WEBVTT

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TOBIAS COLDING: OK, so last
time, we talked about--

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so we had a function or
sequence of function.

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We had an integral, say,
I, and we had a sequence

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of function fn and a function
f all defined on this interval.

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And then we talked about
pointwise convergence.

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So pointwise convergence
means that for each--

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so this is for each x when
you're looking at this.

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So this is for each x fixed.

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This is a sequence.

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This is supposed to
convert to f of x.

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So this was pointwise
convergence.

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And then we also talked
about uniform convergence.

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And this meant that for
all epsilon greater than 0,

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there exists a capital N such
that if little n is bigger

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or equal to this capital N,
then the difference between fn

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of x and f of x, this here,
is smaller than epsilon,

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and this here have
to hold for all x.

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So uniform, again, refer
to that as uniform in x.

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The convergence is uniform in x.

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Then so we talk about that.

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And then one of the
theorems we proved

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was that if you take a
sequence, fn and [INAUDIBLE]

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was integrable, and these
converge to some function

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f, then f is integrable.

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So this is uniform convergence.

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Then f here is integrable
and the integral

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is the limit of the integrals.

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So the integral
from a to b of fn

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x dx is equal as the
limit here of this.

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So the limit exists and it is
equal to the integral of f.

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So this is how uniform
convergence and integrals

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interact.

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Suppose you take
a sequence here.

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So this is a theorem.

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Suppose you take a sequence fn
of functions on some interval

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into R. You have x0
is in this interval.

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And then you have
the following if you

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have the following
properties, that one

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is that this sequence here
converged to some number C.

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So the sequence converged
to some number c.

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Two is that these functions
here, fn, are differentiable.

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So these are maybe, I'll just
say here, differentiable.

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And these here converge
to some function g.

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And then 3 is that
these functions here--

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sorry the derivative
converge, and I'm also

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requiring that the
derivative are continuous.

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Suppose we have
these three things.

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So we have the sequence of
differentiable functions.

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If you just fix this
one particular point,

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x0, then the values of
these functions converge.

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And then the functions--
their derivatives

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are continuous, and the
derivative converges

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to some function.

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And this convergence
here is uniform.

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Then the claim is that then
there exists f on the interval

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so that f is differentiable.

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The derivative
here is continuous.

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And you have the
following two properties

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that the function here--

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these functions
converge to f uniformly.

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I'm going to restrict
my interval, which

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would take it just to be
some interval from A to B.

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And I want it to be
bounded, like that.

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And so these converge
uniformly, and two

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is that their derivative
converges to the derivative of f

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uniformly.

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So we want to prove that.

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And then so we're going
to define a function f.

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So g here is a proof of this.

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Since this sequence here--

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since these are continuous
and these functions here

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convert to g uniformly,
then this means that then,

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therefore, g here
is also continuous.

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So we proved this
already, that if you

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have a sequence of
continuous function

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that converges uniformly, then
the limit is also continuous.

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And so then we can look
at-- so we can therefore

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define f as a function on this
interval here by that f of x

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is equal to the
integral from x0.

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So I'm defining it,
sorry, to be the c

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constant, c plus the integral
from 0 to x of g of x, g of s

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ds.

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So I define this
function like this.

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g is continuous, so this is
a nice continuous function.

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And in fact, by the fundamental
theorem of calculus,

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f here is differentiable with
the derivative equal to g.

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We also have that
we also have that

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if we're looking at
f of x0, fn of x0,

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then we know already
that these converts to c.

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This is the assumption
one up there.

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But this here is the
value of f at x0.

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So we have that.

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I want to now prove that
not just at this point

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but that this sequence
converges to f uniformly.

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b we get for free.

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So b follows from that this
fn prime converges to g.

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And this here is
the derivative of f.

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And we have this uniformly
by assumption two.

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So all we need to
show is-- so we just

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need to show that each fn
converges to f uniformly.

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We just need to show
that the property a--

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and so we're looking at fn of x.

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We have to look at
this difference.

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And for a given epsilon we
have to find at little n.

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So we have to find
a capital N so

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that if little n is bigger
than this capital N,

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then this difference here is
smaller than epsilon for all x.

