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TTU Math2450 Calculus3 chap. 10-11-12 review

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    PROFESSOR: Questions so far?
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    STUDENT: [INAUDIBLE]
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    PROFESSOR: Yes, ma'am.
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    You are Megan?
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    STUDENT: Yes.
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    PROFESSOR: OK.
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    STUDENT: I was just wondering
    if we get like a form
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    of [INAUDIBLE], note cards--
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    PROFESSOR: No, you
    [INAUDIBLE] sheet whatsoever.
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    So I think it's better that
    I review some of the formulas
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    today that you are
    expected to know by heart,
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    because they are also-- they
    require you know to expect you
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    to know the same formulas
    by heart for the final
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    with no cheat sheet.
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    So the final will have
    exactly the same policy,
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    at the end of [INAUDIBLE].
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    No calculator, no formula sheet,
    no cheat sheet, no nothing,
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    but you know I'm telling
    you guys this, except what
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    you remember.
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    Let me remind you
    that you are expected
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    to know the equation
    of the tangent plane.
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    I'm not going to give them
    in chronological order,
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    but I think it's a good idea to
    review for midterm and final,
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    some of the must-know formulas.
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    One, well, I discussed this
    before but I didn't remind you,
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    differential of a function
    of several variables.
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    In particular, two
    variables most likely
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    are the examples we've worked
    on a lot this semester.
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    Number two, the definition
    and especially formula,
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    main formula for responding to
    directional derivatives of F
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    at P of coordinates X 0, Y 0,
    in the direction U 1 and U 2,
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    equals U.
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    Just to test you,
    OK, well, I believe
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    you know the formula
    of the differential.
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    But without me reminding you
    what was that of two variables,
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    I expect you to say d F equals--
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    STUDENT: F [INAUDIBLE].
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    D X plus F Y, D Y.
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    PROFESSOR: How
    about-- thank you--
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    how about the
    directional derivative
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    of F at P in the
    direction of the vector U?
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    You will need the formula.
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    Good, [INAUDIBLE].
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    Yeah, that's the easiest
    way to remember it,
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    but that's not the first thing
    I want you to say, right?
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    How did I write this?
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    [INAUDIBLE]
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    Of course, F of X-- thank
    you-- and [INAUDIBLE] 0,
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    times Z 1 plus
    derivative inspect Y,
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    and X 0, Y 0 times U 2.
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    What do we assume about it, F
    C 1 on the domain [INAUDIBLE]?
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    Which means differential goal
    with continuous derivatives.
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    This is what we assume
    through chapter 11.
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    Number three, I think I
    told you, but I'm not sure.
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    But I think I did.
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    Review the tangent
    plane formula,
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    formulas-- how about both?
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    Well, only one is the one
    I consider relative for us.
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    Which is Z equals F of X,
    Y, will imply that at P
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    with on the surface,
    even as a reference, we
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    have a tangent plane
    of formula Z minus Z 0,
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    equals-- who does it?
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    OK, now you have
    to remember this.
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    Of course, it's your midterm.
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    Review all of these things
    by [INAUDIBLE] Thursday.
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    Variable S of X,
    [INAUDIBLE] 0 at 0, times--
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    STUDENT: X minus X 0.
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    PROFESSOR: Thank you,
    Roberto, X 0 minus X 0,
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    plus the same kind o thing in
    a different color, because I
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    like to play [INAUDIBLE] orange,
    S Y, X 0, Y 0, Y minus Y 0.
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    Don't come to the midterm-- you
    better not come to the midterm,
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    and you get a 0 for not
    knowing the formulas, right?
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    Now maybe you will see
    on this midterm, maybe
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    not, maybe you'll see
    it on the final-- what
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    happens when you don't have
    the graph of a surface?
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    Maybe you'll have an implicit
    equation, an implicit equation
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    where we write F of coordinates,
    X, Y and Z, equals a constant.
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    Why is the tangent plane a P?
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    Tangent plane, tangent plane
    in both cases should be Y.
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    Well, if you consider
    the first formula
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    as a consequence
    of the second one,
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    that would be simply
    easy, because you
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    will have to write F of
    X Y minus Z equals 0.
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    And there you are, the same
    kind of formula in this.
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    So what do you write--
    remember the surface,
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    the implicit formula.
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    Who gave you the normal to
    the surface of a point P?
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    No?
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    The gradient of who?
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    Not the gradient of the left,
    don't confuse-- the gradient
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    of the big F, right?
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    OK, at P. And the tangent
    plane represents a what?
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    The tangent plane represents
    exactly the perpendicular plane
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    that passes through the
    point P, and is [INAUDIBLE]
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    to the normal.
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    So you're going to have
    your surface, your normal,
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    and the tangent plane, which
    is perpendicular to the normal.
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    Is this easy to remember,
    maybe for your final?
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    I want to check if you know--
    make a list, this list,
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    you have to post it in
    the bathroom or somewhere,
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    on the wall or a closet.
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    Because you need to know
    these things by the final.
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    S of X at point P becomes
    S minus X 0 plus what?
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    The same kind of thing, right?
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    But it [INAUDIBLE] Y and Z.
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    So if you have the
    curiosity to want
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    to prove that the first colorful
    formula for the tangent plane,
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    using the red formula for the
    tangent plane, it would come,
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    is an immediate [INAUDIBLE].
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    We've actually done that before.
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    We even did the implicit
    function theorem.
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    There are some very
    nice things you
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    can do when you have a
    function of several variables.
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    And in particular, for a
    function of two variables,
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    makes it really easy.
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    I'm gonna erase one,
    two, three, and continue.
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    So I guess when
    I leave the room,
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    I have to be careful not
    to leave the actual midterm
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    in the room, although I
    know that you wouldn't even
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    try to check my papers.
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    I did also something
    in this for finding
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    a direction in which
    the function increases
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    most rapidly.
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    I don't have to
    write it down, but I
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    can remind you of the concept.
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    So it's just the concept now,
    no formula to actually memorize.
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    But I'll still say number
    four, problem number four,
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    because that's what I set
    up on the actual exam.
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    So what is the direction of
    highest ascend, deepest ascend?
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    STUDENT: [INAUDIBLE].
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    PROFESSOR: Is the
    direction of the plane.
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    And what is the direction
    of the steepest descent?
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    The opposite of the
    direction of the grade.
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    So the direction of
    steepest ascend and descend
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    is the direction of for the
    graph Z equals F of X 1.
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    This is the function [INAUDIBLE]
    that I'm talking about.
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    Five, the direction
    of U that you
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    found at the previous problem,
    I didn't ask if it's unique, OK?
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    Because that was one--
    of course it's unique.
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    Because we [INAUDIBLE] sizes.
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    How do you say units
    of sizing, [INAUDIBLE]?
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    By deriving with it,
    [INAUDIBLE] a second,
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    you have a U and a -U.
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    STUDENT: So isn't the direction
    that the actual [INAUDIBLE]
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    for is the gradient
    of a normal vector?
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    PROFESSOR: So yeah,
    so the way I-- OK, you
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    want me to read the problem?
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    I'm going to read the actual
    function So find the direction
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    U, in which the function F of
    X Y, blah, blah, blah, blah,
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    is here, it increases
    most rapidly.
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    So what do you have to do?
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    So the direction
    of that is, what is
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    the direction of that or this?
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    U equals [INAUDIBLE]
    respectively minus U at P.
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    Five, this direction U that you
    found at the previous problem,
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    could be perpendicular
    to a certain line, which
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    of the following planes?
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    I may give you multiple choice.
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    Now what do you have
    to do when you think
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    the direction of-- the way
    it's actually formulated
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    is zero direction
    is parallel to one
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    of the following [INAUDIBLE]
    planes, which one?
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    Let me give you an example.
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    Z equals X [INAUDIBLE]
    squared, at P coordinates 1, 1.
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    So that means X 0 is 1,
    Y 0 is 1, and Z 0 is two.
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    Find the direction
    of the gradient of F.
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    Let me put Z for alpha-- I'm
    abusing my [INAUDIBLE]-- at P.
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    And state which of the following
    lines is parallel for this
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    direction?
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    A, lines in plane.
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    X equals 2.
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    B, Y equals 3.
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    Or C, X plus 1 equals 0.
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    D, these are lines in
    plane in the plane,
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    X Y. X plus Y. E,
    none of the above.
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    So how are you going
    to do that quickly?
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    Well, it's easy, right?
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    So what do I do?
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    I say gradient 2 X
    2 Y, at the point
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    1, 1-- you don't have to
    write down everything.
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    It's going to be the gradient
    of F at P, will be 2, 2.
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    That means U will
    be normalized 2, 2.
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    What do you get?
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    STUDENT: [INAUDIBLE]
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    PROFESSOR: Well, what
    do people do normally
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    if they want to do
    it by the definition?
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    They [INAUDIBLE]
    the vector 2, 2,
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    by the square root [INAUDIBLE].
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    Well, you could be a little
    bit smarter than that,
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    and say, F is the same
    as the direction 1,
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    1 divided by the square
    root of the sums,
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    of a sum of the squares.
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    It doesn't matter
    which one you pick.
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    All the co-linear ones
    will reveal the unique U.
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    And that's exactly what
    I was trying to say,
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    was this thinking by in just two
    or three moves ahead of that.
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    STUDENT: So that's the
    same as 2, 2 over 4?
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    PROFESSOR: Yes, sir.
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    It's the same as 2, 2 over
    the square root of 4 plus 4.
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    But it's easier, why it's
    sort of faster to do it.
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    So why is that true
    actually, Ryan is very right?
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    Why is that true?
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    Exactly because of that
    uniqueness that I told you
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    about last time, when you
    said, well, [INAUDIBLE],
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    what is that?
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    So you get 1 over square root of
    2, and 1 over square root of 2,
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    is that you [INAUDIBLE]
    vector direction.
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    Now without doing
    further work, this
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    is just a simple
    multiple question,
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    of [INAUDIBLE] question.
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    You are in front of your exam,
    and you see lines in play.
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    You close your eyes and see
    all of-- I will see my what?
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    You see all the lines in plane.
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    Of all these lines,
    your favorite line
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    has to have the same direction
    as the vector U. Is X equals 2?
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    No, that's nothing.
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    Y equals 3?
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    Those are horizontal, vertical.
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    That's the direction of
    the first [INAUDIBLE].
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    So is this true of C?
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    No.
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    STUDENT: No, that's
    for parallel lines.
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    PROFESSOR: D?
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    STUDENT: Yes.
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    PROFESSOR: Right?
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    So the incline X, Y--
    the first bisector
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    is X equals Y [INAUDIBLE].
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    Number C is Y minus X, which
    is called the second bisector.
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    You've seen that in college
    algebra-- high school algebra,
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    more likely.
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    So we call this first
    bisector, second bisector.
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    All right, so the
    answer is D. Do you have
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    the same thing [INAUDIBLE]?
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    On the two multiple
    choice things
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    you have, you see very
    well, OK, I'm testing you.
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    I didn't say anything.
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    It was three feet away, OK?
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    We have just a quick
    answer, and it's
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    going to be easy,
    without algebra,
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    without computational stuff.
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    Just from the first glance,
    you'll be able to answer.
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    Number six, what
    is the maximum rate
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    of increase in the same
    case as in problem five?
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    You say [INAUDIBLE], what
    is the maximum, maximal rate
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    of increase of a [INAUDIBLE]?
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    And we all know what
    I'm talking about,
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    although maybe not everybody.
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    But this is the gradient.
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    Who is giving you the
    maximum rate of increase?
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    As I said last
    time in the review,
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    that's actually the
    directional derivative
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    in the direction
    of the gradient.
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    But you are supposed to
    know without proving again
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    that the directional
    derivative and the direction
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    of the gradient will
    give you that what?
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    Gradient of norm of--
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    STUDENT: [INAUDIBLE].
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    PROFESSOR: Exactly, the
    magnitude of this F. So
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    what does that-- what
    would that be in my case?
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    [INAUDIBLE] pay
    attention, please.
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    Don't look at this,
    if it's confusing you.
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    Look at that, right?
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    How much is that?
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    All right, [INAUDIBLE].
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    So you can put this
    as [INAUDIBLE].
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    So your multiple choice-- how
    many multiple choices do you
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    have?
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    Only two.
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    It may seem like what
    is the maximum rate?
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    1, 0, 0, is telling-- that
    means you have no increase.
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    You're not moving.
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    You're just lying
    there on the plane.
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    OK.
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    What else?
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    2 root 2, 2 [INAUDIBLE]
    to infinity.
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    I don't know.
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    I'm giving some
    nonsensical choices.
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    But one of them
    would be 2 root 2.
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    So you would see, it would
    jump in front of your eyes.
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    Number seven, I think I'm
    going-- I thought about this,
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    and I said one of
    you guys asked me,
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    can you re-open any homework?
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    And I said, nope.
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    Why?
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    Because once the homework
    closes, automatically
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    a few seconds later, all
    the answers are gonna be up.
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    Do I have other
    problems handy to create
  • 20:24 - 20:29
    a make-up for that individual
    person who had the problem?
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    My cat almost died this
    week, but she said,
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    but I have a treatment, and
    hopefully she's going to live.
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    So in situations of [INAUDIBLE],
    like an accident, a problem,
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    [INAUDIBLE] hospitalization,
    and so on, I'm sorry,
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    I cannot re-open the homework.
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    The homework is already up
    there with all the answers.
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    When I extend homework, it's
    still doing that interval when
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    you cannot see the answers.
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    So I can extend it
    by there [INAUDIBLE],
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    that was an exception.
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    So you have until the
    fourth-- is the the fourth?
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    OK.
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    But once that closes,
    I cannot re-open it.
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    However, I thought of giving
    you a compensation midterm exam,
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    contains an extra
    credit problem.
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    Because once you told
    me that, I started
  • 21:21 - 21:27
    feeling bad for the two
    people who have problems.
  • 21:27 - 21:31
    There were two or three people
    who had very serious problems
  • 21:31 - 21:34
    this past weekend.
  • 21:34 - 21:37
    So in the midterm, you have
    that extra credit problem,
  • 21:37 - 21:41
    that is meant to touch up
    a little bit of let's say
  • 21:41 - 21:45
    if you missed a few
    problems from the homework,
  • 21:45 - 21:48
    you had some bad day, whatever.
  • 21:48 - 21:51
    So you have ten
    problems plus one.
  • 21:51 - 21:57
    Seven, you've seen that
    before I told you about it.
  • 21:57 - 22:00
    It's an easy problem.
  • 22:00 - 22:07
    You have Z equals
    F over X Y. And I'm
  • 22:07 - 22:28
    saying compute the volume of the
    body that lies below the graph
  • 22:28 - 22:40
    and above the unit
    [INAUDIBLE] D. Fine.
  • 22:40 - 22:46
    Eight, unfortunately
    eight have [INAUDIBLE]
  • 22:46 - 22:49
    was disclosed because
    Ryan was dreaming
  • 22:49 - 22:51
    of the problems in the midterm.
  • 22:51 - 22:56
    But it was something like
    that, very good information.
  • 22:56 - 23:02
    So I would say a problem
    like that, maybe a plane that
  • 23:02 - 23:05
    is cut in what?
  • 23:05 - 23:09
    The plane's coordinates form
    something like a tetrahedron,
  • 23:09 - 23:14
    find the volume,
    something like that.
  • 23:14 - 23:21
    Nine, again without giving
    you the exact values,
  • 23:21 - 23:26
    you will have a function
    F of X, and U of X,
  • 23:26 - 23:30
    I'd say positive over
    a certain interval.
  • 23:30 - 23:35
  • 23:35 - 23:45
    Set up the double integral,
    set up a double integral
  • 23:45 - 23:52
    for the area of the domain
    between F and G contained.
  • 23:52 - 24:01
  • 24:01 - 24:15
    Compute that, and also reverse
    the order of integration
  • 24:15 - 24:17
    to check your work.
  • 24:17 - 24:19
  • 24:19 - 24:25
    Your answer, because here,
    a multiple choice answer,
  • 24:25 - 24:28
    [INAUDIBLE] answer, no guesses.
  • 24:28 - 24:30
    It's going to not be
    hard at all-- very
  • 24:30 - 24:33
    nice, friendly functions, very
    nice, friendly [INAUDIBLE]
  • 24:33 - 24:34
    functions.
  • 24:34 - 24:38
    Just I have done this
    before, but I'm not
  • 24:38 - 24:40
    going to repeat what it was.
  • 24:40 - 24:45
    I did it in the-- it's like
    the one I did last week.
