus
  • 68:16 - 68:25
    [INAUDIBLE] minus 2u the
    derivative of this times 4u
  • 68:25 - 68:30
    divided by the square of that.
  • 68:30 - 68:34
    Did I go too fast?
  • 68:34 - 68:39
    So what you have is 4u
    squared minus 8u squared
  • 68:39 - 68:46
    equals minus 4u squared plus
    4v squared divided by that.
  • 68:46 - 68:54
  • 68:54 - 68:55
    v squared.
  • 68:55 - 68:56
    Squared, sorry.
  • 68:56 - 68:58
  • 68:58 - 69:02
    x of v, that should be easier.
  • 69:02 - 69:03
    Why is it easy?
  • 69:03 - 69:14
    The first guy prime
    minus the second guy
  • 69:14 - 69:16
    So the first primes,
    second not prime.
  • 69:16 - 69:21
    Minus second prime, straight to
    v, times the first not prime.
  • 69:21 - 69:25
  • 69:25 - 69:29
    Divided by u squared.
  • 69:29 - 69:35
    Which is minus 8uv over that.
  • 69:35 - 69:41
    Is this one of those that you
    said you couldn't do it yet?
  • 69:41 - 69:42
    You?
  • 69:42 - 69:43
    Both?
  • 69:43 - 69:44
    You did this one?
  • 69:44 - 69:48
    You got the right answer, good.
  • 69:48 - 70:02
    y sub v. Y sub u, it's OK
    to have a minus 0 times
  • 70:02 - 70:05
    the second one.
  • 70:05 - 70:14
    Minus this prime with
    respect to u, times
  • 70:14 - 70:22
    6v over the square of that.
  • 70:22 - 70:30
    And finally, y sub v
    equals minus the derivative
  • 70:30 - 70:35
    of the top, with respect to
    6v times u squared plus v
  • 70:35 - 70:39
    squared minus the derivative
    of the bottom with respect
  • 70:39 - 70:52
    to v. v times 6v divided
    by the whole shebang.
  • 70:52 - 70:53
    Now is it simplified?
  • 70:53 - 70:56
    No, I will simplify in a second.
  • 70:56 - 70:59
    You get minus 12uv.
  • 70:59 - 71:03
    I'm not going to finish
    it, but we are almost done.
  • 71:03 - 71:04
    Why are we almost done?
  • 71:04 - 71:06
    This is very easy.
  • 71:06 - 71:09
    I mean, not very
    easy, but doable.
  • 71:09 - 71:11
    How about this guy?
  • 71:11 - 71:13
    What do you get?
  • 71:13 - 71:18
    A 6u squared, a 6v squared,
    a minus 12v squared.
  • 71:18 - 71:19
    It's not that bad.
  • 71:19 - 71:25
    So you have 6u squared
    minus 6v squared,
  • 71:25 - 71:27
    over u squared plus v squared.
  • 71:27 - 71:32
  • 71:32 - 71:34
    What did I do?
  • 71:34 - 71:38
  • 71:38 - 71:39
    Add a minus in front.
  • 71:39 - 71:41
    I didn't copy.
  • 71:41 - 71:43
    Let me make room
    for that, thank you.
  • 71:43 - 71:46
    STUDENT: It's also the 12.
  • 71:46 - 71:50
    It's 12uv, because there's
    a negative in front of it.
  • 71:50 - 71:52
    It's minus times minus.
  • 71:52 - 71:53
    PROFESSOR: Here?
  • 71:53 - 71:54
    STUDENT: No, y sub u.
  • 71:54 - 71:55
    The third one.
  • 71:55 - 71:58
    PROFESSOR: Minus, minus,
    plus, that's good.
  • 71:58 - 72:00
    Thanks for observing things.
  • 72:00 - 72:03
    Anything else that's fishy?
  • 72:03 - 72:04
    Minus, minus, plus.
  • 72:04 - 72:07
  • 72:07 - 72:08
    OK that's better.
  • 72:08 - 72:09
    Change the signs.
  • 72:09 - 72:14
    When I move onto this one,
    remind me to change the signs.
  • 72:14 - 72:15
    So what is the Jacobian?
  • 72:15 - 72:18
    I'm too lazy to
    write this thing.