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But let's try to
estimate this here first.

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So this difference is f.

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So we want to estimate
this difference.

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And we can use the fundamental
theorem of calculus

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or use the fundamental theorem
of calculus to write f of x.

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We can write this
as the value at x0

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plus the integral of the
derivative from this point.

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And then this should
be less like this.

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We can use the fundamental
theorem of calculus

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to just rewrite fn like that.

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And so now I want to look
at this difference here.

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And so to look at
this difference

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fn of dx minus f of x, now I
can fill in this form of it.

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So I have that this is f of
x0 plus the integral from x0

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to f prime s ds.

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And then I have to
subtract f of x.

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But f of x was given
by this formula here,

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and so minus c plus this
integral here, g of s ds,

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like that.

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And so now I'm just
rearranging terms.

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So I just think about this
thing here as fn of x0 minus c.

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I take these two first, and
then plus the integral of x0

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to x f prime n s ds minus
this integral here, like that.

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And then I use the
triangle inequality

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that this thing here is
less than fn of x minus c--

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sorry fn of x0 minus c,
absolute value, like this.

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And then I have the
second integral here.

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So the absolute value
or the difference

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here, if you do it
slowly like this,

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so you have this minus this in
here of g of s ds, like that.

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Now I can think about this thing
here as I can find the integral,

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so I can write this
thing here as--

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so I'm just keeping
this first term here.

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And then the second
here I can think

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about this as integral of the
difference of this function.

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And this here was an
n here, like that.

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So now, here, I can just
take the absolute value sign.

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If I take the value
I and under it, then

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I get something
potentially larger.

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So this thing here is
less than or equal to f

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of x minus 0 minus c.

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That's the first term.

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And now I'm replacing
it by something

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that is bigger or equal to this,
so where I'm just integrating

00:16:09.030 --> 00:16:15.710 align:middle line:84%
from x0 to x, and then
of this difference here,

00:16:15.710 --> 00:16:21.580 align:middle line:90%
f prime s minus g of s ds.

00:16:21.580 --> 00:16:24.230 align:middle line:90%


00:16:24.230 --> 00:16:28.970 align:middle line:90%
And now I'm using that the fn--

00:16:28.970 --> 00:16:41.330 align:middle line:90%


00:16:41.330 --> 00:16:46.650 align:middle line:84%
so actually, let me just
write this thing here.

00:16:46.650 --> 00:16:48.430 align:middle line:90%
So I can write this thing here.

00:16:48.430 --> 00:16:51.390 align:middle line:90%
This one here, I'm keeping.

00:16:51.390 --> 00:16:52.930 align:middle line:90%
This one here, I'm keeping.

00:16:52.930 --> 00:16:55.950 align:middle line:84%
So I'm writing this as less
than or equal to keeping

00:16:55.950 --> 00:16:56.640 align:middle line:90%
the first term.

00:16:56.640 --> 00:17:00.190 align:middle line:90%


00:17:00.190 --> 00:17:02.830 align:middle line:84%
And the second term,
you see, this thing

00:17:02.830 --> 00:17:08.230 align:middle line:84%
here is this difference
between these two.

00:17:08.230 --> 00:17:13.710 align:middle line:84%
Well, the difference
is at some s is smaller

00:17:13.710 --> 00:17:17.470 align:middle line:90%
than the maximum for all s.

00:17:17.470 --> 00:17:19.829 align:middle line:84%
But the maximum
for all s, that's

00:17:19.829 --> 00:17:25.990 align:middle line:90%
what we call d fn prime g.

00:17:25.990 --> 00:17:28.470 align:middle line:90%
That was the maximum over all s.

00:17:28.470 --> 00:17:32.110 align:middle line:84%
And so now we just have--
so this function in here

00:17:32.110 --> 00:17:33.590 align:middle line:90%
is less than this.

00:17:33.590 --> 00:17:35.590 align:middle line:84%
And now we are
using-- this is where

00:17:35.590 --> 00:17:38.390 align:middle line:84%
I want to use that the
interval is bounded.