  • 24:45 - 24:49
  • 24:49 - 24:53
    All right, so remember you
    write the vertical strip thing,
  • 24:53 - 24:56
    integration with respect to Y
    first, and then with respect
  • 24:56 - 24:59
    to X. You switch to
    the horizontal strip
  • 24:59 - 25:02
    method of integration
    with respect
  • 25:02 - 25:08
    to X first, and then with
    respect to Y. Okie-doke?
  • 25:08 - 25:13
    And the actual algebra
    here will be [INAUDIBLE]
  • 25:13 - 25:16
    expect to be done in one line.
  • 25:16 - 25:20
    So you will have something
    extremely simple.
  • 25:20 - 25:24
    Ten-- it's another long exam.
  • 25:24 - 25:28
    So I have to try
    to test everything
  • 25:28 - 25:31
    you know without you
    spending more than one minute
  • 25:31 - 25:37
    per problem, just to conceive
    the result. Formally,
  • 25:37 - 25:39
    hold on-- now nine, I split it.
  • 25:39 - 25:41
    Because I felt pity for you.
  • 25:41 - 25:46
    So I put [INAUDIBLE], I put
    just set up the level integral,
  • 25:46 - 25:50
    and reverse the
    order of integration.
  • 25:50 - 25:54
    So you have to write integral
    integral equals integral
  • 25:54 - 25:57
    integral, nothing else,
    no answer, no number.
  • 25:57 - 26:07
    And ten, actually compute
    any of the two integrals
  • 26:07 - 26:15
    at number nine to find
    the area of the domain.
  • 26:15 - 26:18
  • 26:18 - 26:22
    Just like we did
    last time, and you
  • 26:22 - 26:24
    don't have a calculator, OK?
  • 26:24 - 26:28
    Suppose your answer will
    be-- what was last time?
  • 26:28 - 26:30
    One over six, I don't know.
  • 26:30 - 26:33
    If you give me decimals,
    I will be very upset.
  • 26:33 - 26:37
    You have to give me the precise
    answer for that problem,
  • 26:37 - 26:41
    because it's so easy to
    compute that you would have
  • 26:41 - 26:47
    no need for using a calculator
    or software, or any kind
  • 26:47 - 26:51
    of electronic device.
  • 26:51 - 26:57
    And finally number
    11-- and number 11, I
  • 26:57 - 27:01
    shouldn't say what it is,
    because it's extra credit.
  • 27:01 - 27:03
    But I'll still say what it is.
  • 27:03 - 27:05
    It's some simple
    integral where you
  • 27:05 - 27:08
    are going to have to use
    spherical coordinates.
  • 27:08 - 27:10
    And shut up,
    [INAUDIBLE], because you
  • 27:10 - 27:12
    are talking too much.
  • 27:12 - 27:16
    So again, number 11 will
    be a triple integral
  • 27:16 - 27:18
    that is easy to compute.
  • 27:18 - 27:23
    And when you're going-- well,
    you don't have to use vehicle.
  • 27:23 - 27:26
    You can still do it with
    cylindrical coordinates,
  • 27:26 - 27:27
    for example.
  • 27:27 - 27:33
    But it's a big pain doing
    the cylindrical coordinates
  • 27:33 - 27:35
    for that kind of problem.
  • 27:35 - 27:41
    So imagine maybe I'm looking
    at the domain to be a sphere.
  • 27:41 - 27:44
  • 27:44 - 27:49
    The problems we worked
    as a training in class,
  • 27:49 - 27:53
    are actually harder than
    the ones I put on the exam.
  • 27:53 - 27:58
    I have a professor who's a grad
    student, and he used to say,
  • 27:58 - 28:01
    the easy problems
    are the professor
  • 28:01 - 28:03
    to work in classes examples.
  • 28:03 - 28:08
    The hard problems are the
    students who have on the exam.
  • 28:08 - 28:10
    I think exactly the opposite.
  • 28:10 - 28:18
    Because when you will in
    training for any kind of sports
  • 28:18 - 28:21
    or a skill or music, you
    have to train yourself
  • 28:21 - 28:26
    above the level of
    your competition.
  • 28:26 - 28:29
    Otherwise your
    competition will be bored.
  • 28:29 - 28:31
    So what you're
    doing with training
  • 28:31 - 28:33
    should not always
    be how whether you
  • 28:33 - 28:37
    are an athlete or a
    mathematician or a violinist
  • 28:37 - 28:39
    or whatever.
  • 28:39 - 28:44
    So you're not going to see
    something like intersector
  • 28:44 - 28:49
    cylinders, passing one through
    the other, one the cone,
  • 28:49 - 28:51
    ice cream cone will
    be doing a parabola,
  • 28:51 - 28:55
    then the cone is full of ice
    cream-- nothing like that.
  • 28:55 - 28:58
    Something simpler.
  • 28:58 - 29:02
    And you may guess what it is,
    but keep in mind that force
  • 29:02 - 29:06
    of speed components, you
    have to know the Jacobian,
  • 29:06 - 29:07
    don't hesitate.
  • 29:07 - 29:10
    That's assumed to be memorized.
  • 29:10 - 29:12
    Don't ask me in the
    middle of the exam.
  • 29:12 - 29:14
    Why was the Jacobian
    [INAUDIBLE] components?
  • 29:14 - 29:17
    You are supposed to
    know that as being what?
  • 29:17 - 29:18
    What was that?
  • 29:18 - 29:19
    Roberto knows.
  • 29:19 - 29:20
    [INTERPOSING VOICES]
  • 29:20 - 29:22
    PROFESSOR: [INAUDIBLE]
    assign by, and by
  • 29:22 - 29:25
    was what, for a friend of yours?
  • 29:25 - 29:29
    The latitude from Santa Claus,
    measured down all the way
  • 29:29 - 29:31
    to [INAUDIBLE].
  • 29:31 - 29:35
    Theta is the longitude
    from 0 to 2 pi.
  • 29:35 - 29:40
    You are going to have
    some very nice domain.
  • 29:40 - 29:42
    All right.
  • 29:42 - 29:43
    That's it, guys.
  • 29:43 - 29:45
    That's what the exam will say.
  • 29:45 - 29:48
    I'm asking you for a few things.
  • 29:48 - 29:52
    First of all, you are already
    prepared, I guarantee it.
  • 29:52 - 29:55
    Do not stay up late at night.
  • 29:55 - 29:58
    The biggest mistake
    students make
  • 29:58 - 30:02
    is staying up the night before a
    midterm or a final because they
  • 30:02 - 30:04
    want to study everything.
  • 30:04 - 30:06
    That's bad.
  • 30:06 - 30:10
    The next day you will be tired
    and you won't perform as well.
  • 30:10 - 30:16
    Second of all, do not
    be nervous at all.
  • 30:16 - 30:17
    You have no reason
    to be nervous.
  • 30:17 - 30:19
    You have plenty of time.
  • 30:19 - 30:24
    You have plenty of
    things to write down.
  • 30:24 - 30:29
    OK, about the way I grade.
  • 30:29 - 30:31
    If you leave the problem
    completely blank,
  • 30:31 - 30:33
    yes, that's a zero.
  • 30:33 - 30:39
    But if you provide me with at
    least a hint, a formula that
  • 30:39 - 30:42
    serves you-- not just
    an arbitrary formula
  • 30:42 - 30:43
    that has nothing to do with it.
  • 30:43 - 30:46
    But a formula that's
    in the regulation,
  • 30:46 - 30:50
    I give you partial
    credit for everything.
  • 30:50 - 30:53
    So you have no
    reason to freak out.
  • 30:53 - 30:57
    Even if you mess up, let's
    say, one or two problems,
  • 30:57 - 31:01
    your algebra at the
    end, you should still
  • 31:01 - 31:04
    gather together lots of credit.
  • 31:04 - 31:12
    I wrote the exam especially
    because I, myself,
  • 31:12 - 31:15
    hate some medical
    answers from web work.
  • 31:15 - 31:18
    I made the answers to
    be fat and sassy, not
  • 31:18 - 31:21
    like the ones in the web works.
  • 31:21 - 31:25
    So something that you
    can do even mentally,
  • 31:25 - 31:29
    not have to struggle
    with the answer.
  • 31:29 - 31:31
    Several people have
    asked me to go over
  • 31:31 - 31:39
    the last two problems of the
    homework, and I'll go forward.
  • 31:39 - 31:41
    I'll give you an example
    of a problem that bothered
  • 31:41 - 31:45
    a few bothered a few people.
  • 31:45 - 31:52
    And it's somewhat interesting
    because, of course,
  • 31:52 - 31:58
    I make the algebra
    easier than it is.
  • 31:58 - 32:01
    You have 2, 3, 7,
    9, I don't know.
  • 32:01 - 32:07
    You have a function x and y that
    are both functions of u and v.
  • 32:07 - 32:11
    And instead of asking you
    for the determinant-- well,
  • 32:11 - 32:15
    one of them may have asked
    you for the determinant,
  • 32:15 - 32:19
    the functions x, derivative
    of x, y with [INAUDIBLE] u,
  • 32:19 - 32:20
    v as Jacobian.
  • 32:20 - 32:25
    But the other one was asking
    you for just the opposite.
  • 32:25 - 32:27
    Well, several people
    didn't see that.
  • 32:27 - 32:31
    And they kept asking me, so
    I answered some 20 questions
  • 32:31 - 32:34
    during the weekend exactly
    about problems like that.
  • 32:34 - 32:36
    Which doesn't bother me.
  • 32:36 - 32:40
    I think I would have had
    the same problem when
  • 32:40 - 32:42
    I was like you.
  • 32:42 - 32:45
    The easy part on
    the first Jacobian
  • 32:45 - 32:50
    is that you have 1, 1, 1
    minus 1, whatever that is.
  • 32:50 - 32:54
    The definition is
    x sub u, x sub v,
  • 32:54 - 32:58
    y sub u, y sub v. These
    are the partial derivatives
  • 32:58 - 33:00
    and that's called Jacobian.
  • 33:00 - 33:06
    And what you have, you
    have an easy answer.
  • 33:06 - 33:09
    In this case, you have
    the answer negative 2.
  • 33:09 - 33:16
    And if you, however, are asked
    by the author of the problem,
  • 33:16 - 33:18
    whoever created the
    problem of this.
  • 33:18 - 33:20
    And you put negative
    2, it's going
  • 33:20 - 33:22
    to say no, this is not correct.
  • 33:22 - 33:24
    And this is what happened
    to several people.
  • 33:24 - 33:27
    Now, there are two
    ways around it.
  • 33:27 - 33:31
    There are two ways
    you can solve that.
  • 33:31 - 33:34
    STUDENT: On the work, it
    says the reverse [INAUDIBLE].
  • 33:34 - 33:37
    That Jacobian times the
    reverse Jacobian [INAUDIBLE].
  • 33:37 - 33:41
  • 33:41 - 33:46
    PROFESSOR: I want
    to say why that is.
  • 33:46 - 33:49
    For a student who doesn't know
    why this Jacobian is exactly
  • 33:49 - 33:54
    j inverse, there are still
    chances the student can say,
  • 33:54 - 33:57
    well, here's how smart I am.
  • 33:57 - 34:01
    I'm going to say u out, v
    out in terms of x and y.
  • 34:01 - 34:04
    I inverse the
    functions because they
  • 34:04 - 34:07
    are linear functions
    [INAUDIBLE] linear system.
  • 34:07 - 34:09
    So I say x plus y.
  • 34:09 - 34:12
    This is elimination called--
    when we were little,
  • 34:12 - 34:16
    this was called elimination 2u.
  • 34:16 - 34:22
    x minus y equals 2v.
  • 34:22 - 34:28
    So u is x plus y over 2.
  • 34:28 - 34:30
    That means 1/2 x, 1/2 y.
  • 34:30 - 34:31
    Right, guys?
  • 34:31 - 34:31
    I'm right?
  • 34:31 - 34:32
    STUDENT: Mm-hmm.
  • 34:32 - 34:33
    PROFESSOR: OK.
  • 34:33 - 34:38
    And 1/2 of x and minus 1/2 of y.
  • 34:38 - 34:40
    And then, what does
    the student say?
  • 34:40 - 34:43
    I know what I'm going to do.
  • 34:43 - 34:48
    Just by the same definition,
    I say the du, v dx,
  • 34:48 - 34:51
    y as I have an inverse function.
  • 34:51 - 34:54
    And I knew how to
    invert the system.
  • 34:54 - 34:56
    I get 1/2.
  • 34:56 - 35:00
    Not matrix, Magdalena,
    now, determinant.
  • 35:00 - 35:04
    1/2, 1/2 and 1/2, minus 1/2.
  • 35:04 - 35:07
  • 35:07 - 35:09
    And guess what?
  • 35:09 - 35:10
    What do I get?
  • 35:10 - 35:15
    Exactly what it was saying,
    but I did it the long way.
  • 35:15 - 35:21
    I got minus 1 over 4 minus 1
    over 4, which is minus 1/2.
  • 35:21 - 35:22
    Which is--
  • 35:22 - 35:22
    STUDENT: Inverse.
  • 35:22 - 35:24
    PROFESSOR: The inverse of that.
  • 35:24 - 35:27
  • 35:27 - 35:33
    And you are going to ask me,
    OK, I don't understand why.
  • 35:33 - 35:36
    That's why I want to
    tell you a story that I
  • 35:36 - 35:37
    think is beautiful.
  • 35:37 - 35:41
    The book doesn't start like
    that, because the book doesn't
  • 35:41 - 35:45
    necessarily have enough
    space to remind you
  • 35:45 - 35:50
    everything you learned in
    Calc 1 when you are in Calc 3.
  • 35:50 - 35:55
    But if you think of what you
    learned in Calc 1, in Calc 1
  • 35:55 - 35:58
    your professor-- I'm sure that
    he or she showed you this.
  • 35:58 - 36:02
    If you have a function
    y equals f of x,
  • 36:02 - 36:06
    assume this is a c1 function
    and everything is nice.
  • 36:06 - 36:14
    And then you have that
    f prime of x exists
  • 36:14 - 36:15
    and it's continuous everywhere.
  • 36:15 - 36:18
    That's what it means c1.
  • 36:18 - 36:21
    And you want to
    invert this function.
  • 36:21 - 36:25
    You want to invert this
    function around the point x0.
  • 36:25 - 36:38
    So you know that at
    least for some interval
  • 36:38 - 36:41
    that f is one-to-one.
  • 36:41 - 36:42
    So it's invertible.
  • 36:42 - 36:49
  • 36:49 - 36:54
    What is the derivative
    of [INAUDIBLE]?
  • 36:54 - 36:56
  • 36:56 - 37:00
    Somebody asks you, so what
    is the-- the derivative
  • 37:00 - 37:02
    of the inverse
    function is a function
  • 37:02 - 37:06
    of x with respect to x.
  • 37:06 - 37:09
    [INAUDIBLE]?
  • 37:09 - 37:10
    I don't know.
  • 37:10 - 37:16
  • 37:16 - 37:18
    Remind yourself
    how you did that.
  • 37:18 - 37:19
    Was this hard?
  • 37:19 - 37:23
  • 37:23 - 37:31
    Anybody remembers the formula
    for the inverse function?
  • 37:31 - 37:32
    STUDENT: [INAUDIBLE].
  • 37:32 - 37:35
    PROFESSOR: 1 over f prime of x.
  • 37:35 - 37:39
  • 37:39 - 37:42
    So assume that you do
    that at the next 0,
  • 37:42 - 37:46
    assume that f prime of
    x0 is different from 0.
  • 37:46 - 37:49
    Now, how would you
    prove that and how--
  • 37:49 - 37:52
    well, too much memorization.
  • 37:52 - 38:03
    This is what we are doing
    in-- the derivative of e
  • 38:03 - 38:07
    to the x was what?
  • 38:07 - 38:10
    What was the derivative
    of natural log of this?
  • 38:10 - 38:12
    STUDENT: [INAUDIBLE].
  • 38:12 - 38:12
    PROFESSOR: 1/x.
  • 38:12 - 38:15
  • 38:15 - 38:19
    Now, when you have an
    arbitrary function f
  • 38:19 - 38:24
    and you compose with inverse,
    what is it by definition?
  • 38:24 - 38:25
    X equals x.
  • 38:25 - 38:27
    So this is the
    identity function.
  • 38:27 - 38:32
  • 38:32 - 38:35
    Chain rule tells
    you, wait a minute.
  • 38:35 - 38:41
    Chain rule tell you how
    to prime the whole thing.
  • 38:41 - 38:46
    So I prime-- what
    is this animal?
  • 38:46 - 38:50
    F of f inverse of x is the
    composition of functions,
  • 38:50 - 38:50
    right?
  • 38:50 - 38:56
    So apply chain rule to f of
    f inverse of x, all prime,
  • 38:56 - 38:58
    with respect to x.
  • 38:58 - 39:01
    What is x prime
    with respect to x?
