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5DUQ3-Y_gX4
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So we'll call it a
vector space as well.
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5DUQ3-Y_gX4
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STEVEN G. JOHNSON: Yeah.
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5DUQ3-Y_gX4
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But it's incredibly
useful, though.
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Because very often, especially
in physical sciences,
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you have something where
conceptually you're
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solving for a functions.
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5DUQ3-Y_gX4
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So you're solving for the
fluid flow or something
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around an airplane wing.
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5DUQ3-Y_gX4
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And what you want is that
then take that fluid flow
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5DUQ3-Y_gX4
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and compute the drag
on the airplane wing.
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5DUQ3-Y_gX4
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And then in order
to optimize it,
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you want the derivative
of the drag with respect
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to that flow field, with
respect to the function,
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or with respect to the
shape of the airplane, which
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5DUQ3-Y_gX4
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is a function.
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5DUQ3-Y_gX4
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So it's very, very nice to
be able to take derivatives
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5DUQ3-Y_gX4
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connected to functions and
work with vector functions
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as vector spaces.
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5DUQ3-Y_gX4
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And very soon we're going
to be able to do that
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5DUQ3-Y_gX4
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with this notion
of a derivative.
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5DUQ3-Y_gX4
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Because we're going to be able
to define linear operators,
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5DUQ3-Y_gX4
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functions that act on functions.
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5DUQ3-Y_gX4
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And linear operators
are functions.
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5DUQ3-Y_gX4
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But that's getting a bit
too far ahead of ourselves.
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5DUQ3-Y_gX4
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OK.
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5DUQ3-Y_gX4
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So the point is that
the 18.01-- so far, we
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5DUQ3-Y_gX4
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haven't done any derivatives
more than 18.01, at least
|
5DUQ3-Y_gX4
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in my half.
|
5DUQ3-Y_gX4
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Alan went a bit further.
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5DUQ3-Y_gX4
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But already we can start
to see, hopefully, how
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5DUQ3-Y_gX4
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this is going to generalize.
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5DUQ3-Y_gX4
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So if you have a
function f of x and you
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5DUQ3-Y_gX4
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make a small change
in the input, delta x,
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5DUQ3-Y_gX4
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and you ask for the small
change in the output
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5DUQ3-Y_gX4
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to first order, which we can
denote with this d notation,
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5DUQ3-Y_gX4
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the derivative is
the linear operator
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5DUQ3-Y_gX4
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that gives us that,
the linearization
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5DUQ3-Y_gX4
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of that function for a
small change in the input.
|
5DUQ3-Y_gX4
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And that is exactly equivalent
to what you learned in 18.01.
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5DUQ3-Y_gX4
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But it's going to be easier
now to generalize this
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5DUQ3-Y_gX4
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to other kinds of inputs
and other kinds of outputs,
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5DUQ3-Y_gX4
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where, in 18.01, we move this to
the side where we take df, dx.
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5DUQ3-Y_gX4
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We divide them.
|
5DUQ3-Y_gX4
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For numbers, that's fine.
|
5DUQ3-Y_gX4
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For other kinds of things, that
becomes a little bit weirder
|
5DUQ3-Y_gX4
|
to talk about.
|
5DUQ3-Y_gX4
|
Of course, you could
define it as notation.
|
5DUQ3-Y_gX4
|
But I think it's a
lot clearer if you
|
5DUQ3-Y_gX4
|
think of it in this sense
once you start generalizing
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5DUQ3-Y_gX4
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to other kinds of objects.
|
5DUQ3-Y_gX4
|
So with that said,
let's do that.
|
5DUQ3-Y_gX4
|
Now, let's revisit 18.02.
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5DUQ3-Y_gX4
|
And let me do it in two parts.
|
5DUQ3-Y_gX4
|
So part one is going
to be functions--
|
5DUQ3-Y_gX4
|
the first thing you
usually do in 18.02,
|
5DUQ3-Y_gX4
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which is functions that take a
vector in or multiple variables
|
5DUQ3-Y_gX4
|
in.
|
5DUQ3-Y_gX4
|
But we'll think of it as a
vector in and a scalar out.
|
5DUQ3-Y_gX4
|
So we're going to have a scalar.
|
5DUQ3-Y_gX4
|
My output is blue, right?
|
5DUQ3-Y_gX4
|
Yes.
|
5DUQ3-Y_gX4
|
We'll keep the same
color scheme, good.
|
5DUQ3-Y_gX4
|
So we're going to have a scalar
function f of a vector input x.
|
5DUQ3-Y_gX4
|
And I'll put a little
vector sign above it.
|
5DUQ3-Y_gX4
|
I won't always do that, but
it's nice to be clear sometimes,
|
5DUQ3-Y_gX4
|
which is a vector,
which is a scalar.
|
5DUQ3-Y_gX4
|
So x is going to live in our m.
|
5DUQ3-Y_gX4
|
So this is going to be an
m component column vector.
|
5DUQ3-Y_gX4
|
OK.
|
5DUQ3-Y_gX4
|
And what we want
to do is imagine
|
5DUQ3-Y_gX4
|
what happens to the
output when you change
|
5DUQ3-Y_gX4
|
the input by a little bit.
|
5DUQ3-Y_gX4
|
So we're going to
take f of x plus dx.
|
5DUQ3-Y_gX4
|
Think of this as a
really small change.
|
5DUQ3-Y_gX4
|
It's infinitesimal.
|
5DUQ3-Y_gX4
|
We're going to
drop anything that
|
5DUQ3-Y_gX4
|
goes like dx squared or anything
like that, any higher terms.
|
5DUQ3-Y_gX4
|
Let me just move
it to [INAUDIBLE]..
|
5DUQ3-Y_gX4
|
It's black-- minus f of x.
|
5DUQ3-Y_gX4
|
And we're going to define
this as f prime of x dx.
|
5DUQ3-Y_gX4
|
So we wanted to note we have an
arbitrary change in the inputs.
|
5DUQ3-Y_gX4
|
dx is an arbitrary,
very, very small vector.
|
5DUQ3-Y_gX4
|
And we want to ask, what's
the change in the output
|
5DUQ3-Y_gX4
|
differential, df?
|
5DUQ3-Y_gX4
|
And the answer is
going to be that this
|
5DUQ3-Y_gX4
|
is going to be, for
a very small dx,
|
5DUQ3-Y_gX4
|
we can approximate this by
a linear operator on dx.
|
5DUQ3-Y_gX4
|
So this is going to be a
linear operator, always
|
5DUQ3-Y_gX4
|
going to be a linear operator.
|
5DUQ3-Y_gX4
|
And what is that
linear operator do?
|
5DUQ3-Y_gX4
|
This one takes a vector
in and gives you a scalar.
|
5DUQ3-Y_gX4
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So this has to equal a--
|
5DUQ3-Y_gX4
|
df is a scalar,
but dx is a vector.
|
5DUQ3-Y_gX4
|
So what this has to be is it
has to be kind of a row vector.
|
5DUQ3-Y_gX4
|
You can think of it more
as a one-row matrix.
|
5DUQ3-Y_gX4
|
Or there's fancier names
for this, like covector
|
5DUQ3-Y_gX4
|
or dual vector.
|
5DUQ3-Y_gX4
|
We won't really use that.
|
5DUQ3-Y_gX4
|
I just want to throw
them out there.
|
5DUQ3-Y_gX4
|
So if you want to take a vector
in and take a vector out,
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