  • 72:18 - 72:22
    I'm going to have-- so, x sub u.
  • 72:22 - 72:26
  • 72:26 - 72:32
    4 times v squared
    minus u squared.
  • 72:32 - 72:37
    Let's me count the OK.
  • 72:37 - 72:39
    Let's do it over a.
  • 72:39 - 72:42
  • 72:42 - 72:44
    I'll show you what happens.
  • 72:44 - 72:46
    Maybe you don't know
    yet what happens,
  • 72:46 - 72:49
    but I'll show you what happens.
  • 72:49 - 72:58
    Then the next one is going to
    be x sub v minus 8, uv over a.
  • 72:58 - 73:05
    y sub u, 12.
  • 73:05 - 73:13
    uv over a, and last,
    with your help.
  • 73:13 - 73:18
    It's plus this was
    my-- so 6 times v
  • 73:18 - 73:21
    squared minus u squared over a.
  • 73:21 - 73:24
  • 73:24 - 73:26
    OK OK, let me erase.
  • 73:26 - 73:30
  • 73:30 - 73:33
    So you guys know
    what happens when
  • 73:33 - 73:36
    you have something like that?
  • 73:36 - 73:41
    A determinate has one
    line multiplied or column
  • 73:41 - 73:43
    multiplied by a number.
  • 73:43 - 73:50
    If you have alpha a,
    alpha b, alpha c and d.
  • 73:50 - 73:55
    The determinate of that
    is alpha aut, a, b, c, d.
  • 73:55 - 73:57
    I assume you know
    this from high school,
  • 73:57 - 74:00
    but I know very well
    that many of you don't.
  • 74:00 - 74:02
    How do you prove this?
  • 74:02 - 74:03
    Very easily.
  • 74:03 - 74:06
    This times that would be
    an alpha out, minus this,
  • 74:06 - 74:08
    and alpha out.
  • 74:08 - 74:11
    It's very easy to prove.
  • 74:11 - 74:17
    So when you have one line or one
    column multiplied by an alpha,
  • 74:17 - 74:19
    that alpha gets out.
  • 74:19 - 74:23
    So if you have two lines
    multiplied by an alpha,
  • 74:23 - 74:28
    or two rows, alpha
    squared, excellent.
  • 74:28 - 74:29
    So who gets out?
  • 74:29 - 74:37
    1 over a squared, which
    means this guy to the fourth.
  • 74:37 - 74:40
    Sorry that this is so long.
  • 74:40 - 74:43
    I don't like this problem,
    because of this computation
  • 74:43 - 74:45
    you have to go through here.
  • 74:45 - 74:52
  • 74:52 - 74:57
    So I would simplify
    it as much as I could.
  • 74:57 - 75:02
    Let's see, before I
    missed my a group.
  • 75:02 - 75:12
    So you have 24 times v squared
    minus u squared, plus 96,
  • 75:12 - 75:14
    am I right?
  • 75:14 - 75:19
    v squared divided by all
    this ugly guy which I hate,
  • 75:19 - 75:20
    to the fourth.
  • 75:20 - 75:23
  • 75:23 - 75:27
    Fortunately, everybody's
    a multiple of 24.
  • 75:27 - 75:31
    So we can pull a 24 out.
  • 75:31 - 75:35
    and get it out of our life,
    because it drives us crazy.
  • 75:35 - 75:40
    And then you have v to the
    fourth plus u to the 4,
  • 75:40 - 75:40
    minus twice.
  • 75:40 - 75:42
    Was that the binomial format?
  • 75:42 - 75:45
    Minus 2 us squared, v squared.
  • 75:45 - 75:48
    What was left when
    I pull this out?
  • 75:48 - 75:52
  • 75:52 - 75:56
    I pulled 24 out, 96 is what?
  • 75:56 - 75:56
    4.
  • 75:56 - 76:02
    So I have a 4 left.
  • 76:02 - 76:04
    So I would put that down.
  • 76:04 - 76:09
    4u squared, v squared over
    the-- it looks symmetric
  • 76:09 - 76:11
    but-- that's OK.
  • 76:11 - 76:14
    It's not so bad.