  • 39:01 - 39:03
    x prime with respect to x is 1.
  • 39:03 - 39:05
    All right.
  • 39:05 - 39:06
    Chain rule.
  • 39:06 - 39:07
    What does the chain rule say?
  • 39:07 - 39:11
    Chain rule says f
    prime of f inverse
  • 39:11 - 39:17
    of x times a function on
    the outside prime first.
  • 39:17 - 39:21
    We go from the outside to the
    inside one step at a time.
  • 39:21 - 39:24
    Derivative of the guy--
    you cover f with your hand.
  • 39:24 - 39:27
    Derivative of the guy inside,
    the core function inside,
  • 39:27 - 39:33
    that will simply be f inverse
    of x prime with respect to x
  • 39:33 - 39:35
    equals 1.
  • 39:35 - 39:37
    That was x prime.
  • 39:37 - 39:42
    So the derivative of the
    inverse function-- all right.
  • 39:42 - 39:52
    f inverse prime is 1 over
    f prime of f inverse of x.
  • 39:52 - 39:56
  • 39:56 - 40:00
    So if you think of
    this being the y,
  • 40:00 - 40:09
    you have f inverse prime at
    y equals 1 over-- well, yeah.
  • 40:09 - 40:16
    If you put it at x, it's
    f prime of f inverse of x.
  • 40:16 - 40:20
    Because the f
    inverse-- this is x.
  • 40:20 - 40:22
    This is f of x.
  • 40:22 - 40:25
    This is the y [INAUDIBLE].
  • 40:25 - 40:29
    When you have f inverse,
    x is the image of y.
  • 40:29 - 40:31
    So f inverse has an input.
  • 40:31 - 40:33
  • 40:33 - 40:35
    How is this called?
  • 40:35 - 40:37
    In the domain of f inverse.
  • 40:37 - 40:40
    That means, who is
    in the domain of f?
  • 40:40 - 40:41
    f inverse of x.
  • 40:41 - 40:43
    So one is x, one is y.
  • 40:43 - 40:47
  • 40:47 - 40:52
    So keep that in mind that when
    you have to invert a function,
  • 40:52 - 40:53
    what do you do?
  • 40:53 - 41:02
    You say 1 over the
    derivative of the initial--
  • 41:02 - 41:06
    so the derivative of
    the inverse function
  • 41:06 - 41:10
    is 1 over derivative
    of our initial function
  • 41:10 - 41:14
    at the corresponding point.
  • 41:14 - 41:19
    This is how you did the
    derivative for the Calc 1
  • 41:19 - 41:21
    people.
  • 41:21 - 41:22
    All right.
  • 41:22 - 41:34
  • 41:34 - 41:38
    So how do I apply that formula?
  • 41:38 - 41:41
    Well, I have two functions here.
  • 41:41 - 41:49
    One is e to the x and
    one is natural log of x.
  • 41:49 - 41:51
    How do I know they are
    inverse to one another?
  • 41:51 - 41:55
    Their graphs should be
    symmetric with respect to the?
  • 41:55 - 41:56
    STUDENT: y equals x.
  • 41:56 - 41:59
    PROFESSOR: With respect
    to the first [INAUDIBLE].
  • 41:59 - 42:03
  • 42:03 - 42:09
    Assume that f of
    x is e to the x.
  • 42:09 - 42:11
    OK.
  • 42:11 - 42:19
    f inverse of-- well,
    let's say f inverse of y.
  • 42:19 - 42:23
    That would be natural
    log of y, right?
  • 42:23 - 42:29
  • 42:29 - 42:35
    So what if you put
    here, what is f inverse?
  • 42:35 - 42:38
  • 42:38 - 42:40
    Natural log.
  • 42:40 - 42:44
    Let's say a simple way to
    write this, simple division.
  • 42:44 - 42:48
  • 42:48 - 42:52
    According to that formula,
    how would you do the math?
  • 42:52 - 43:02
    You go f inverse prime of x must
    be 1 over the derivative of f
  • 43:02 - 43:07
    with respect of f inverse x.
  • 43:07 - 43:10
    So you go, wait a minute.
  • 43:10 - 43:12
    OK, who is f inverse of x?
  • 43:12 - 43:21
  • 43:21 - 43:25
    Sorry, if f of x is e to the
    x, who is f inverse of x?
  • 43:25 - 43:32
  • 43:32 - 43:34
    You want me to change a letter?
  • 43:34 - 43:36
    I can put a y here.
  • 43:36 - 43:39
    But in any case, I want to
    convince you that this is 1/x.
  • 43:39 - 43:42
  • 43:42 - 43:44
    Why?
  • 43:44 - 43:47
    Because f prime is e to the x.
  • 43:47 - 43:53
    This is going to be e
    to the f inverse of x,
  • 43:53 - 43:58
    which is e to the natural
    log of x, which is x.
  • 43:58 - 44:01
    That's why I have x here.
  • 44:01 - 44:05
    So again, if f of x
    equals e to the x, then f
  • 44:05 - 44:11
    inverse of x is the
    national log of x.
  • 44:11 - 44:13
    By this formula,
    you know that you
  • 44:13 - 44:19
    have to compute natural
    log-- this is f inverse.
  • 44:19 - 44:23
    Natural log of x prime, right?
  • 44:23 - 44:25
    What is this by that formula?
  • 44:25 - 44:31
    1 over the derivative of f prime
    computed at f inverse of x.
  • 44:31 - 44:34
    Now, who is f inverse of x?
  • 44:34 - 44:35
    f inverse of x is
    natural log of x.
  • 44:35 - 44:37
    So again, let me write.
  • 44:37 - 44:41
    All this guy here in the orange
    thing, this [INAUDIBLE] f
  • 44:41 - 44:45
    inverse of x is ln x.
  • 44:45 - 44:48
    Who is f prime?
  • 44:48 - 44:51
    f prime of x is e to the x.
  • 44:51 - 44:53
    So f prime of
    natural log of x will
  • 44:53 - 44:56
    be e to the natural log of x.
  • 44:56 - 45:00
    Applied to natural
    log of x, which is x.
  • 45:00 - 45:03
    So you got it.
  • 45:03 - 45:04
    All right?
  • 45:04 - 45:10
    So remember, this formula,
    professors actually avoid.
  • 45:10 - 45:11
    They say, oh my god.
  • 45:11 - 45:14
    My students will never
    understand this composition
  • 45:14 - 45:16
    thing, derivative.
  • 45:16 - 45:17
    So Magdalena, I don't care.
  • 45:17 - 45:19
    You are the
    undergraduate director.
  • 45:19 - 45:21
    I'll never give it like that.
  • 45:21 - 45:23
    That's a mistake.
  • 45:23 - 45:26
    They should show it
    to you like that.
  • 45:26 - 45:31
    f inverse prime of x equals
    1 over f prime of what?
  • 45:31 - 45:34
    Of the inverse image of x.
  • 45:34 - 45:38
    Because you act on x.
  • 45:38 - 45:44
    So if x is acting on--
    this is f of x, then
  • 45:44 - 45:47
    you have to invert by
    acting on f of x, like this
  • 45:47 - 45:49
    and like that.
  • 45:49 - 45:55
    If x is in the domain of f
    inverse, that means what?
  • 45:55 - 46:01
    That in the domain of f, you
    have f inverse of x as input.
  • 46:01 - 46:04
    So instead of giving
    you the formula,
  • 46:04 - 46:08
    they just make you
    memorize the formulas
  • 46:08 - 46:12
    for the inverse functions,
    like-- believe me,
  • 46:12 - 46:16
    you take e to the x
    [INAUDIBLE] derivative.
  • 46:16 - 46:20
    You take natural log,
    it's 1/x derivative.
  • 46:20 - 46:24
    Don't worry about the fact that
    they are inverse to one another
  • 46:24 - 46:27
    and you an relate the
    derivatives of two
  • 46:27 - 46:28
    inverse functions.
  • 46:28 - 46:33
    They try to stay out of trouble
    because this is hard to follow.
  • 46:33 - 46:36
    You could see that you had
    [INAUDIBLE] a little bit
  • 46:36 - 46:37
    and concentrate.
  • 46:37 - 46:39
    What is this woman saying?
  • 46:39 - 46:42
    This looks hard.
  • 46:42 - 46:46
    But it's the same process
    that happens in the Jacobian.
  • 46:46 - 46:53
    So in the Jacobian of a
    function of two variables.
  • 46:53 - 46:57
  • 46:57 - 47:05
    Now, remember the signed
    area that I told you about.
  • 47:05 - 47:09
    Signed area notion.
  • 47:09 - 47:10
    What did we say?
  • 47:10 - 47:14
    We said that dA is
    dx dy, but it's not
  • 47:14 - 47:17
    the way they explain in
    the book because it's
  • 47:17 - 47:21
    more like a wedge thing.
  • 47:21 - 47:26
    And that wedge thingy had
    a meaning in the sense
  • 47:26 - 47:31
    that if you were to not take
    the exterior derivative dx dy,
  • 47:31 - 47:36
    but take dy wedge dx,
    it would change sign.
  • 47:36 - 47:38
    So we thought of
    signed area before.
  • 47:38 - 47:42
    When we did dx wedge
    dy, what did we
  • 47:42 - 47:45
    get in terms of Jacobian?
  • 47:45 - 47:49
    We get j d r
    [INAUDIBLE] coordinates.
  • 47:49 - 47:53
    Do you remember what this j was?
  • 47:53 - 47:54
    STUDENT: r.
  • 47:54 - 47:56
    PROFESSOR: Very good, r.
  • 47:56 - 48:01
    In the case, in the simple
    case of Cartesian versus polar,
  • 48:01 - 48:07
    Cartesian going to polar,
    you have a function f.
  • 48:07 - 48:10
    Coming back it's called
    the inverse function.
  • 48:10 - 48:15
    So I'm asking, this is the
    Jacobian of which function?
  • 48:15 - 48:18
    This is the Jacobian of
    the function that goes
  • 48:18 - 48:20
    from [INAUDIBLE] theta to x, y.
  • 48:20 - 48:23
    If I want the Jacobian
    of the function that
  • 48:23 - 48:25
    goes from x, y into
    [INAUDIBLE] theta,
  • 48:25 - 48:30
    I should write--
    well, d r d theta
  • 48:30 - 48:34
    will be something times dx dy.
  • 48:34 - 48:37
    And now you understand
    better what's going on.
  • 48:37 - 48:39
    1/j.
  • 48:39 - 48:40
    1/j.
  • 48:40 - 48:43
    So Matthew was
    right, in the sense
  • 48:43 - 48:48
    that he said why are you so
    clumsy and go ahead and compute
  • 48:48 - 48:50
    again u, v?
  • 48:50 - 48:52
    Express u, v in terms of x, y.
  • 48:52 - 48:55
    You waste your time
    and get minus a 1/2.
  • 48:55 - 48:56
    What was that, guys?
  • 48:56 - 48:57
    Minus 1/2.
  • 48:57 - 49:02
    When I'm telling you that
    for the inverse mapping,
  • 49:02 - 49:05
    the Jacobian you get is
    the inverse of a Jacobian.
  • 49:05 - 49:07
    It's very simple.
  • 49:07 - 49:09
    It's a very simple relationship.
  • 49:09 - 49:11
    I could observe that.
  • 49:11 - 49:12
    And he was right.
  • 49:12 - 49:19
    So keep in mind that when you
    have Jacobian of the map where
  • 49:19 - 49:25
    x, y are functions of u, v,
    this is 1 over the Jacobian
  • 49:25 - 49:30
    where you have u, v
    as functions of x, y.
  • 49:30 - 49:33
    So you have inverse mapping.
  • 49:33 - 49:36
    In Advanced Calculus, you
    may learn a little bit more
  • 49:36 - 49:38
    about the inverse
    mapping theorem.
  • 49:38 - 49:41
    This is what I'm talking about.
  • 49:41 - 49:42
    For the inverse
    mapping theorem, you
  • 49:42 - 49:48
    go, well, if the derivative
    of these two with respect
  • 49:48 - 49:50
    to these two are done as
    j Jacobian, the derivative
  • 49:50 - 49:54
    of these two with
    respect to these two
  • 49:54 - 49:59
    in a Jacobian [INAUDIBLE]
    exactly j inverse, or 1/j.
  • 49:59 - 50:02
    j is a real number.
  • 50:02 - 50:06
    So for a real number, whether
    I write 1/j or j inverse,
  • 50:06 - 50:09
    it's the same.
  • 50:09 - 50:12
    So as an application, do
    you have to know all this?
  • 50:12 - 50:14
    No, you don't.
  • 50:14 - 50:21
    But as an application, let
    me ask you the following.
  • 50:21 - 50:34
  • 50:34 - 50:38
    Something harder than
    [INAUDIBLE] in the book.
  • 50:38 - 50:41
    In the book, you have
    simple transformations.
  • 50:41 - 50:46
    What is the Jacobian
    of r theta-- theta, phi
  • 50:46 - 50:46
    or phi, theta.
  • 50:46 - 50:47
    It doesn't matter.
  • 50:47 - 50:50
    If I swap the two, I
    still have the same thing.
  • 50:50 - 50:54
  • 50:54 - 50:57
    If a determinant swaps
    two rows or two columns,
  • 50:57 - 51:00
    do you guys know what happens?
  • 51:00 - 51:02
    You took linear algebra.
  • 51:02 - 51:03
    STUDENT: Swap.
  • 51:03 - 51:05
    PROFESSOR: You swap two
    rows or two columns.
  • 51:05 - 51:06
    STUDENT: [INAUDIBLE].
  • 51:06 - 51:08
    PROFESSOR: It's going to pick
    up a minus sign, very good.
  • 51:08 - 51:10
    But only three people in
    this class figured it out.
  • 51:10 - 51:13
  • 51:13 - 51:14
    How shall I denote?
  • 51:14 - 51:17
    Not j, but the notation
    was [INAUDIBLE].
  • 51:17 - 51:20
    And this is j.
  • 51:20 - 51:24
    So [INAUDIBLE] phi theta
    over [INAUDIBLE] x, y, z.
  • 51:24 - 51:26
    How do you compute them?
  • 51:26 - 51:29
    You say, no, I'm not
    going to compute it
  • 51:29 - 51:33
    by hand because until tomorrow
    I'm not going to finish it.
  • 51:33 - 51:35
    STUDENT: Does that
    need a 3 by 3 matrix?
  • 51:35 - 51:37
    PROFESSOR: It's a determinant.
  • 51:37 - 51:40
    So when you were to
    write this, you're
  • 51:40 - 51:46
    not going to do it because it's
    a killer for somebody to work
  • 51:46 - 51:49
    like that in spherical
    coordinates with only
  • 51:49 - 51:51
    those inverse functions.
  • 51:51 - 51:57
    Do you remember as a review
    what spherical coordinates were?
  • 51:57 - 52:01
    x, y, z versus r, theta, phi.
  • 52:01 - 52:02
    We reviewed that.
  • 52:02 - 52:03
    Theta was the longitude.
  • 52:03 - 52:06
    Phi was the latitude
    from the North Pole.
  • 52:06 - 52:08
    So x was-- who remembers that?
  • 52:08 - 52:09
    [INTERPOSING VOICES]
  • 52:09 - 52:14
  • 52:14 - 52:19
    PROFESSOR: Cosine theta
    r sine phi sine theta.
  • 52:19 - 52:21
    And z was the adjacent guy.
  • 52:21 - 52:24
    Remember, this was the thingy?
  • 52:24 - 52:27
    And this was the phi.
  • 52:27 - 52:32
    And to express x, the
    phi was adjacent to it.
  • 52:32 - 52:33
    And that's why you
    have cosine phi.
  • 52:33 - 52:36
  • 52:36 - 52:41
    It's a killer if somebody wants
    to pull out the r, phi, theta.
  • 52:41 - 52:43
    First of all, r will be easy.
  • 52:43 - 52:46
    But the other ones are a
    little bit of a headache.
  • 52:46 - 52:48
    And with all those
    big functions,
  • 52:48 - 52:51
    you would waste a lot of time
    to compute the determinant.
  • 52:51 - 52:52
    What do you do?
  • 52:52 - 52:55
    You say, well, didn't
    you say that if I
  • 52:55 - 52:58
    take the inverse mapping,
    the Jacobian would be
  • 52:58 - 53:01
    1 over the original Jacobian?
  • 53:01 - 53:04
    Yes, I just said that.
  • 53:04 - 53:09
    So go ahead and remember what
    the original Jacobian was
  • 53:09 - 53:13
    and leave us alone
    you're going to say.
  • 53:13 - 53:16
    And you're right.
  • 53:16 - 53:22
    What was that I just said
    the other Jacobian was?