00:17:38.390 --> 00:17:40.750 align:middle line:90%
So I just get plus b minus a.

00:17:40.750 --> 00:17:45.470 align:middle line:84%
This is the length of
the interval, like that.

00:17:45.470 --> 00:17:50.110 align:middle line:90%
And so now you see that s--

00:17:50.110 --> 00:17:53.970 align:middle line:84%
and now there's no
reference to x on this side.

00:17:53.970 --> 00:17:58.550 align:middle line:84%
And so you see that,
as n goes to infinity,

00:17:58.550 --> 00:18:02.390 align:middle line:84%
well, this thing here goes
to 0 and this thing here

00:18:02.390 --> 00:18:14.680 align:middle line:84%
goes to 0, so as this
upper bound goes to 0.

00:18:14.680 --> 00:18:18.790 align:middle line:90%


00:18:18.790 --> 00:18:23.050 align:middle line:84%
And again, note that
there's no reference to x.

00:18:23.050 --> 00:18:24.730 align:middle line:90%
There's a reference to x0.

00:18:24.730 --> 00:18:26.490 align:middle line:84%
But that's just
some fixed point.

00:18:26.490 --> 00:18:29.990 align:middle line:90%
So this is uniform in x.

00:18:29.990 --> 00:18:42.530 align:middle line:84%
So this implies
uniform in x converges.

00:18:42.530 --> 00:18:46.710 align:middle line:90%


00:18:46.710 --> 00:18:55.750 align:middle line:84%
And so I want to draw
some consequences of this.

00:18:55.750 --> 00:18:59.550 align:middle line:84%
First, let me look
at what will be,

00:18:59.550 --> 00:19:07.430 align:middle line:84%
shortly, a particular case
of a more general phenomenon.

00:19:07.430 --> 00:19:17.590 align:middle line:84%
So this example we looked
at several times last time.

00:19:17.590 --> 00:19:21.010 align:middle line:84%
But it's now applied
in this case here.

00:19:21.010 --> 00:19:26.310 align:middle line:90%


00:19:26.310 --> 00:19:33.310 align:middle line:84%
So suppose you're looking
at the functions En of x.

00:19:33.310 --> 00:19:37.190 align:middle line:84%
The En is where
you're summing from k

00:19:37.190 --> 00:19:44.050 align:middle line:84%
equal to 0 to n of x to the
power k divided by k factorial.

00:19:44.050 --> 00:19:46.790 align:middle line:84%
I looked at those last
time, these functions.

00:19:46.790 --> 00:19:50.230 align:middle line:90%
And we call them En.

00:19:50.230 --> 00:19:56.670 align:middle line:84%
And then we also looked at
the exponential function

00:19:56.670 --> 00:20:01.550 align:middle line:84%
and the exponential function
in terms of power series.

00:20:01.550 --> 00:20:03.710 align:middle line:90%
That was just this power series.

00:20:03.710 --> 00:20:07.630 align:middle line:90%


00:20:07.630 --> 00:20:18.150 align:middle line:84%
And we have that we have that
En here so that for all--

00:20:18.150 --> 00:20:21.350 align:middle line:90%
we used Weinstrass M-test to--

00:20:21.350 --> 00:20:37.150 align:middle line:84%
so by Weinstrass
M-test for all L--

00:20:37.150 --> 00:20:40.140 align:middle line:90%
L is a positive real number--

00:20:40.140 --> 00:20:44.150 align:middle line:90%


00:20:44.150 --> 00:20:53.710 align:middle line:84%
we had that these functions
converge to E uniformly

00:20:53.710 --> 00:20:57.430 align:middle line:90%
on an interval like this.

00:20:57.430 --> 00:20:59.990 align:middle line:84%
They don't necessarily--
in fact, they don't.

00:20:59.990 --> 00:21:05.870 align:middle line:84%
But the claim here about
uniform convergence

00:21:05.870 --> 00:21:08.990 align:middle line:84%
is just on every
bounded interval.

00:21:08.990 --> 00:21:11.830 align:middle line:84%
So you fix a bounded
interval like that interval,

00:21:11.830 --> 00:21:13.610 align:middle line:84%
and then you have
uniform convergence.