  • 76:14 - 76:15
    So can you write this better?
  • 76:15 - 76:18
    Look at it.
  • 76:18 - 76:20
    Do you like it?
  • 76:20 - 76:22
    There is a 3.
  • 76:22 - 76:27
    The 4 the 2, 4
    minus 2 is a plus 2.
  • 76:27 - 76:30
    Just like when we did those
    tricky things in high school.
  • 76:30 - 76:33
    That would be, again,
    the binomial formula.
  • 76:33 - 76:35
    u squared plus v squared.
  • 76:35 - 76:39
  • 76:39 - 76:41
    Are you guys with me?
  • 76:41 - 76:44
    Because minus 2
    plus 4 is plus 2.
  • 76:44 - 76:47
    This is exactly the
    same thing as that.
  • 76:47 - 76:51
    Over u squared plus v
    squared to the fourth.
  • 76:51 - 76:53
    If you have problems
    computing that,
  • 76:53 - 76:56
    send me some emails from
    WebWork, because I'm
  • 76:56 - 76:59
    going to help you do that, OK.
  • 76:59 - 77:03
    24 divided by what?
  • 77:03 - 77:05
    Yes?
  • 77:05 - 77:10
    u squared plus v
    squared squared.
  • 77:10 - 77:13
    Oh my god.
  • 77:13 - 77:13
    All right.
  • 77:13 - 77:17
    So, I'm not going to
    think lesser of you
  • 77:17 - 77:21
    if you don't put
    all of this here.
  • 77:21 - 77:26
    Therefore, if you
    get in trouble,
  • 77:26 - 77:31
    click from the expression from
    the whatever you got, and say,
  • 77:31 - 77:34
    this horrible problem gives
    me a headache, help me.
  • 77:34 - 77:38
    And I'm going to help you with
    that simple computation that
  • 77:38 - 77:40
    is just algebra.
  • 77:40 - 77:43
    That's not going to teach you
    anything more about Cal 3.
  • 77:43 - 77:44
    That's why I'm
    going to help you.
  • 77:44 - 77:47
    I'll help you with
    the answers on those.
  • 77:47 - 77:50
    Just send me an email.
  • 77:50 - 77:57
    I'm planning on still
    reviewing even on Tuesday.
  • 77:57 - 78:00
    I don't want to teach anything
    new, because I'm tired
  • 78:00 - 78:02
    and-- I'm just kidding.
  • 78:02 - 78:05
    I don't want to teach
    anything new on Tuesday,
  • 78:05 - 78:10
    because I want you to be very
    well prepared for the midterms.
  • 78:10 - 78:13
    So I'll do a general
    review again,
  • 78:13 - 78:16
    and I'll go over some
    homework like problems,
  • 78:16 - 78:21
    but mostly over
    exam like problems.
  • 78:21 - 78:26
    So I want everybody to succeed,
    to get very high scores.
  • 78:26 - 78:29
    But we need to practice,
    practice, practice.
  • 78:29 - 78:31
    It's like you did
    before your SATs.
  • 78:31 - 78:34
  • 78:34 - 78:40
    It's not that much, I mean what
    happens if you don't do great
  • 78:40 - 78:40
    on the midterm?
  • 78:40 - 78:47
    Well the midterms is
    a portion the final.
  • 78:47 - 78:50
    But what I am trying
    to do by reviewing
  • 78:50 - 78:53
    so much for the
    midterm is also trying
  • 78:53 - 78:55
    to help you for the final.
  • 78:55 - 78:57
    Because on the final,
    half of the problems
  • 78:57 - 79:00
    will be just like the ones
    on the midterm Emphasizing
  • 79:00 - 79:03
    the same type of concepts.
  • 79:03 - 79:06
    It's good practice
    for the final as well.
  • 79:06 - 79:07
    All right, good luck.
  • 79:07 - 79:09
    I'll see you Tuesday.
  • 79:09 - 79:13
    Let me know by email how
    it goes with the problems.
  • 79:13 - 79:19
Title:
TTU Math2450 Calculus3 Secs 12.7 - 12.8
Description:

Review of Integration in 3 dimensions and Jacobian of a transformation

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Video Language:
English

English subtitles

Revisions