  • 53:22 - 53:23
    STUDENT: [INAUDIBLE].
  • 53:23 - 53:25
    PROFESSOR: You told me.
  • 53:25 - 53:27
    I forgot it already.
  • 53:27 - 53:29
    r squared sine phi, right?
  • 53:29 - 53:33
    So if somebody's asking
    you to solve this problem,
  • 53:33 - 53:37
    you don't need to
    write out anything.
  • 53:37 - 53:38
    Just 1 over [INAUDIBLE].
  • 53:38 - 53:40
    I'm done.
  • 53:40 - 53:42
    But I'm not going to ask you.
  • 53:42 - 53:45
    Of course, I saw
    this problem exactly.
  • 53:45 - 53:48
    Find the Jacobian of
    the inverse mapping
  • 53:48 - 53:50
    for the spherical coordinates.
  • 53:50 - 53:54
    That was given at Princeton
    in Advanced Calculus.
  • 53:54 - 53:59
    There were three variables, and
    then there was a generalization
  • 53:59 - 54:01
    to [INAUDIBLE] variables.
  • 54:01 - 54:03
    But based on this
    at Princeton, I'm
  • 54:03 - 54:04
    not going to give you
    anything like that
  • 54:04 - 54:05
    to compute in the exam.
  • 54:05 - 54:08
  • 54:08 - 54:12
    And I just expect that you
    know your basics about how
  • 54:12 - 54:16
    to compute triple integrals.
  • 54:16 - 54:20
    Use the Jacobians and
    be successful with it.
  • 54:20 - 54:25
  • 54:25 - 54:29
    Let's do one last
    problem about the review.
  • 54:29 - 54:30
    Although, it's not
    in the midterm,
  • 54:30 - 54:37
    but I would like to-- I'd
    like to see how you solve it.
  • 54:37 - 55:01
  • 55:01 - 55:06
    A student from another
    class, Calc 3, came to me.
  • 55:06 - 55:10
    And I was hesitant about even
    helping him on the homework
  • 55:10 - 55:16
    because we're not supposed
    to help our college students.
  • 55:16 - 55:19
    So I told him, did you go
    to the tutoring center?
  • 55:19 - 55:22
    And he said yes, but they
    couldn't help him much.
  • 55:22 - 55:24
    So I said, OK.
  • 55:24 - 55:27
    So let me see the problem.
  • 55:27 - 55:29
    He showed me the
    problem and I wanted
  • 55:29 - 55:33
    to talk about this
    problem with you.
  • 55:33 - 55:37
    This is not a hard problem, OK?
  • 55:37 - 55:42
    You just have to see
    what this is about.
  • 55:42 - 55:43
    Understand what this is about.
  • 55:43 - 55:50
  • 55:50 - 55:56
    So you have the z equals x
    squared plus y squared, which
  • 55:56 - 56:00
    is the [INAUDIBLE].
  • 56:00 - 56:01
    Sorry about my typos.
  • 56:01 - 56:08
  • 56:08 - 56:11
    We didn't write this
    problem in the book.
  • 56:11 - 56:16
    So I suspect that his instructor
    came up with this problem.
  • 56:16 - 56:20
    This is a cone.
  • 56:20 - 56:21
    We only look at
    the upper halves.
  • 56:21 - 56:24
  • 56:24 - 56:26
    Do these surfaces intersect?
  • 56:26 - 56:34
  • 56:34 - 56:43
    Draw the body between
    them if the case.
  • 56:43 - 56:49
  • 56:49 - 56:51
    And compute the
    volume of that body.
  • 56:51 - 57:02
  • 57:02 - 57:03
    And what do you think
    my reaction was?
  • 57:03 - 57:05
    Oh, this is a piece of cake.
  • 57:05 - 57:07
    And it is a piece of cake.
  • 57:07 - 57:11
    But you need to
    learn Calc 3 first
  • 57:11 - 57:15
    in order to help other
    people do Calc 3 problems.
  • 57:15 - 57:17
    Especially if they
    are not in the book.
  • 57:17 - 57:22
    So one has to have a very good
    understanding of the theory
  • 57:22 - 57:26
    and of geometry, analytic
    geometry, and conics
  • 57:26 - 57:32
    before they move onto
    triple integrals and so on.
  • 57:32 - 57:36
    Can you imagine these with
    the eyes of your imagination?
  • 57:36 - 57:38
    Can we draw them?
  • 57:38 - 57:39
    Yeah.
  • 57:39 - 57:43
    We better draw them because
    they are not nasty to draw.
  • 57:43 - 57:47
    Of course this looks
    like the Tower of Pisa.
  • 57:47 - 57:50
    Let me do it again.
  • 57:50 - 57:50
    Better.
  • 57:50 - 57:53
    x, y, and z.
  • 57:53 - 57:56
    And then I'll take the cone.
  • 57:56 - 58:02
    Well, let me draw
    the paraboloid first.
  • 58:02 - 58:04
    Kind of sort of.
  • 58:04 - 58:07
    And then the cone.
  • 58:07 - 58:10
    I hate myself when
    I cannot draw.
  • 58:10 - 58:14
  • 58:14 - 58:20
    If you were to cut, slice
    up, it could be this.
  • 58:20 - 58:25
    And who asked me last
    time, was it Alex, or Ryan,
  • 58:25 - 58:30
    or maybe somebody else, who
    said maybe we could do that even
  • 58:30 - 58:31
    in Calc 2 by--
  • 58:31 - 58:32
    STUDENT: Yeah.
  • 58:32 - 58:32
    PROFESSOR: You asked me.
  • 58:32 - 58:33
    STUDENT: [INAUDIBLE].
  • 58:33 - 58:35
    PROFESSOR: If you
    take a leaf like that
  • 58:35 - 58:37
    and you rotate it
    around the body,
  • 58:37 - 58:41
    like in-- using one
    of the two methods
  • 58:41 - 58:44
    that you learned in Calc 2.
  • 58:44 - 58:46
    Well, we can do that.
  • 58:46 - 58:49
    But you see we have in Calc 3.
  • 58:49 - 58:53
    So I would like to
    write that in terms
  • 58:53 - 58:59
    of the volume of the body
    faster with knowledge I have.
  • 58:59 - 58:59
    Do they intersect?
  • 58:59 - 59:01
    And where do they intersect?
  • 59:01 - 59:03
    And how do I find this out?
  • 59:03 - 59:04
    STUDENT: [INAUDIBLE].
  • 59:04 - 59:06
    PROFESSOR: Yes.
  • 59:06 - 59:17
    I have to make them equal and
    solve for z, and then the rest.
  • 59:17 - 59:19
    How do I solve for z?
  • 59:19 - 59:24
    Well, z equals z0 gives
    me two possibilities.
  • 59:24 - 59:28
    One is z equals 0
    and 1 is z equals 1
  • 59:28 - 59:34
    because this is the same as
    writing z times z minus 1
  • 59:34 - 59:35
    equals 0.
  • 59:35 - 59:36
    So where do they intersect?
  • 59:36 - 59:38
    They intersect
    here at the origin
  • 59:38 - 59:42
    and they intersect
    where z equals 1.
  • 59:42 - 59:47
    And where z equals 1, I'm
    going to have what circle?
  • 59:47 - 59:49
    The unit circle.
  • 59:49 - 59:53
    I'll draw over--
    I'll make it in red.
  • 59:53 - 59:58
    This is x squared plus y squared
    equals 1 at the altitude 1,
  • 59:58 - 60:00
    z equals 1.
  • 60:00 - 60:02
    This is the plane z equals 1.
  • 60:02 - 60:08
  • 60:08 - 60:15
    OK, so how many ways
    to do this are there?
  • 60:15 - 60:22
    When we were in Chapter 12,
    we said the triple integral
  • 60:22 - 60:24
    will give me the volume.
  • 60:24 - 60:26
    So the volume will
    be triple integral
  • 60:26 - 60:31
    of a certain body-- of
    1 over a certain body
  • 60:31 - 60:41
    dv, where the body is
    the body of revolution
  • 60:41 - 60:50
    created by the motion
    of-- what is this thing?
  • 60:50 - 60:51
    What shall we call it?
  • 60:51 - 60:53
    A wing.
  • 60:53 - 60:54
    [INAUDIBLE]
  • 60:54 - 60:57
  • 60:57 - 61:03
    Domain D. No, domain D is
    usually what's on [INAUDIBLE].
  • 61:03 - 61:09
  • 61:09 - 61:10
    I don't know.
  • 61:10 - 61:14
    STUDENT: L for leaf?
  • 61:14 - 61:15
    PROFESSOR: L for leaf.
  • 61:15 - 61:15
    Wonderful.
  • 61:15 - 61:16
    I like that.
  • 61:16 - 61:21
    L. OK.
  • 61:21 - 61:27
    So I can write it up as
    a triple integral how?
  • 61:27 - 61:30
    Is it easy to use it in
    spherical coordinates?
  • 61:30 - 61:30
    No.
  • 61:30 - 61:33
    That's not a spherical
    coordinate problem.
  • 61:33 - 61:35
    That's a cylindrical
    coordinate problem.
  • 61:35 - 61:36
    Why is that?
  • 61:36 - 61:39
    I'm going to have to
    think where I live.
  • 61:39 - 61:45
    I live above a beautiful disk,
    which is the shadowy plane.
  • 61:45 - 61:48
    And that beautiful disk
    has exactly radius 1.
  • 61:48 - 61:49
    So we are lucky.
  • 61:49 - 61:53
    That's the unit disk, x squared
    plus y squared less than 1
  • 61:53 - 61:56
    and greater than 0.
  • 61:56 - 62:00
    So when I revolve, I'm
    using polar coordinates.
  • 62:00 - 62:03
    And that means I'm using
    cylindrical coordinates, which
  • 62:03 - 62:05
    is practically the same thing.
  • 62:05 - 62:10
    r will be between what and what?
  • 62:10 - 62:11
    STUDENT: [INAUDIBLE].
  • 62:11 - 62:13
    PROFESSOR: 0 to 1, very good.
  • 62:13 - 62:14
    Theta?
  • 62:14 - 62:15
    STUDENT: [INAUDIBLE].
  • 62:15 - 62:17
    PROFESSOR: 0 to 2 pi.
  • 62:17 - 62:19
    How about z?
  • 62:19 - 62:21
    z is the z from
    cylindrical coordinates.
  • 62:21 - 62:25
    STUDENT: Square root x
    squared plus y squared--
  • 62:25 - 62:27
    PROFESSOR: Who is on the bottom?
  • 62:27 - 62:29
    STUDENT: 0.
  • 62:29 - 62:35
    PROFESSOR: So the z is between--
    let me write it in x first,
  • 62:35 - 62:37
    and then switch to polar.
  • 62:37 - 62:38
    Is that OK?
  • 62:38 - 62:38
    STUDENT: Yeah
  • 62:38 - 62:39
    PROFESSOR: All right.
  • 62:39 - 62:42
    So what do I write on
    the left-hand side?
  • 62:42 - 62:43
    I need water.
  • 62:43 - 62:44
    STUDENT: [INAUDIBLE].
  • 62:44 - 62:51
  • 62:51 - 62:52
    PROFESSOR: Who is smaller?
  • 62:52 - 62:54
    Who is smaller?
  • 62:54 - 62:57
    Square root of x
    squared y squared or x
  • 62:57 - 62:59
    squared plus y squared?
  • 62:59 - 63:01
    STUDENT: Square root over.
  • 63:01 - 63:02
    PROFESSOR: This is smaller.
  • 63:02 - 63:03
    Why?
  • 63:03 - 63:05
    STUDENT: Because [INAUDIBLE].
  • 63:05 - 63:07
    PROFESSOR: So it's less than 1.
  • 63:07 - 63:08
    I mean, less than 1.
  • 63:08 - 63:10
    This is less than 1.
  • 63:10 - 63:11
    It's between 0 and 1.
  • 63:11 - 63:15
  • 63:15 - 63:19
    So I was trying to explain
    this to my son, but I couldn't.
  • 63:19 - 63:20
    But he's 10.
  • 63:20 - 63:22
    It's so hard.
  • 63:22 - 63:33
    So I said compare square
    root of 0.04 with 0.04.
  • 63:33 - 63:35
    This is smaller, obviously.
  • 63:35 - 63:37
    This is 0.2.
  • 63:37 - 63:38
    He can understand.
  • 63:38 - 63:41
  • 63:41 - 63:43
    So this is what we're doing.
  • 63:43 - 63:47
    We are saying that
    this is x squared
  • 63:47 - 63:52
    plus y squared, the round
    thing on the bottom.
  • 63:52 - 64:01
    And this is going to be on the
    top, square root of x squared
  • 64:01 - 64:03
    plus y squared
    from the cylinder,
  • 64:03 - 64:07
    from the cone-- sorry
    guys, the upper half.
  • 64:07 - 64:09
    Because I only work
    with the upper half.
  • 64:09 - 64:12
    Everything is about
    the sea level.
  • 64:12 - 64:15
    Good, now let's write
    out the whole thing.
  • 64:15 - 64:19
    So I have integral from
    the polar coordinates,
  • 64:19 - 64:20
    from what to what?
  • 64:20 - 64:23
  • 64:23 - 64:24
    STUDENT: r squared to r.
  • 64:24 - 64:31
    PROFESSOR: r squared to
    r, 0 to 1, 0 to 2 pi.
  • 64:31 - 64:35
    So the order of integration
    would be dz dr d theta.
  • 64:35 - 64:38
  • 64:38 - 64:40
    And what's inside here?
  • 64:40 - 64:43
    STUDENT: [INAUDIBLE].
  • 64:43 - 64:44
    PROFESSOR: No.
  • 64:44 - 64:44
    STUDENT: r.
  • 64:44 - 64:48
    PROFESSOR: r,
    excellent, r-- why r?
  • 64:48 - 64:50
    Because 1 was 1.
  • 64:50 - 64:59
    But dv is Jacobian times dr
    d theta dz-- dz, dr, d theta.
  • 64:59 - 65:02
    So this is going to be the r
    from the change of coordinates,
  • 65:02 - 65:04
    the Jacobian.
  • 65:04 - 65:05
    Is this hard?
  • 65:05 - 65:06
    Well, let's do it.
  • 65:06 - 65:08
    Come on, this shouldn't be hard.
  • 65:08 - 65:14
    We can even separate
    the functions.
  • 65:14 - 65:20
    And I got you some tricks.
  • 65:20 - 65:22
    The first one we
    have to work it out.
  • 65:22 - 65:23
    We have no other choice.
  • 65:23 - 65:28
    So I'm going to have
    the integral from 0
  • 65:28 - 65:32
    to 2 pi, integral from 0 to 1.
  • 65:32 - 65:33
    And then I go what?
  • 65:33 - 65:40
    I go integral of what you see
    with z, the z between r and r
  • 65:40 - 65:47
    squared times r dr d theta.
  • 65:47 - 65:48
    Who is going on my nerves?
  • 65:48 - 65:50
    Not you guys.
  • 65:50 - 65:54
    Here, there is a guy that
    goes on my nerves-- the theta.
  • 65:54 - 65:57
    I can get rid of him, and I
    say, I don't need the theta.
  • 65:57 - 65:59
    I've got things
    to do with the r.
  • 65:59 - 66:06
    So I go 2 pi, which is the
    integral from 0 to 2 pi of 1
  • 66:06 - 66:07
    d theta.
  • 66:07 - 66:09
    2 pi goes out.
  • 66:09 - 66:15
    Now 2 pi times integral
    from 0 to 1 of what?
  • 66:15 - 66:17
    What's the simplest
    way to write it?
  • 66:17 - 66:20
    STUDENT: [INAUDIBLE].
  • 66:20 - 66:22
    PROFESSOR: r squared in the end.
  • 66:22 - 66:24
    I mean, I do the whole
    thing in the end.
  • 66:24 - 66:31
    I have r squared minus
    r cubed, right guys?
  • 66:31 - 66:33
    Are you with me?
  • 66:33 - 66:36
    dr, so this is when I did it.
  • 66:36 - 66:40
    But I didn't do the
    anti-derivative, not yet.
  • 66:40 - 66:42
    I did not apply the fundamental.
  • 66:42 - 66:47
    Now you apply the
    fundamental [INAUDIBLE]
  • 66:47 - 66:48
    and tell me what you get.
  • 66:48 - 66:51
    What is this?
  • 66:51 - 66:54
    STUDENT: [INAUDIBLE] 1/12.
  • 66:54 - 66:59
    PROFESSOR: 1/12, that's very
    good-- r cubed over 3 minus r
  • 66:59 - 67:05
    to the 4 over 4, 1/3 minus
    1/4, 1/12, very good.