00:21:13.610 --> 00:21:15.110 align:middle line:84%
It's not like
uniform convergence

00:21:15.110 --> 00:21:19.070 align:middle line:90%
of all of R at the same time.

00:21:19.070 --> 00:21:26.850 align:middle line:84%
So we have that, and now
if we are looking at--

00:21:26.850 --> 00:21:32.530 align:middle line:84%
so now if we're looking
at the function--

00:21:32.530 --> 00:21:38.230 align:middle line:90%


00:21:38.230 --> 00:21:42.510 align:middle line:84%
if we take now the
derivative of the En's--

00:21:42.510 --> 00:21:44.600 align:middle line:84%
so what is the
derivative of the En's?

00:21:44.600 --> 00:21:50.470 align:middle line:90%


00:21:50.470 --> 00:21:53.110 align:middle line:90%
So the derivative of the En--

00:21:53.110 --> 00:21:55.470 align:middle line:90%
but the En is just a polynomial.

00:21:55.470 --> 00:22:00.790 align:middle line:84%
So you can just differentiate
each term on its own.

00:22:00.790 --> 00:22:15.190 align:middle line:84%
So this here is the sum here
of x to the power k minus 1

00:22:15.190 --> 00:22:19.030 align:middle line:90%
divided by k factorial.

00:22:19.030 --> 00:22:24.310 align:middle line:84%
And here, you would be summing
from k equal to 0 to n.

00:22:24.310 --> 00:22:28.870 align:middle line:90%


00:22:28.870 --> 00:22:34.310 align:middle line:90%
And now I can write this also.

00:22:34.310 --> 00:22:39.230 align:middle line:84%
You see, because
when k is equal to 0,

00:22:39.230 --> 00:22:41.270 align:middle line:84%
the first term
doesn't really count.

00:22:41.270 --> 00:22:44.710 align:middle line:84%
So this thing here,
I can write as--

00:22:44.710 --> 00:22:47.710 align:middle line:84%
I mean, it doesn't
count because it's 0.

00:22:47.710 --> 00:22:50.270 align:middle line:84%
So you don't really
need to write that term.

00:22:50.270 --> 00:22:54.030 align:middle line:84%
So you can just write it
from k equal to 1 to n.

00:22:54.030 --> 00:23:00.030 align:middle line:84%
And then you can write it
again as k times x to the power

00:23:00.030 --> 00:23:04.510 align:middle line:90%
k minus 1 over k factorial.

00:23:04.510 --> 00:23:11.350 align:middle line:90%
But k factorial is just--

00:23:11.350 --> 00:23:19.830 align:middle line:84%
it's the same as k times
k minus 1 factorial.

00:23:19.830 --> 00:23:25.350 align:middle line:84%
So this means that
k factorial over k

00:23:25.350 --> 00:23:29.440 align:middle line:84%
is just the same as
k minus 1 factorial.

00:23:29.440 --> 00:23:32.030 align:middle line:90%


00:23:32.030 --> 00:23:36.710 align:middle line:84%
Or, if you will, if I
take the inverse of this,

00:23:36.710 --> 00:23:45.210 align:middle line:84%
k over k factorial is the same
as 1 over k minus 1 factorial.

00:23:45.210 --> 00:23:50.350 align:middle line:84%
It's just flipping the
denominator and the denominator.

00:23:50.350 --> 00:23:57.170 align:middle line:84%
So this finite sum I can
write as k equal to 1 to n

00:23:57.170 --> 00:24:00.990 align:middle line:84%
because you see, this
thing here is exactly this.

00:24:00.990 --> 00:24:02.810 align:middle line:90%
So we can just replace it.

00:24:02.810 --> 00:24:07.870 align:middle line:90%


00:24:07.870 --> 00:24:09.090 align:middle line:90%
You can write it like that.

00:24:09.090 --> 00:24:14.390 align:middle line:90%


00:24:14.390 --> 00:24:21.670 align:middle line:84%
But now this thing here,
I'm summing from 1 to n.