  • 67:05 - 67:09
    So you have 2 pi times
    1/12 equals pi over 6.
  • 67:09 - 67:12
    Thank god, we got it.
  • 67:12 - 67:13
    Was it hard?
  • 67:13 - 67:15
  • 67:15 - 67:18
    Would you have spent two
    days without doing this?
  • 67:18 - 67:22
    I think you would have
    gotten it by yourselves.
  • 67:22 - 67:25
    Am I right, with no problem?
  • 67:25 - 67:26
    Why is that?
  • 67:26 - 67:30
    Because I think you
    worked enough problems
  • 67:30 - 67:33
    to master the material,
    and you are prepared.
  • 67:33 - 67:37
    And this is not a
    surprise for you
  • 67:37 - 67:41
    like it is for many
    students in other classes.
  • 67:41 - 67:42
    Yes, sir.
  • 67:42 - 67:45
    STUDENT: Can you put that
    one in spherical coordinates?
  • 67:45 - 67:46
    PROFESSOR: You can.
  • 67:46 - 67:50
    That is going to be a hassle.
  • 67:50 - 67:55
    I would do one more
    problem that is not
  • 67:55 - 67:57
    quite appropriate
    for spherical work,
  • 67:57 - 68:00
    but I want to do it [INAUDIBLE].
  • 68:00 - 68:03
    Because it looks like the
    ones I gave you as a homework,
  • 68:03 - 68:06
    and several people
    struggled with that.
  • 68:06 - 68:13
    And I want to see how it's done
    since not everybody finished
  • 68:13 - 68:14
    it.
  • 68:14 - 68:17
  • 68:17 - 68:21
    Given [INAUDIBLE] numbers,
    you have a flat plane
  • 68:21 - 68:27
    z equals a at some
    altitude a and a cone
  • 68:27 - 68:29
    exactly like the cone
    I gave you before.
  • 68:29 - 68:33
    And of course this is
    not just like you asked.
  • 68:33 - 68:36
    This is not very appropriate
    for spherical coordinates.
  • 68:36 - 68:39
    It's appropriate
    for cylindrical.
  • 68:39 - 68:42
    But they ask you
    to do it in both.
  • 68:42 - 68:44
    Remember that problem, guys?
  • 68:44 - 68:49
    So you have the volume of, or
    some function, or something.
  • 68:49 - 68:53
    And they say, put it in
    both spherical coordinates
  • 68:53 - 68:57
    and cylindrical coordinates.
  • 68:57 - 68:59
    And let's assume that
    you don't know what
  • 68:59 - 69:01
    function you are integrating.
  • 69:01 - 69:03
    I'm working too
    much with volumes.
  • 69:03 - 69:05
    Let's suppose that
    you are simply
  • 69:05 - 69:10
    integrating in function
    F of x, y, z dV, which
  • 69:10 - 69:17
    is dx dy dx over the body of
    the [INAUDIBLE], of the-- this
  • 69:17 - 69:23
    is the flat cone, the
    flat ice cream cone.
  • 69:23 - 69:28
    Then somebody licked your
    ice cream up to this point.
  • 69:28 - 69:31
    And you are left
    with the ice cream
  • 69:31 - 69:37
    only under this at the level
    of the rim of the waffle.
  • 69:37 - 69:40
  • 69:40 - 69:44
    Let's break this into two-- they
    don't ask you to compute it.
  • 69:44 - 69:51
    They ask you to set up
    cylindrical coordinates
  • 69:51 - 69:55
    and set up the
    spherical coordinates.
  • 69:55 - 69:57
    But thank you for the idea.
  • 69:57 - 69:59
    That was great.
  • 69:59 - 70:02
    So let's see, how hard is it?
  • 70:02 - 70:07
    I think it's very easy in
    cylindrical coordinates.
  • 70:07 - 70:09
    What do you do in
    cylindrical coordinates?
  • 70:09 - 70:10
    You say, well, wait a minute.
  • 70:10 - 70:14
    If z equals a has
    to be intersected
  • 70:14 - 70:18
    with z squared
    equals x squared, I
  • 70:18 - 70:20
    know the circle that
    I'm going to get
  • 70:20 - 70:21
    is going to be a piece of cake.
  • 70:21 - 70:26
    x squared plus y squared
    equals a squared.
  • 70:26 - 70:34
    So really my ice cream
    cone has the radius a.
  • 70:34 - 70:35
    Are you guys with me?
  • 70:35 - 70:36
    Is it true?
  • 70:36 - 70:40
    Is it true that the radius
    of this licked ice cream cone
  • 70:40 - 70:41
    is a?
  • 70:41 - 70:41
    STUDENT: Mhmm.
  • 70:41 - 70:44
    PROFESSOR: It is true.
  • 70:44 - 70:49
    Whatever that a was-- yours
    was 43, 34, 37, god knows what,
  • 70:49 - 70:52
    doesn't matter.
  • 70:52 - 70:58
    I would foresee-- I'm not
    a prophet or even a witch.
  • 70:58 - 70:59
    I am a witch.
  • 70:59 - 71:03
    But anyway, I would
    not foresee somebody
  • 71:03 - 71:05
    giving you a hard
    problem to solve
  • 71:05 - 71:07
    like that computationally.
  • 71:07 - 71:11
    But on the final, they can
    make you set up the limits
  • 71:11 - 71:13
    and leave it like that.
  • 71:13 - 71:17
    So how do we do cylindrical?
  • 71:17 - 71:19
    Is this hard?
  • 71:19 - 71:22
    So r will be from 0 to a.
  • 71:22 - 71:24
    And god, that's easy.
  • 71:24 - 71:27
    0 to 2 pi is going
    to be for the theta.
  • 71:27 - 71:29
    First I write dz.
  • 71:29 - 71:32
    Then I do dr and d theta.
  • 71:32 - 71:36
  • 71:36 - 71:40
    Theta will be between 0 and
    2 pi, r between 0 and a.
  • 71:40 - 71:44
    z-- you guys have to
    tell me, because it's
  • 71:44 - 71:48
    between a bottom and a top.
  • 71:48 - 71:51
    And I was about to
    take this to drink.
  • 71:51 - 71:52
    STUDENT: [INAUDIBLE].
  • 71:52 - 72:02
  • 72:02 - 72:05
    PROFESSOR: r is the
    one on the bottom,
  • 72:05 - 72:09
    and a is the one on the top.
  • 72:09 - 72:11
    And I think that's clear
    to everybody, right?
  • 72:11 - 72:16
    Is there anything
    missing obviously?
  • 72:16 - 72:20
    So what do I do when they
    ask me on the final--
  • 72:20 - 72:23
    when I say this is a
    mysterious function, what
  • 72:23 - 72:24
    do you put in here?
  • 72:24 - 72:29
    F of x, y, z, yes,
    but yes and no.
  • 72:29 - 72:40
    Because you say F of x of r z
    theta, y of r z theta, z of god
  • 72:40 - 72:42
    knows z, z.
  • 72:42 - 72:44
    z is the same, do
    you understand?
  • 72:44 - 72:46
    So you indicate
    to the poor people
  • 72:46 - 72:51
    that I'm not going to stay in
    x, y, z, because I'm not stupid.
  • 72:51 - 72:54
    I'm going to transform
    the whole thing
  • 72:54 - 72:56
    so it's going to be expressed
    in terms of these letters-- r
  • 72:56 - 73:00
    theta and z.
  • 73:00 - 73:02
    Do you have to write all this?
  • 73:02 - 73:05
    If you were a professional
    writing the math paper, yes,
  • 73:05 - 73:09
    you have to, or a math book
    or whatever, you have to.
  • 73:09 - 73:12
    But you can also skip it
    and put the F. I'm not
  • 73:12 - 73:13
    going to take off points.
  • 73:13 - 73:16
    I will understand.
  • 73:16 - 73:19
    Times r-- very good.
  • 73:19 - 73:21
    Never forget about
    your nice Jacobian.
  • 73:21 - 73:26
    If you forget the r, this
    is no good, 0 points,
  • 73:26 - 73:30
    even with all the setup you
    tried to do going into it.
  • 73:30 - 73:34
    OK, finally let's see.
  • 73:34 - 73:38
    How you do this in
    spherical is not-- yes, sir.
  • 73:38 - 73:40
    STUDENT: When you're
    finding the volume,
  • 73:40 - 73:44
    isn't it with a triple integral,
    don't you just put a 1?
  • 73:44 - 73:44
    PROFESSOR: Hm?
  • 73:44 - 73:46
    STUDENT: When you're
    finding a volume?
  • 73:46 - 73:49
    PROFESSOR: No, I didn't
    say-- I just said,
  • 73:49 - 73:51
    but you probably were
    thinking of [INAUDIBLE].
  • 73:51 - 73:54
    I said, I gave you
    too many volumes.
  • 73:54 - 73:57
    I just said, and
    I'm tired of saying
  • 73:57 - 73:59
    volume of this, volume of that.
  • 73:59 - 74:01
    And in the actual
    problem, they may
  • 74:01 - 74:05
    ask you to do triple
    integral of any function,
  • 74:05 - 74:08
    differentiable function
    or continuous function,
  • 74:08 - 74:13
    over a volume, over a body.
  • 74:13 - 74:16
    So this could be-- in
    the next chapter we're
  • 74:16 - 74:17
    going to see some applications.
  • 74:17 - 74:20
  • 74:20 - 74:25
    I maybe saw some in 12.6 like
    mass moment, those things.
  • 74:25 - 74:28
    But in three coordinates,
    you have other functions
  • 74:28 - 74:30
    that are these functions.
  • 74:30 - 74:35
    You'll have that included,
    row z, x, y, z, and so on.
  • 74:35 - 74:37
    OK, good.
  • 74:37 - 74:40
    When you would integrate a
    density function in that case,
  • 74:40 - 74:42
    you will have a mass.
  • 74:42 - 74:45
    Because you integrate this, d
    over volume, you'd have a mass.
  • 74:45 - 74:50
    OK, in this case,
    we have to be smart,
  • 74:50 - 74:56
    say F times r squared
    sine phi is the Jacobian.
  • 74:56 - 75:02
    This is a function in r
    phi and theta, right guys?
  • 75:02 - 75:04
    We don't care what it is.
  • 75:04 - 75:06
    We are going to have
    the d something,
  • 75:06 - 75:07
    d something, d something.
  • 75:07 - 75:09
    The question is, which ones?
  • 75:09 - 75:14
    Because it's not obvious
    at all, except for theta.
  • 75:14 - 75:15
    Theta is nice.
  • 75:15 - 75:16
    He's so nice.
  • 75:16 - 75:20
    And we say, OK theta,
    we are grateful to you.
  • 75:20 - 75:25
    We put you at the end, because
    it's a complete rotation.
  • 75:25 - 75:31
    And we know you are between 0
    and 2 pi, very reliable guy.
  • 75:31 - 75:34
    Phi is not so reliable.
  • 75:34 - 75:36
    Well, phi is a nice guy.
  • 75:36 - 75:40
    But he puts us through
    a little bit of work.
  • 75:40 - 75:41
    Do we like to work?
  • 75:41 - 75:46
    Well, not so much,
    but we'll try.
  • 75:46 - 75:53
    So we need to know a little
    bit more about this triangle.
  • 75:53 - 75:56
  • 75:56 - 76:01
    We need to understand a little
    bit more about this triangle.
  • 76:01 - 76:05
    STUDENT: Well, the angle
    between the angle at the bottom
  • 76:05 - 76:06
    is 45 degrees.
  • 76:06 - 76:07
    PROFESSOR: How can you say?
  • 76:07 - 76:09
    STUDENT: Because the
    slope of that line is 1.
  • 76:09 - 76:13
    PROFESSOR: Right, so say,
    now I'm going to observe z
  • 76:13 - 76:14
    was a as well.
  • 76:14 - 76:19
  • 76:19 - 76:23
    So that means it's a
    right isosceles triangle.
  • 76:23 - 76:25
    If it's a right
    isosceles triangle,
  • 76:25 - 76:28
    this is 45 degree angle.
  • 76:28 - 76:37
    So this is from d phi from
    0 to pi over 4, excellent.
  • 76:37 - 76:41
    Finally, the only one that gives
    us a little bit of a headache
  • 76:41 - 76:47
    but not too much of a
    headache is the radius r.
  • 76:47 - 76:48
    Should I change the color?
  • 76:48 - 76:51
    No, I'll leave it
    r dr. So we have
  • 76:51 - 77:02
    to think a little bit of
    the meaning of our rays.
  • 77:02 - 77:04
    Drawing vertical strips
    or horizontal strips
  • 77:04 - 77:07
    or whatever strips
    is not a good idea.
  • 77:07 - 77:09
    When we are in
    spherical coordinates,
  • 77:09 - 77:12
    what do we need to draw?
  • 77:12 - 77:16
    Rays, like rays of sun
    coming from a source.
  • 77:16 - 77:21
    The source is here at the
    origin in spherical coordinates.
  • 77:21 - 77:25
    These are like rays of
    sun that are free to move.
  • 77:25 - 77:27
    But they bump.
  • 77:27 - 77:32
    They just bump against
    the plane, the flat roof.
  • 77:32 - 77:36
    So they would reflect if
    this were a physical problem.
  • 77:36 - 77:39
  • 77:39 - 77:43
    So definitely all
    your rays start at 0.
  • 77:43 - 77:45
    So you have to put 0 here.
  • 77:45 - 77:49
    But this is a question mark.
  • 77:49 - 77:50
    STUDENT: [INAUDIBLE].
  • 77:50 - 77:58
  • 77:58 - 77:59
    STUDENT: a square root 2.
  • 77:59 - 78:02
  • 78:02 - 78:04
    PROFESSOR: No, it's
    not a fixed answer.
  • 78:04 - 78:07
    So you have z will be a fixed.
  • 78:07 - 78:10
    But who was z in
    spherical coordinates?
  • 78:10 - 78:13
    That was the only
    thing you can ask.
  • 78:13 - 78:16
    So z equals a is your
    tradition that is the roof.
  • 78:16 - 78:18
    STUDENT: That would
    be r [INAUDIBLE].
  • 78:18 - 78:28
    PROFESSOR: Very good,
    r cosine of phi,
  • 78:28 - 78:33
    of the latitude
    from the North Pole.
  • 78:33 - 78:34
    This is 45.
  • 78:34 - 78:39
    But I mean for a point like
    this, phi will be this phi.
  • 78:39 - 78:40
    Do you guys understand?
  • 78:40 - 78:44
    Phi could be any point where the
    point inside [INAUDIBLE], phi
  • 78:44 - 78:46
    will be the latitude
    from the North Pole.
  • 78:46 - 78:52
    OK, so the way you do it
    is r is between 0 and z
  • 78:52 - 78:57
    over cosine phi.
  • 78:57 - 78:58
    And that's the hard thing.
  • 78:58 - 79:02
    Since z at the
    roof is a, you have
  • 79:02 - 79:07
    to put here a over-- a is
    fixed, that 43 of yours,
  • 79:07 - 79:09
    whatever it was-- cosine phi.
  • 79:09 - 79:14
  • 79:14 - 79:18
    So when you guys integrate
    with respect to r,
  • 79:18 - 79:24
    assume this F will be 1,
    just like you asked me, Alex.
  • 79:24 - 79:27
    That would make my life
    easier and would be good.
  • 79:27 - 79:29
    When I integrate
    with respect to r,
  • 79:29 - 79:32
    would it be hard
    to solve a problem?
  • 79:32 - 79:33
    Oh, not so hard.
  • 79:33 - 79:35
    Why?
  • 79:35 - 79:38
    OK, integrate this
    with respect to r.
  • 79:38 - 79:40
    We have r cubed.
  • 79:40 - 79:42
    Integrate r squared.
  • 79:42 - 79:43
    We have r cubed over 3, right?
  • 79:43 - 79:49
    Let's do this, solve the
    same problem when F is 1.
  • 79:49 - 79:55
  • 79:55 - 80:03
    Solve the same problem when
    F would be 1, for F equals 1.
  • 80:03 - 80:07
    Then you get integral
    from 0 to 2 pi,
  • 80:07 - 80:11
    integral from 0 to pi
    over 4, integral from 0
  • 80:11 - 80:22
    to a over cosine phi, 1 r
    squared sine phi dr d phi d
  • 80:22 - 80:22
    theta.
  • 80:22 - 80:26
    The guy that sits on my
    nerves is again theta.
  • 80:26 - 80:27
    He's very nice.
  • 80:27 - 80:30
    He can be eliminated
    from the game.
  • 80:30 - 80:34
    So 2 pi out, and I
    will focus my attention
  • 80:34 - 80:37
    to the product of function.
  • 80:37 - 80:41
    Well, OK, I have to
    integrate one at a time.
  • 80:41 - 80:43
    So I integrate with
    respect to what?
  • 80:43 - 80:46
    STUDENT: [INAUDIBLE].
  • 80:46 - 80:50
    PROFESSOR: So I get r cubed
    over 3, all right, the integral
  • 80:50 - 80:53
    from 0 to pi over 4.
  • 80:53 - 80:55
    STUDENT: [INAUDIBLE].
  • 80:55 - 80:59
    PROFESSOR: r cubed over 3
    between-- it's a little bit
  • 80:59 - 81:03
    of a headache. r equals
    a over cosine phi.
  • 81:03 - 81:05
    And I bet you my video
    doesn't see anything,
  • 81:05 - 81:08
    so let me change the colors.
  • 81:08 - 81:11
    r equals a over cosine phi.
  • 81:11 - 81:13
    And r equals 0 down.
  • 81:13 - 81:15
    That's the easy part.
  • 81:15 - 81:19
    Inside I have r
    cubed over 3, right?
  • 81:19 - 81:26
    All right, and sine
    phi, and all I'm
  • 81:26 - 81:32
    left with is a phi
    integration, is an integration
  • 81:32 - 81:34
    with respect to phi.
  • 81:34 - 81:36
    Let's see-- yes, sir.
  • 81:36 - 81:37
    STUDENT: [INAUDIBLE].
  • 81:37 - 81:41
    PROFESSOR: Well, I should be
    able to manage with this guy.
  • 81:41 - 81:47
  • 81:47 - 81:47
    STUDENT: [INAUDIBLE].
  • 81:47 - 82:05
  • 82:05 - 82:07
    PROFESSOR: I'm writing
    just as you said, OK?
  • 82:07 - 82:14
  • 82:14 - 82:16
    Now, how much of a headache
    do you think this is?
  • 82:16 - 82:18
    STUDENT: It's not much
    of one, because it's
  • 82:18 - 82:21
    the same as a tangent
    times the secant squared
  • 82:21 - 82:23
    with a constant pulled out.
  • 82:23 - 82:26
    STUDENT: So psi and
    cosine don't [INAUDIBLE].
  • 82:26 - 82:34
    Tangents will give
    you 1 over cosine--
  • 82:34 - 82:37
    PROFESSOR: What's the simplest
    way to do it without thinking
  • 82:37 - 82:40
    of tangent and cotangent, huh?
  • 82:40 - 82:41
    STUDENT: [INAUDIBLE].
  • 82:41 - 82:44
    PROFESSOR: Instead, a
    u substitution there?
  • 82:44 - 82:45
    What is the u substitution?
  • 82:45 - 82:48
    STUDENT: [INAUDIBLE].
  • 82:48 - 82:50
    PROFESSOR: Is this good?
  • 82:50 - 82:51
    STUDENT: No.
  • 82:51 - 82:52
    PROFESSOR: No?
  • 82:52 - 82:55
    STUDENT: [INAUDIBLE].
  • 82:55 - 82:58
    PROFESSOR: It's
    u to the minus 3.
  • 82:58 - 83:00
    And that's OK.
  • 83:00 - 83:06
    So I have 2 pi a cubed
    over 3 [INAUDIBLE]
  • 83:06 - 83:10
    because they are in my way
    there making my life miserable,
  • 83:10 - 83:11
    integral.
  • 83:11 - 83:18
    And then I have u to the
    minus 3 times-- for du
  • 83:18 - 83:22
    I get a minus that
    that is sort of ugh.
  • 83:22 - 83:26
    I have to invent the minus, and
    I have to invent the minus here
  • 83:26 - 83:28
    in front as well.
  • 83:28 - 83:32
    So they will compensate
    for one another.
  • 83:32 - 83:35
    And I'll say du.
  • 83:35 - 83:40
    But these limit points, of
    course I can do them by myself.
  • 83:40 - 83:42
    I don't need your help.
  • 83:42 - 83:46
    But I pretend that
    I need your help.
  • 83:46 - 83:48
    What will be u when phi is 0?
  • 83:48 - 83:49
    STUDENT: 1.
  • 83:49 - 83:52
    PROFESSOR: 1.
  • 83:52 - 83:57
    What will be u when
    phi is pi over 4?
  • 83:57 - 83:58
    STUDENT: [INAUDIBLE].
  • 83:58 - 84:02
  • 84:02 - 84:04
    PROFESSOR: And from now on
    you should be able to do this.
  • 84:04 - 84:15
    So I have minus 2 pi a cubed
    over 3 times-- I integrate.
  • 84:15 - 84:18
    So I add the power, I add
    the 1, and I add the 1.
  • 84:18 - 84:20
    So you have u to the
    minus 2 over minus 2.
  • 84:20 - 84:27
    Are you guys with
    me-- between u equals
  • 84:27 - 84:31
    1 and u equals root 2 over 2.
  • 84:31 - 84:33
    I promise you if
    you have something
  • 84:33 - 84:35
    like that in the final
    and you stop here,
  • 84:35 - 84:38
    I'm not going to be blaming you.
  • 84:38 - 84:41
    I'll say, very good, leave
    it there, I don't care.
  • 84:41 - 84:45
    Because from this
    point on, what follows
  • 84:45 - 84:48
    is just routine algebra.
  • 84:48 - 84:52
    So we have-- I hate this.
  • 84:52 - 84:55
    I'm not a calculator.
  • 84:55 - 85:00
    But it's better for me to write
    1 over root 2, like you said.
  • 85:00 - 85:03
    Because in that case, the
    square will be 1 over 2.
  • 85:03 - 85:06
    And when I invert 1
    over 2, I get a 2.
  • 85:06 - 85:11
    So I have 2 over minus 2.
  • 85:11 - 85:12
    Are you guys with me again?
  • 85:12 - 85:14
    So I'm thinking the
    same-- 1 over root 2.
  • 85:14 - 85:17
    Square it, you have 1 over 2.
  • 85:17 - 85:21
    Take it as a minus,
    you have exactly 2.
  • 85:21 - 85:24
    And you have 2 over
    minus-- is this a minus?
  • 85:24 - 85:27
    I'm so silly, look
    at me, minus 2.
  • 85:27 - 85:29
    STUDENT: It's a cubed
    over 3, not over 2.
  • 85:29 - 85:32
    PROFESSOR: It's going to be--
  • 85:32 - 85:34
    STUDENT: You've got an a
    cubed over 2 right there.
  • 85:34 - 85:36
    And it was--
  • 85:36 - 85:37
    PROFESSOR: Huh?
  • 85:37 - 85:39
    STUDENT: You just wrote
    2 pi a cubed over 2.
  • 85:39 - 85:41
    It's a cubed over 3.
  • 85:41 - 85:43
    PROFESSOR: Yes,
    it's my silliness.
  • 85:43 - 85:46
    I looked, and I say
    this instead of that.
  • 85:46 - 85:48
    Thank you so much.
  • 85:48 - 85:50
    What do I have here?
  • 85:50 - 85:52
    1 over minus 2.
  • 85:52 - 85:55
    In the end, what does this mean?
  • 85:55 - 85:56
    Let's see, what does this mean?
  • 85:56 - 86:01
    When I plug in, I subtract.
  • 86:01 - 86:02
    This is what?
  • 86:02 - 86:08
    This is minus 1 plus
    1/2 is minus 1/2.
  • 86:08 - 86:12
    But that minus
    should not scare me.
  • 86:12 - 86:14
    Because of course
    a minus in a volume
  • 86:14 - 86:16
    would be completely wrong.
  • 86:16 - 86:18
    But I have a minus from before.
  • 86:18 - 86:32
    So it's plus 2 pi times a
    cubed over 3, and times 1/2.
  • 86:32 - 86:35
    So in the end, the
    answer, the total answer,
  • 86:35 - 86:37
    would be answered what?
  • 86:37 - 86:40
    STUDENT: [INAUDIBLE].
  • 86:40 - 86:45
    PROFESSOR: Pi a cubed
    over 3, pi a cubed over 3.
  • 86:45 - 86:47
    It looks very-- huh?
  • 86:47 - 86:48
    It looks pretty.
  • 86:48 - 86:53
    Actually yes, it looks
    pretty because-- now,
  • 86:53 - 86:56
    OK, I'm asking you a question.
  • 86:56 - 87:00
    Would we have done
    that without calculus?
  • 87:00 - 87:06
    If somebody told you [INAUDIBLE]
    it has a volume of some cone,
  • 87:06 - 87:09
    what's the volume of a cone?
  • 87:09 - 87:13
    Area of the base times
    the height divided by 3.
  • 87:13 - 87:17
    So you could have very nicely
    cheated on me on the exam
  • 87:17 - 87:21
    by saying, you
    have this cone that
  • 87:21 - 87:26
    has pi is squared times a-- pi
    is squared times a-- divided
  • 87:26 - 87:30
    by 3 equals pi cubed over 3.
  • 87:30 - 87:33
    When can you not
    cheat on this problem?
  • 87:33 - 87:35
    STUDENT: When you say,
    you've got to do it with a--
  • 87:35 - 87:38
    PROFESSOR: Exactly, when I
    say, do it with a-- well,
  • 87:38 - 87:45
    I can say, OK, if we say, set up
    the integral and write it down,
  • 87:45 - 87:47
    you set up the integral
    and write it down.
  • 87:47 - 87:50
    If we say, set up the
    integral and compute it,
  • 87:50 - 87:54
    you set up the integral,
    you fake the computation,
  • 87:54 - 87:55
    and you come up with this.
  • 87:55 - 87:58
  • 87:58 - 88:02
    If we say, set up the integral
    and show all your work,
  • 88:02 - 88:03
    then you're in trouble.
  • 88:03 - 88:09
    But I'm going to try to advocate
    that for a simple problem, that
  • 88:09 - 88:11
    is actually elementary.
  • 88:11 - 88:16
    One should not have
    to show all the work.
  • 88:16 - 88:19
    All right, but keep in mind
    when you have 2 minuses
  • 88:19 - 88:23
    like that-- that reminds me.
  • 88:23 - 88:29
    So there was a professor whose
    sink didn't work anymore.
  • 88:29 - 88:32
    And he asked for a plumber
    to come to his house.
  • 88:32 - 88:33
    He was a math professor.
  • 88:33 - 88:37
    So the plumber comes to his
    house and fixes this, and says,
  • 88:37 - 88:38
    what else is wrong?
  • 88:38 - 88:40
    Fixes the toilet, fixes
    everything in the house,
  • 88:40 - 88:44
    and then he shows the
    professor the bill.
  • 88:44 - 88:50
    So the guy said, oh my god, this
    is 1/3 of my monthly salary.
  • 88:50 - 88:54
    So the plumber said,
    yeah, I mean, really?
  • 88:54 - 88:55
    You're a smart guy.
  • 88:55 - 88:55
    You're a professor.
  • 88:55 - 88:57
    You make that little money?
  • 88:57 - 88:59
    Yeah, really.
  • 88:59 - 89:00
    I'm so sorry for you.
  • 89:00 - 89:04
    Why don't you apply
    to our company
  • 89:04 - 89:07
    and become a plumber if you're
    interested, if you crave money?
  • 89:07 - 89:09
    No, of course, I need
    money desperately.
  • 89:09 - 89:13
    I have five children
    and a wife [INAUDIBLE].
  • 89:13 - 89:15
    OK, he applies.
  • 89:15 - 89:17
    And he says, pay attention.
  • 89:17 - 89:21
    Don't write that you are a
    professor or you have a PhD.
  • 89:21 - 89:24
    Just say you just finished
    high school or say,
  • 89:24 - 89:25
    I didn't finish high school.
  • 89:25 - 89:27
    So he writes, I didn't
    finish high school.
  • 89:27 - 89:29
    I went to 10th grade.
  • 89:29 - 89:30
    They accept him.
  • 89:30 - 89:32
    They give him a job.
  • 89:32 - 89:35
    And they say, this
    is your salary.
  • 89:35 - 89:36
    But there is something new.
  • 89:36 - 89:40
    Everybody has to
    finish high school.
  • 89:40 - 89:43
    So they have to
    take AP Calculus.
  • 89:43 - 89:45
    So he goes, oh my god.
  • 89:45 - 89:46
    They all go.
  • 89:46 - 89:50
    And there comes a TA from
    the community college.
  • 89:50 - 89:51
    The class was full.
  • 89:51 - 89:56
    He tries to solve a
    problem-- with calculus
  • 89:56 - 90:01
    compute the area inside
    this disc of radius a.
  • 90:01 - 90:04
    So the TA-- OK, I did this.
  • 90:04 - 90:07
    I got minus pi a squared.
  • 90:07 - 90:12
    And the professor says,
    OK, you cannot get that.
  • 90:12 - 90:14
    Let me explain to you.
  • 90:14 - 90:16
    He goes, I don't know
    where he made a mistake.
  • 90:16 - 90:22
    Because I still get-- where
    is minus pi a squared?
  • 90:22 - 90:23
    I don't see where
    the mistake is.
  • 90:23 - 90:27
    And then the whole
    class, 12, 15-- reverse
  • 90:27 - 90:30
    the integral limits.
  • 90:30 - 90:34
    Change the integral limits
    and you'll get it right.
  • 90:34 - 90:41
    So we can all pretend that
    we want to do something else
  • 90:41 - 90:46
    and we didn't finish high school
    and we'll get a lot more money.
  • 90:46 - 90:48
    The person who came to
    fix my air conditioner
  • 90:48 - 90:55
    said that he actually
    makes about $100 an hour.
  • 90:55 - 90:57
    And I was thinking, wow.
  • 90:57 - 91:00
    Wow, I'll never get there.
  • 91:00 - 91:02
    But that's impressive.
  • 91:02 - 91:05
    Just changing some
    things and fix,
  • 91:05 - 91:08
    press the button, $100 an hour.
  • 91:08 - 91:11
    STUDENT: But they don't
    work full time. [INAUDIBLE].
  • 91:11 - 91:15
    PROFESSOR: Yeah, and I think
    they are paid by the job.
  • 91:15 - 91:19
    But in any case, whether
    it's a simple job
  • 91:19 - 91:21
    and they just-- there
    is a contact that's
  • 91:21 - 91:26
    missing or something
    trivial, they still
  • 91:26 - 91:28
    charge a lot of money.
  • 91:28 - 91:30
    STUDENT: [INAUDIBLE].
  • 91:30 - 91:32
    PROFESSOR: A professor?
  • 91:32 - 91:34
    STUDENT: [INAUDIBLE].
  • 91:34 - 91:35
    PROFESSOR: What?
  • 91:35 - 91:38
    [LAUGHING] No.
  • 91:38 - 91:39
    STUDENT: I know the professor.
  • 91:39 - 91:40
    I won't tell you who.
  • 91:40 - 91:42
    PROFESSOR: OK, I
    don't want to know.
  • 91:42 - 91:43
    I don't want to know.
  • 91:43 - 91:45
    But anyway, it's interesting.
  • 91:45 - 91:47
    STUDENT: But he doesn't
    do in the college.
  • 91:47 - 91:51
    He does outside the college
    by just advising it.
  • 91:51 - 91:54
    PROFESSOR: Oh, you mean
    like consulting or tutoring
  • 91:54 - 91:54
    or stuff like that?
  • 91:54 - 91:57
    STUDENT: Not tutoring,
    consulting for the--
  • 91:57 - 91:59
    PROFESSOR: Consulting.
  • 91:59 - 92:03
    Actually, I bet that
    if we did tutoring,
  • 92:03 - 92:06
    which we don't have time for,
    we would make a lot of money.
  • 92:06 - 92:09
    But the nature of
    my job, for example,
  • 92:09 - 92:12
    is that I work about
    60 hours a week, 65,
  • 92:12 - 92:15
    and I will not have any time
    left to do other things,
  • 92:15 - 92:18
    like consulting,
    tutoring, and stuff.
  • 92:18 - 92:20
    STUDENT: [INAUDIBLE].
  • 92:20 - 92:22
    PROFESSOR: I don't need
    normally that much.
  • 92:22 - 92:25
    I don't crave money that much.
  • 92:25 - 92:27
    STUDENT: [INAUDIBLE].
  • 92:27 - 92:29
    PROFESSOR: I have a
    friend who got a masters.
  • 92:29 - 92:31
    She didn't get a PhD.
  • 92:31 - 92:35
    She got an offer from
    this-- I told you about her.
  • 92:35 - 92:36
    She moved to California.
  • 92:36 - 92:39
    She was a single mom.
  • 92:39 - 92:42
    She earns a lot of
    money working for Pixar.
  • 92:42 - 92:45
    And she helped with all
    the animation things.
  • 92:45 - 92:48
  • 92:48 - 92:52
    It was about 15 years
    ago that she started.