00:24:21.670 --> 00:24:26.270 align:middle line:84%
The first term, I
get that is just this

00:24:26.270 --> 00:24:30.150 align:middle line:84%
here by definition
when k is equal to 1.

00:24:30.150 --> 00:24:31.390 align:middle line:90%
That's 0 factorial.

00:24:31.390 --> 00:24:35.350 align:middle line:84%
0 factorial, by
definition, is 1.

00:24:35.350 --> 00:24:38.070 align:middle line:84%
So this thing here
and this thing here,

00:24:38.070 --> 00:24:40.910 align:middle line:90%
by definition, is also 1.

00:24:40.910 --> 00:24:42.330 align:middle line:90%
So this is just 1.

00:24:42.330 --> 00:24:48.710 align:middle line:84%
So starting off at 1, when k is
equal to 2, then this becomes x.

00:24:48.710 --> 00:24:50.670 align:middle line:90%
This will become 1 factorial.

00:24:50.670 --> 00:24:52.790 align:middle line:90%
1 factorial is 1.

00:24:52.790 --> 00:24:54.190 align:middle line:90%
So this here is x.

00:24:54.190 --> 00:24:57.470 align:middle line:90%
So this here is like this x.

00:24:57.470 --> 00:25:04.190 align:middle line:84%
The next one, when k is equal
to 3, then you get x squared.

00:25:04.190 --> 00:25:05.690 align:middle line:90%
So you get x squared.

00:25:05.690 --> 00:25:09.570 align:middle line:84%
And down here, you
get 2 factorial.

00:25:09.570 --> 00:25:11.770 align:middle line:90%
And so you continue like this.

00:25:11.770 --> 00:25:17.470 align:middle line:84%
And the last one you get is x
to the power n minus 1 over n

00:25:17.470 --> 00:25:20.050 align:middle line:90%
minus 1 factorial.

00:25:20.050 --> 00:25:22.830 align:middle line:90%


00:25:22.830 --> 00:25:25.210 align:middle line:90%
Let me just say--

00:25:25.210 --> 00:25:32.134 align:middle line:84%
so you see that this thing here
is nothing but En minus 1 of x.

00:25:32.134 --> 00:25:35.950 align:middle line:90%


00:25:35.950 --> 00:25:45.030 align:middle line:84%
So the derivative of the En is
the previous element En minus 1.

00:25:45.030 --> 00:25:45.896 align:middle line:90%
Yeah?

00:25:45.896 --> 00:25:46.670 align:middle line:84%
AUDIENCE: I think
that cleared it up.

00:25:46.670 --> 00:25:47.462 align:middle line:90%
TOBIAS COLDING: OK.

00:25:47.462 --> 00:25:54.060 align:middle line:90%


00:25:54.060 --> 00:26:15.710 align:middle line:84%
So now we have that these En,
if I'm looking at the En, is 0.

00:26:15.710 --> 00:26:18.310 align:middle line:90%


00:26:18.310 --> 00:26:21.670 align:middle line:90%
The value here of these guys--

00:26:21.670 --> 00:26:27.230 align:middle line:84%
the only term that matters is
the first term, and that's 1.

00:26:27.230 --> 00:26:28.770 align:middle line:90%
So this here for each n.

00:26:28.770 --> 00:26:37.830 align:middle line:90%


00:26:37.830 --> 00:26:39.830 align:middle line:90%
So now what you have is--

00:26:39.830 --> 00:26:43.430 align:middle line:84%
so now we have that
you have that if you're

00:26:43.430 --> 00:26:47.150 align:middle line:84%
looking at this
sequence, you have this.

00:26:47.150 --> 00:26:54.830 align:middle line:84%
We have that the En prime
is equal to En minus 1.

00:26:54.830 --> 00:26:57.090 align:middle line:84%
And we already proved
that these here--

00:26:57.090 --> 00:26:58.590 align:middle line:84%
and it doesn't
matter whether you're

00:26:58.590 --> 00:27:00.150 align:middle line:90%
looking at the previous one--

00:27:00.150 --> 00:27:03.910 align:middle line:84%
that they converge
to E uniformly.