  • 92:52 - 92:54
    And it was really hard.
  • 92:54 - 93:01
    We were all on Toy Story
    and that kind of-- what
  • 93:01 - 93:04
    was that called?
  • 93:04 - 93:08
    There were two
    rendering algorithms,
  • 93:08 - 93:09
    rendering algorithms.
  • 93:09 - 93:14
    Two masters students
    were interested in that.
  • 93:14 - 93:16
    They got in immediately.
  • 93:16 - 93:19
    To be hired, I think
    a post-doc with a PhD
  • 93:19 - 93:23
    was making about $40,000.
  • 93:23 - 93:25
    That was my offer.
  • 93:25 - 93:31
    My first offer was a post-doc
    at Urbana-Champaign for $38,000
  • 93:31 - 93:34
    while she was at the hundred
    and something thousand
  • 93:34 - 93:37
    dollars to start with
    working at Disney.
  • 93:37 - 93:41
    Imagine-- with just a masters,
    no aspiration for a PhD
  • 93:41 - 93:43
    whatever.
  • 93:43 - 93:46
    So in a way, if you're
    thinking of doing this,
  • 93:46 - 93:51
    a masters in mathematics
    is probably paying off.
  • 93:51 - 93:54
    Because it opens a
    lot of doors for you.
  • 93:54 - 93:56
    And that's just in general.
  • 93:56 - 93:59
    I mean, masters in engineering
    opens a lot of doors.
  • 93:59 - 94:02
    But in a way, you
    pay a price after
  • 94:02 - 94:06
    if you want to start
    even further, get a PhD,
  • 94:06 - 94:07
    stay in academia.
  • 94:07 - 94:08
    Then you pay a price.
  • 94:08 - 94:11
    And if you want to
    augment your salary,
  • 94:11 - 94:16
    you really have to be very
    good and accomplish some--
  • 94:16 - 94:19
    get [INAUDIBLE]
    two or three times
  • 94:19 - 94:23
    and get higher up
    each [INAUDIBLE].
  • 94:23 - 94:28
    But we all struggle
    with these issues.
  • 94:28 - 94:31
    It's a lot of work.
  • 94:31 - 94:34
    But having a masters
    in math is not so hard.
  • 94:34 - 94:39
    If you like math,
    it's easy to get it.
  • 94:39 - 94:40
    It's a pleasure.
  • 94:40 - 94:42
    It's not a lot of hours.
  • 94:42 - 94:46
    I think in 36 hours in most
    schools you can get a masters.
  • 94:46 - 94:50
    And it's doable.
  • 94:50 - 95:02
    All right, let's go back to
    review Chapter 11 briefly here.
  • 95:02 - 95:12
  • 95:12 - 95:14
    Is this on the midterm?
  • 95:14 - 95:16
    No, but it's going
    to be on the final.
  • 95:16 - 95:23
  • 95:23 - 95:33
    Assume you have a
    x equals u plus v,
  • 95:33 - 95:47
    y equals u minus v. Write
    the following derivative.
  • 95:47 - 95:57
  • 95:57 - 96:14
    dx/dv where u of t equals
    t squared and v equals t.
  • 96:14 - 96:31
    Do these both directly
    and by writing a chain
  • 96:31 - 96:38
    rule for the values you have.
  • 96:38 - 96:44
  • 96:44 - 96:46
    OK, how do we do this directly?
  • 96:46 - 96:48
    It's probably the simplest way.
  • 96:48 - 96:57
  • 96:57 - 97:02
    Replace u by t squared, replace
    v by t and see what you have.
  • 97:02 - 97:03
    So 1, directly.
  • 97:03 - 97:08
  • 97:08 - 97:12
    X of t equals t squared plus t.
  • 97:12 - 97:16
    y of t equals t squared minus t.
  • 97:16 - 97:24
  • 97:24 - 97:25
    Good.
  • 97:25 - 97:33
    So it's a piece of cake.
    dx/dt equals 2t plus 1.
  • 97:33 - 97:38
    Unfortunately, this is just
    the first part of the problem.
  • 97:38 - 97:41
    And it's actually
    [INAUDIBLE] to show the chain
  • 97:41 - 97:44
    rule for the mappings we have.
  • 97:44 - 97:45
    And what mappings do we have?
  • 97:45 - 97:54
    We have a map from t
    to u of t and v of t.
  • 97:54 - 98:00
    And then again, from u of t and
    v of t to x of t and y of t.
  • 98:00 - 98:05
    And the transformation is
    what? x equals u plus v,
  • 98:05 - 98:10
    y equals u minus v. And we have
    another transformation here.
  • 98:10 - 98:15
    So how do you write dx/dt?
  • 98:15 - 98:21
    x is a function
    of u and v, right?
  • 98:21 - 98:25
    So first you say
    that dx/dv round,
  • 98:25 - 98:28
    which means we do it
    with the first variable.
  • 98:28 - 98:31
    I'll write it for
    you to see better,
  • 98:31 - 98:39
    that initially your x and y
    were functions of u and v.
  • 98:39 - 98:51
    Times-- what is that?
    dv/dt plus dx/du.
  • 98:51 - 98:53
    You can change the order.
  • 98:53 - 98:56
    If you didn't like
    that I started with v,
  • 98:56 - 99:00
    I could have started with
    the u, and the u, and the v,
  • 99:00 - 99:01
    and the v here.
  • 99:01 - 99:04
    It doesn't matter.
  • 99:04 - 99:06
    Guys, do you mind, really?
  • 99:06 - 99:08
    v, v. u, u.
  • 99:08 - 99:09
    Shooting cowboys?
  • 99:09 - 99:11
    Doesn't matter, remember just
    that they're [INAUDIBLE].
  • 99:11 - 99:14
  • 99:14 - 99:15
    D sorry, d.
  • 99:15 - 99:18
    Because where there
    is no other variable,
  • 99:18 - 99:23
    we would put v. So dx/dt?
  • 99:23 - 99:25
    Lets see if we get
    the same answer.
  • 99:25 - 99:26
    We should.
  • 99:26 - 99:28
    What is dx/dt?
  • 99:28 - 99:31
    1, from here.
  • 99:31 - 99:32
    What is dv/dt?
  • 99:32 - 99:38
  • 99:38 - 99:43
    1 plus dx/du.
  • 99:43 - 99:46
    1, du/dt.
  • 99:46 - 99:48
    2t.
  • 99:48 - 99:50
    If we were to do
    the same thing-- so
  • 99:50 - 99:52
    we got the same answer.
  • 99:52 - 99:56
    If you want to do
    the same thing,
  • 99:56 - 100:02
    quickly with respect
    to say dy/dt,
  • 100:02 - 100:06
    suppose that most finals
    ask you to do both.
  • 100:06 - 100:08
    I have students
    who didn't finish
  • 100:08 - 100:13
    because they didn't
    have the time to finish,
  • 100:13 - 100:15
    but that was just my policy.
  • 100:15 - 100:18
    When I grade it,
    I gave them 100%,
  • 100:18 - 100:21
    no matter if they
    stopped here, because I
  • 100:21 - 100:23
    said you prove to me that
    you know the chain rule.
  • 100:23 - 100:27
    Why would I punish you further?
  • 100:27 - 100:28
    So that's what I do.
  • 100:28 - 100:32
    But I want you to do it
    now, without my help.
  • 100:32 - 100:35
    Both ways, dy/dt.
  • 100:35 - 100:39
    First you do it
    with the chain rule.
  • 100:39 - 100:42
    First you write those
    three [INAUDIBLE].
  • 100:42 - 100:48
  • 100:48 - 100:49
    dy del y.
  • 100:49 - 100:52
  • 100:52 - 100:56
    del u, du/dt, plus del y.
  • 100:56 - 100:59
    del v, dv/dt.
  • 100:59 - 101:04
    I'm not going to write it
    down, you write it down.
  • 101:04 - 101:06
    What I'm going to
    write down is what
  • 101:06 - 101:08
    you tell me the numbers are.
  • 101:08 - 101:13
  • 101:13 - 101:14
    For everything.
  • 101:14 - 101:20
  • 101:20 - 101:25
    STUDENT: Dy divided by d
  • 101:25 - 101:30
    PROFESSOR: Or just give me
    the final answer in terms of
  • 101:30 - 101:30
    [INAUDIBLE].
  • 101:30 - 101:42
  • 101:42 - 101:48
    What are the two [INAUDIBLE]?
  • 101:48 - 101:50
    Tell me.
  • 101:50 - 101:57
    Tell me, this times this,
    plus this times that.
  • 101:57 - 101:58
    What?
  • 101:58 - 101:59
    So let's write down.
  • 101:59 - 102:01
    Let's write it down together.
  • 102:01 - 102:16
    dy/du, du/dt, plus dy/dv dv/dt.
  • 102:16 - 102:17
    Alright.
  • 102:17 - 102:30
  • 102:30 - 102:35
    1 This is 1.
  • 102:35 - 102:36
    How much is dy/dt?
  • 102:36 - 102:39
  • 102:39 - 102:40
    Or du/dt, I'm sorry.
  • 102:40 - 102:45
    I said dy, it's du/dt.
  • 102:45 - 102:51
    Plus minus 1, excellent.
  • 102:51 - 102:54
    Times 1.
  • 102:54 - 102:56
    Of course you would have
    done the same thing,
  • 102:56 - 103:00
    by plugging in the
    variables and saying well,
  • 103:00 - 103:05
    I have y, which is this
    is t squared, this is t,
  • 103:05 - 103:09
    and I have t squared minus
    t prime is 2t minus 1.
  • 103:09 - 103:14
    That's a simpler way
    to verify [INAUDIBLE].
  • 103:14 - 103:14
    OK.
  • 103:14 - 103:20
    So remember to do that,
    have this in mind,
  • 103:20 - 103:25
    because on the final you may
    have something like that.
  • 103:25 - 103:29
    As we keep going in
    the month of April,
  • 103:29 - 103:33
    I'm going to do as much review
    as possible for the final.
  • 103:33 - 103:37
    Mark a star, or F, not the grade
    F, but F around for the final,
  • 103:37 - 103:45
    put F and circle there to say
    review this for the final.
  • 103:45 - 103:49
    And since we are still
    in chapter 11 review,
  • 103:49 - 103:57
    we'll do another problem
    of F, final review
  • 103:57 - 104:02
    that I didn't put on the midterm
    but it may be on the final.
  • 104:02 - 104:07
    Let's say given the
    constraint x squared
  • 104:07 - 104:13
    plus y squared plus z squared
    equals 5, compute z sub x
  • 104:13 - 104:17
    and z sub y.
  • 104:17 - 104:18
    How do you do that?
  • 104:18 - 104:21
    What is this called,
    actually, and why is it
  • 104:21 - 104:23
    so important for the final?
  • 104:23 - 104:24
    It's called implicit
    differentiation
  • 104:24 - 104:29
    and it appears on almost every
    final, at least once a year,
  • 104:29 - 104:32
    so there is always
    a big possibility
  • 104:32 - 104:36
    that you are going to
    see something like that.
  • 104:36 - 104:42
    I taught you how to think in
    terms of implicit functions.
  • 104:42 - 104:50
    If you think of z as
    a function of x and y.
  • 104:50 - 104:52
    That's a way of changing
    your perspective.
  • 104:52 - 104:57
    So you say, OK, I
    understand that z
  • 104:57 - 105:01
    has to be viewed as a
    function of x and y.
  • 105:01 - 105:05
    I'm just changing
    my perspective.
  • 105:05 - 105:10
    STUDENT: For that one,
    wouldn't you just solve for z?
  • 105:10 - 105:11
    PROFESSOR: No.
  • 105:11 - 105:16
    Solving for z would make
    your life a lot harder.
  • 105:16 - 105:18
    The point of
    implicit functions is
  • 105:18 - 105:20
    that you don't separate them.
  • 105:20 - 105:23
    If you're going
    to separate them,
  • 105:23 - 105:26
    you have to separately
    integrate these.
  • 105:26 - 105:28
    And it's a headache.
  • 105:28 - 105:31
    It's easier-- actually
    it's a good question.
  • 105:31 - 105:36
    It's easier to do z sub x,
    z sub y without splitting it
  • 105:36 - 105:37
    into two cases.
  • 105:37 - 105:40
  • 105:40 - 105:43
    Step two.
  • 105:43 - 105:45
    Differentiate this
    with respect to x.
  • 105:45 - 105:48
    What do we have?
  • 105:48 - 105:56
    2x plus 0 plus the chain rule--
    don't write the chain rule.
  • 105:56 - 106:00
    2 jumping down, it jumped down.
  • 106:00 - 106:06
    2z times-- cover the
    2 with your hand.
  • 106:06 - 106:08
    z sub x, very good.
  • 106:08 - 106:12
    z prime with respect
    to x equals zero.
  • 106:12 - 106:14
    Good.
  • 106:14 - 106:18
    So z sub x, step three.
  • 106:18 - 106:19
    And the last step.
  • 106:19 - 106:23
    See sub x will be what?
  • 106:23 - 106:24
    Pull it out.
  • 106:24 - 106:26
    Pull this 2 out.
  • 106:26 - 106:32
    Minus x over z.
  • 106:32 - 106:36
  • 106:36 - 106:40
    The other one is symmetric.
  • 106:40 - 106:44
    Alex said let's be smart
    and not do the whole thing
  • 106:44 - 106:44
    all over again.
  • 106:44 - 106:47
    Look at beautiful
    symmetric polynomial.
  • 106:47 - 106:50
    You would have to be a
    little bit careful with when
  • 106:50 - 106:54
    you have a 1 here and
    y would have a 2 here.
  • 106:54 - 106:57
    It wouldn't be
    symmetric in x and y.
  • 106:57 - 107:00
    But here, if you reverse
    the roles of x and y,
  • 107:00 - 107:02
    it's not a big deal.
  • 107:02 - 107:03
    Are you guys with me?
  • 107:03 - 107:07
    Here we are. z sub y
    equals minus y over z.
  • 107:07 - 107:10
    Am I right?
  • 107:10 - 107:14
    Keep this in mind
    for-- I also saw,
  • 107:14 - 107:19
    when I was looking at
    the [INAUDIBLE] library
  • 107:19 - 107:21
    files, [INAUDIBLE].
  • 107:21 - 107:25
    I also saw exams, and I was
    looking at your reviews there.
  • 107:25 - 107:28
    I was looking at [INAUDIBLE].
  • 107:28 - 107:32
    The University of Houston has
    a very beautiful online, free
  • 107:32 - 107:37
    library of calculus 1
    and calculus 2 exams
  • 107:37 - 107:40
    that I found very useful.
  • 107:40 - 107:44
    Now, one of them--
    listen to me so you
  • 107:44 - 107:47
    don't fall through this crack.
  • 107:47 - 107:54
    On the Cal 2 exam, they
    wrote something like that.
  • 107:54 - 108:00
  • 108:00 - 108:06
    You don't have to write 1 over
    x squared, and then compute.
  • 108:06 - 108:09
    You just say, OK, if the natural
    part of the of the argument
  • 108:09 - 108:13
    is 5, then the
    argument is a constant.
  • 108:13 - 108:15
    And I don't care
    what constant it
  • 108:15 - 108:18
    is, it it's something
    that prime will give me 0,
  • 108:18 - 108:20
    it's the same problem.
  • 108:20 - 108:21
    Are you guys with me?
  • 108:21 - 108:26
    So in that case, I'm going
    have just what kind of change?
  • 108:26 - 108:29
    This will be to the 5.
  • 108:29 - 108:31
    And I still have 0.
  • 108:31 - 108:33
    It's the same answer.
  • 108:33 - 108:37
    They just wanted to play
    games, and you can play games.
  • 108:37 - 108:41
    For example, you can make this.
  • 108:41 - 108:43
    If you really have
    a working mind,
  • 108:43 - 108:51
    and most mathematicians do,
    give this to your students.
  • 108:51 - 108:54
    I mean, most people
    freak out so bad
  • 108:54 - 108:59
    when they see that, the
    won't even touch it.
  • 108:59 - 109:02
    It's just all in the head.
  • 109:02 - 109:13
    Remember that log in base
    17 of a would be what?
  • 109:13 - 109:16
    STUDENT: If it's a
    constant, it's to the 17th.
  • 109:16 - 109:17
    PROFESSOR: Who knows?
  • 109:17 - 109:19
    STUDENT: What do you
    mean, you don't do that?
  • 109:19 - 109:23
    PROFESSOR: No, no, expressed
    in terms of natural logs.
  • 109:23 - 109:24
    STUDENT: Natural log?
  • 109:24 - 109:27
    The natural log of a
    over natural log of 17.
  • 109:27 - 109:28
    PROFESSOR: Very good.
  • 109:28 - 109:30
    So what does this matter?
  • 109:30 - 109:33
    In the end, you multiply 2, you
    do the derivative, you still
  • 109:33 - 109:35
    get the same answer.
  • 109:35 - 109:38
    Some people are trying
    to make things scarier
  • 109:38 - 109:41
    than they are, just to impress.
  • 109:41 - 109:45
    When you think of the
    problem, it's a piece of cake.
  • 109:45 - 109:48
    So don't be afraid of it.
  • 109:48 - 110:05
  • 110:05 - 110:17
    Oh, by the way, the final
    exam-- so the midterm would
  • 110:17 - 110:24
    be 10 problems pus 1 extra one.
  • 110:24 - 110:27
  • 110:27 - 110:29
    And did I tell
    you how much time?
  • 110:29 - 110:35
    It's going to be approximately--
    I say, in actual time.
  • 110:35 - 110:35
    Needed time.
  • 110:35 - 110:40
  • 110:40 - 110:44
    For average student,
    it'll be about 40 minutes.
  • 110:44 - 110:53
    Allowed time one
    hour and 40 minutes.
  • 110:53 - 110:58
    So you have from 12:10 to 1:50.
  • 110:58 - 111:01
  • 111:01 - 111:06
    On the final, just a guess,
    about 15-16 problems.
  • 111:06 - 111:10
  • 111:10 - 111:12
    Two hours and a half.
  • 111:12 - 111:16
  • 111:16 - 111:18
    STUDENT: Is that allowed time?
  • 111:18 - 111:21
    PROFESSOR: Not allowed time.
  • 111:21 - 111:25
    If I manage to review very
    well with you on these concepts
  • 111:25 - 111:30
    guys, I guarantee you're not
    going to need more than 1.5.
  • 111:30 - 111:31
    This is the allowed time.
  • 111:31 - 111:34
    The allowed time for somebody
    who hasn't practiced enough.
  • 111:34 - 111:39
  • 111:39 - 111:41
    Let me ask you what you
    think would be good.
  • 111:41 - 111:44
  • 111:44 - 111:46
    I have a bunch of finals.
  • 111:46 - 111:50
    All the finals for Cal 3
    look very similar in nature.
  • 111:50 - 111:54
    The same kind of topics
    as the ones I review.
  • 111:54 - 111:57
    I would like to know
    what you would prefer.
  • 111:57 - 112:03
    I would have two or
    three finals to give you.
  • 112:03 - 112:06
    Would you prefer that you
    try them yourselves first,
  • 112:06 - 112:08
    and then I give
    you the solutions?
  • 112:08 - 112:09
    STUDENT: Yes.
  • 112:09 - 112:11
    PROFESSOR: Or I give you the
    solutions from the beginning?
  • 112:11 - 112:17
    I'll give you the
    solutions anyway, but--
  • 112:17 - 112:19
    STUDENT: Can it just
    be on a separate sheet,
  • 112:19 - 112:21
    where we could go through--
  • 112:21 - 112:24
    PROFESSOR: No, no, they are
    already on a separate sheet.
  • 112:24 - 112:28
    For example, I have Fall
    2013, or Spring 2012.
  • 112:28 - 112:30
    They are from
    different semesters.
  • 112:30 - 112:31
    They are all very similar.
  • 112:31 - 112:35
    So I'll give you-- I have
    two files on this blog.
  • 112:35 - 112:37
    The exam itself
    and the solutions.
  • 112:37 - 112:43
    I'll give you the exam, I'll
    let you work if for two weeks,
  • 112:43 - 112:45
    and then I'll give
    you the solutions.
  • 112:45 - 112:46
    How about that?
  • 112:46 - 112:49
    Put you'll work on it, you
    don't cheat on me and any way.
  • 112:49 - 112:52
    Because working things
    yourself, you're learning.
  • 112:52 - 112:56
    If you expect other people
    to feed you the solutions,
  • 112:56 - 112:58
    you're not learning as much.
  • 112:58 - 113:02
    You are learning some, but
    you're not learning as much.
  • 113:02 - 113:04
    OK, it's getting ready.
  • 113:04 - 113:06
    I have a few more
    things to tell you.
  • 113:06 - 113:20
  • 113:20 - 113:22
    Chapter 13, necessary reminders.
  • 113:22 - 113:31
  • 113:31 - 113:35
    The gradient is very important.
  • 113:35 - 113:46
    Gradient of a function
    f from r 2 to r.
  • 113:46 - 113:52
    We write that as z equals
    f of x and y, usually.
  • 113:52 - 113:53
    And what was the gradient?
  • 113:53 - 113:55
    This is good review
    for the midterm,
  • 113:55 - 113:59
    but that's the beginning
    of section 13.1.
  • 113:59 - 114:01
    So I'm actually
    doing two things,
  • 114:01 - 114:04
    I'm giving you the
    beginning of section 13.1,
  • 114:04 - 114:07
    while doing review
    for the final.
  • 114:07 - 114:12
  • 114:12 - 114:18
    You have gradient of f of x,
    y-- some people are ask me,
  • 114:18 - 114:22
    do you prefer that I
    write on the exams,
  • 114:22 - 114:28
    on the midterm, on the
    final a granular bracket?
  • 114:28 - 114:35
    Or do you prefer I write this in
    this form in the standard base
  • 114:35 - 114:35
    i, j.
  • 114:35 - 114:37
    Standard [INAUDIBLE].
  • 114:37 - 114:39
    It doesn't make a difference.
  • 114:39 - 114:41
    In linear algebra,
    you would have
  • 114:41 - 114:43
    to say what bases you are using.
  • 114:43 - 114:46
    But in calculus, we
    assume that you are using
  • 114:46 - 114:48
    the bases which is 1, 0, 0, 1.
  • 114:48 - 114:51
  • 114:51 - 114:56
    So you have space in a plane.
  • 114:56 - 114:59
    I'm indifferent.
  • 114:59 - 115:02
    This is OK, you can
    use whatever you like.
  • 115:02 - 115:06
    If you have a function of
    three variables, of course
  • 115:06 - 115:07
    you have a gradient.
  • 115:07 - 115:10
  • 115:10 - 115:16
    But I prefer to write f sub x,
    i plus f sub y, j plus f sub z,
  • 115:16 - 115:19
    the beginning of some ck.
  • 115:19 - 115:31
  • 115:31 - 115:34
    Has anybody heard of
    divergence before?
  • 115:34 - 115:36
    What is divergence?
  • 115:36 - 115:38
    Gradient is something
    you've heard before.
  • 115:38 - 115:41
    But divergence, have you
    ever heard of divergence?
  • 115:41 - 115:47
  • 115:47 - 115:59
    Maybe in mechanical engineering,
    have you heard of it before?
  • 115:59 - 116:01
    No?
  • 116:01 - 116:02
    OK.
  • 116:02 - 116:06
    Suppose that you
    have a function,
  • 116:06 - 116:08
    and that is a vector
    value function.
  • 116:08 - 116:13
  • 116:13 - 116:15
    What does it mean?
  • 116:15 - 116:21
    A vector in itself will
    have coordinates at x, y.
  • 116:21 - 116:29
    And it's assumed that
    will be f1 of x, y-- no,
  • 116:29 - 116:31
    this is not a vector,
    that's scalar.
  • 116:31 - 116:35
    Times i, plus f2 x, y, j.
  • 116:35 - 116:39
    And somebody, one of you
    actually showed me-- of course
  • 116:39 - 116:45
    in mechanics-- you were
    using divergence in that.
  • 116:45 - 116:49
    And I feel bad that I was
    not the first maybe for some
  • 116:49 - 116:53
    of you, I was not the first to
    tell you what divergence means.
  • 116:53 - 117:00
    Divergence f, assuming that f
    would be missing one function.
  • 117:00 - 117:02
    What does this mean?
  • 117:02 - 117:06
    It means that it's differential,
    but its derivatives
  • 117:06 - 117:07
    are continuous.
  • 117:07 - 117:10
  • 117:10 - 117:14
    We did note that this
    is the diff of f.
  • 117:14 - 117:18
    But in engineering, they denoted
    most of the time like that.
  • 117:18 - 117:22
    There's not a lot of symbols,
    but you saw the gradient
  • 117:22 - 117:24
    with a little dot after that.
  • 117:24 - 117:30
  • 117:30 - 117:32
    If you don't put the dot,
    it doesn't make sense
  • 117:32 - 117:34
    with what I'm saying.
  • 117:34 - 117:37
    So pay attention to the dot.
  • 117:37 - 117:38
    Alright.
  • 117:38 - 117:39
    What does this mean?
  • 117:39 - 117:44
    It means that you
    have the derivative
  • 117:44 - 117:48
    of the first component
    with respect to x.
  • 117:48 - 117:51
  • 117:51 - 117:55
    Plus it's going to
    be a value function,
  • 117:55 - 117:58
    the derivative of the second
    component with respect to y.
  • 117:58 - 118:04
  • 118:04 - 118:08
    How do you generalize
    for higher powers?
  • 118:08 - 118:18
    What if you have a function--
    assume you have a function
  • 118:18 - 118:20
    f that looks like that.
  • 118:20 - 118:31
    If x1, x2, x n variables,
    i plus the last one will be
  • 118:31 - 118:35
    a [INAUDIBLE] of x1, x2
    x n variables times--
  • 118:35 - 118:40
  • 118:40 - 118:42
    eij doesn't make any sense.
  • 118:42 - 118:47
    So e1, e2, e n would
    be the standard bases.
  • 118:47 - 118:55
    [INAUDIBLE] doesn't
    make the [INAUDIBLE]
  • 118:55 - 119:03
    for a computer scientist,
    an ordered set of components
  • 119:03 - 119:05
    and values.
  • 119:05 - 119:08
    And would be 7, 17, 29.
  • 119:08 - 119:10
    Some natural numbers.
  • 119:10 - 119:19
    So all these values are taken
    in r, with every r x is in on.
  • 119:19 - 119:22
    What do you think that
    the divergence of u
  • 119:22 - 119:24
    would be in that case?
  • 119:24 - 119:28
    If you were to generalize y.
  • 119:28 - 119:33
    First component, prime with
    respect to the first variable.
  • 119:33 - 119:36
    Alright.
  • 119:36 - 119:42
    Only plus second component with
    respect to the second variable,
  • 119:42 - 119:43
    and so on.
  • 119:43 - 119:46
    Last component with respect
    to the last variable.
  • 119:46 - 119:49
    So that would be the
    general definition.
  • 119:49 - 119:58
    And now I'm asking you, assume
    x that somebody gives you
  • 119:58 - 120:03
    a function, f of x, y.
  • 120:03 - 120:05
    And with domain in the plane.
  • 120:05 - 120:10
  • 120:10 - 120:14
    And f is c1.
  • 120:14 - 120:18
    [INAUDIBLE] with
    continuous radius.
  • 120:18 - 120:20
    Actually no, I want more.
  • 120:20 - 120:23
    I want c2.
  • 120:23 - 120:34
    So twice differential bond,
    with continuous variables.
  • 120:34 - 120:39
  • 120:39 - 120:45
    Compute a.
  • 120:45 - 120:46
    Gradient double f.
  • 120:46 - 120:49
  • 120:49 - 120:54
    b, divergence of gradient
    of f, which you can also
  • 120:54 - 121:00
    write divergence like engineers
    do, or gradient to our left.
  • 121:00 - 121:08
    Do you know what name that's
    the last thing we need today,
  • 121:08 - 121:15
    the name for this operator.
  • 121:15 - 121:16
    Underlined here.
  • 121:16 - 121:22
  • 121:22 - 121:25
    So what would be a good
    name for this kind?
  • 121:25 - 121:29
    I'm curious if any of you
    know if from engineering.
  • 121:29 - 121:31
    But we will see.
  • 121:31 - 121:40
  • 121:40 - 121:44
    So we are in 13.
  • 121:44 - 121:51
    a will be the gradient of
    f, that's a piece of cake.
  • 121:51 - 121:52
    She only wants the
    definition, let
  • 121:52 - 121:58
    me give her the definition
    of f sub xi, plus f sub y j.
  • 121:58 - 121:59
    And if we don't
    know what those are,
  • 121:59 - 122:02
    this is the variable
    with respect to x.
  • 122:02 - 122:08
    And then for dy, df/dy j.
  • 122:08 - 122:08
    Good.
  • 122:08 - 122:12
    So we know what a gradient is.
  • 122:12 - 122:15
    What will this divergence
    with the gradient be?
  • 122:15 - 122:17
    That sounds really weird.
  • 122:17 - 122:22
  • 122:22 - 122:25
    According to this
    definition, we have
  • 122:25 - 122:30
    to see what big
    F1 and big F2 are.
  • 122:30 - 122:33
    Or, big F1 and big F2.
  • 122:33 - 122:36
    I'm going to take
    them in breaths.
  • 122:36 - 122:39
    Big F1, and big F2.
  • 122:39 - 122:42
  • 122:42 - 122:48
    The components of the vector,
    you apply divergence to it.
  • 122:48 - 122:50
    So now that I'm finishing,
    what do I have to do?
  • 122:50 - 122:53
    Somebody tell me.
  • 122:53 - 122:58
    So yeah, I can write it
    f sub x plus f sub y,
  • 122:58 - 123:03
    and that shows that you are
    fast, and very [INAUDIBLE].
  • 123:03 - 123:06
    I can also write
    it like this, which
  • 123:06 - 123:11
    is what I meant-- this is what
    the book shows first course.
  • 123:11 - 123:13
    This is the same thing.
  • 123:13 - 123:15
  • 123:15 - 123:21
    Now I really doubt that
    somebody knows that,
  • 123:21 - 123:25
    but I want to give a
    dollar to the person who
  • 123:25 - 123:27
    would know the name of this.
  • 123:27 - 123:30
  • 123:30 - 123:33
    Let me see if I have a dollar.
  • 123:33 - 123:38
  • 123:38 - 123:41
    Maybe I have $0.35 and a candy.
  • 123:41 - 123:44
    Does anybody know
    the name of this?
  • 123:44 - 123:55
    Maybe I can help you a little
    bit. $0.25 $0.85, $0.95.
  • 123:55 - 123:57
    Do you know what this is?
  • 123:57 - 124:01
    I'll give you a hint, because I
    know in mechanical engineering,
  • 124:01 - 124:03
    I already introduced this.
  • 124:03 - 124:09
    And some physics classes and
    we would try angle in front,
  • 124:09 - 124:15
    and we did all of this
    triangle operators in the way.
  • 124:15 - 124:19
    And we can play a game.
  • 124:19 - 124:27
    It's a letter that
    starts with L.
  • 124:27 - 124:30
    But $0.95 we have
    two more minutes.
  • 124:30 - 124:33
    STUDENT: [INAUDIBLE]?
  • 124:33 - 124:33
    PROFESSOR: No.
  • 124:33 - 124:38
    You are getting close though,
    because-- [INTERPOSING VOICES]
  • 124:38 - 124:41
    What kind of operator is this?
  • 124:41 - 124:44
    You're getting close, $0.95.
  • 124:44 - 124:46
    Tomorrow, I don't need this.
  • 124:46 - 124:48
    When I go to the
    airports, I don't
  • 124:48 - 124:49
    like to have coins with me.
  • 124:49 - 124:57
  • 124:57 - 124:59
    STUDENT: Laplace?
  • 124:59 - 125:00
    PROFESSOR: $0.95!
  • 125:00 - 125:02
    I wish I had a dollar.
  • 125:02 - 125:05
    Yes, this is the famous
    Laplace operator.
  • 125:05 - 125:06
    Laplace was a mathematician.
  • 125:06 - 125:12
  • 125:12 - 125:14
    And remember it.
  • 125:14 - 125:17
    If you take-- how
    many of you-- you all
  • 125:17 - 125:20
    have to take differential
    equations, right?
  • 125:20 - 125:22
    They will kill you with that.
  • 125:22 - 125:24
    You're going to see
    this all the time.
  • 125:24 - 125:26
    This Laplace operator
    is really famous.
  • 125:26 - 125:29
  • 125:29 - 125:31
    I will tell you more
    when I come back.
  • 125:31 - 125:35
    I'm going to see you on Tuesday.
  • 125:35 - 125:37
    We'll knock out the midterm.
  • 125:37 - 125:41
    For you, the people who feel
    overly prepared for midterm
  • 125:41 - 125:46
    can go ahead and
    read section 13.1
  • 125:46 - 125:49
    and see a little bit
    about Laplace's operator.
  • 125:49 - 125:51
    [INTERPOSING VOICES]
  • 125:51 - 126:46
Title:
TTU Math2450 Calculus3 chap. 10-11-12 review
Description:

Exam review

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Video Language:
English

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