00:27:03.910 --> 00:27:14.850 align:middle line:84%
This is a uniform convergence
on this interval here.

00:27:14.850 --> 00:27:18.550 align:middle line:90%


00:27:18.550 --> 00:27:21.230 align:middle line:90%
And then obviously, 3--

00:27:21.230 --> 00:27:24.430 align:middle line:84%
obviously, the En
prime here, they

00:27:24.430 --> 00:27:32.976 align:middle line:90%
are polynomial, so continuous.

00:27:32.976 --> 00:27:47.150 align:middle line:90%


00:27:47.150 --> 00:28:01.030 align:middle line:84%
So therefore, by
the theorem, there

00:28:01.030 --> 00:28:05.110 align:middle line:84%
exists some function
f So that these are

00:28:05.110 --> 00:28:07.830 align:middle line:90%
converged to this uniformly.

00:28:07.830 --> 00:28:08.980 align:middle line:90%
That's no great surprise.

00:28:08.980 --> 00:28:13.190 align:middle line:90%


00:28:13.190 --> 00:28:17.950 align:middle line:84%
And we also have
that this thing here,

00:28:17.950 --> 00:28:22.150 align:middle line:84%
the derivative converges
to the derivative of this

00:28:22.150 --> 00:28:26.350 align:middle line:90%
here uniformly.

00:28:26.350 --> 00:28:29.100 align:middle line:84%
And again, this is on
integrals of this form.

00:28:29.100 --> 00:28:32.310 align:middle line:90%


00:28:32.310 --> 00:28:39.910 align:middle line:84%
Well, we already know that
it converges uniformly.

00:28:39.910 --> 00:28:42.670 align:middle line:90%
This is just by--

00:28:42.670 --> 00:28:44.930 align:middle line:84%
I mean, it can only
converge to one function

00:28:44.930 --> 00:28:46.790 align:middle line:84%
because uniform
convergence means

00:28:46.790 --> 00:28:50.030 align:middle line:84%
that it's converging
pointwise at each x

00:28:50.030 --> 00:28:55.270 align:middle line:84%
and pointwise convergence, then
the limit is just one thing.

00:28:55.270 --> 00:28:59.990 align:middle line:84%
So we already know that
this here is E of x.

00:28:59.990 --> 00:29:02.390 align:middle line:84%
So you see that the
conclusion here we

00:29:02.390 --> 00:29:15.670 align:middle line:84%
get is now that this and this
here is, as we said, En minus 1.

00:29:15.670 --> 00:29:20.310 align:middle line:84%
So the conclusion that
we get is that the E--

00:29:20.310 --> 00:29:24.510 align:middle line:84%
so this is the conclusion
from the theorem up there--

00:29:24.510 --> 00:29:33.302 align:middle line:84%
that these En minus 1 converge
uniformly to the derivative

00:29:33.302 --> 00:29:34.010 align:middle line:90%
of this function.

00:29:34.010 --> 00:29:39.870 align:middle line:90%


00:29:39.870 --> 00:29:46.750 align:middle line:84%
The theorem said that if you
have these three conditions,

00:29:46.750 --> 00:29:52.470 align:middle line:84%
then there exists a function
f that is differentiable

00:29:52.470 --> 00:29:55.350 align:middle line:84%
and the derivative
of it is continuous.

00:29:55.350 --> 00:29:57.870 align:middle line:84%
And you have these
two properties.

00:29:57.870 --> 00:30:01.470 align:middle line:84%
But we already know that
these converge to this.

00:30:01.470 --> 00:30:04.750 align:middle line:84%
So we've already identified
what this function is.

00:30:04.750 --> 00:30:08.310 align:middle line:84%
So the theorem just gave
us that this function

00:30:08.310 --> 00:30:14.350 align:middle line:84%
must be differentiable and
the derivative continuous.

00:30:14.350 --> 00:30:18.350 align:middle line:84%
And now we try to figure
out what that derivative is.

00:30:18.350 --> 00:30:21.070 align:middle line:84%
But the derivative
of these functions

00:30:21.070 --> 00:30:25.030 align:middle line:84%
are the same functions we
started with, but just shifted

00:30:25.030 --> 00:30:26.550 align:middle line:90%
one backwards.

00:30:26.550 --> 00:30:33.610 align:middle line:84%
So these here, also,
they converge to this.

00:30:33.610 --> 00:30:35.270 align:middle line:90%
That's what the theorem say.

00:30:35.270 --> 00:30:45.510 align:middle line:84%
But the En minus 1,
they also converge to E.

00:30:45.510 --> 00:30:50.910 align:middle line:84%
So this means that these two
functions here, this here,

00:30:50.910 --> 00:30:54.670 align:middle line:90%
and this here must be the same.

00:30:54.670 --> 00:30:59.350 align:middle line:84%
So this means that
E is differentiable

00:30:59.350 --> 00:31:02.550 align:middle line:90%
and the derivative is itself.

00:31:02.550 --> 00:31:04.030 align:middle line:90%
Yeah?

00:31:04.030 --> 00:31:07.910 align:middle line:84%
AUDIENCE: So we defined this
for all n greater than sum--

00:31:07.910 --> 00:31:10.770 align:middle line:84%
TOBIAS COLDING: This
here was for all--

00:31:10.770 --> 00:31:15.190 align:middle line:84%
this here was defined for
any nonnegative integer.

00:31:15.190 --> 00:31:26.020 align:middle line:90%


00:31:26.020 --> 00:31:31.320 align:middle line:84%
And so I mean, when I'm
talking about down here,

00:31:31.320 --> 00:31:33.420 align:middle line:84%
then I'm thinking about
n bigger or equal to 1

00:31:33.420 --> 00:31:36.440 align:middle line:84%
because I didn't strictly
speak define E minus 1.

00:31:36.440 --> 00:31:42.900 align:middle line:90%


00:31:42.900 --> 00:31:48.060 align:middle line:84%
So now I want to do
this more generally.

00:31:48.060 --> 00:31:53.110 align:middle line:90%
So I take a power series.

00:31:53.110 --> 00:32:01.020 align:middle line:90%


00:32:01.020 --> 00:32:03.100 align:middle line:90%
Also, by the way, the plan--

00:32:03.100 --> 00:32:07.580 align:middle line:84%
so after these lectures, there's
two more lectures, Thursday

00:32:07.580 --> 00:32:08.960 align:middle line:90%
and Tuesday next week.

00:32:08.960 --> 00:32:14.260 align:middle line:90%


00:32:14.260 --> 00:32:22.480 align:middle line:84%
And I already updated the
course plan to reflect this.

00:32:22.480 --> 00:32:25.300 align:middle line:84%
So my plan is next
time, I will prove

00:32:25.300 --> 00:32:29.100 align:middle line:84%
existence of
uniqueness of some ODE

00:32:29.100 --> 00:32:32.940 align:middle line:84%
using things we have learned
here about metric spaces.

00:32:32.940 --> 00:32:36.600 align:middle line:84%
And then, Tuesday next week,
we'll do a review of the class.

00:32:36.600 --> 00:32:38.870 align:middle line:84%
So there won't be any
new material on Tuesday.

00:32:38.870 --> 00:33:01.350 align:middle line:90%


00:33:01.350 --> 00:33:06.140 align:middle line:84%
Also, for whatever it's worth, I
decided in the end with a friend

00:33:06.140 --> 00:33:10.700 align:middle line:84%
to turn in the lecture notes,
to turn it into a book,

00:33:10.700 --> 00:33:14.280 align:middle line:84%
just because the TPBB that
was like the main reference,

00:33:14.280 --> 00:33:15.880 align:middle line:90%
I didn't find that great anyway.

00:33:15.880 --> 00:33:22.460 align:middle line:84%
It was also 1,000 pages, who
would want to read 1,000 pages.

00:33:22.460 --> 00:33:26.160 align:middle line:84%
And so the course
notes here is shorter,

00:33:26.160 --> 00:33:28.340 align:middle line:84%
as you probably have
seen, and trying

00:33:28.340 --> 00:33:33.380 align:middle line:90%
to focus on the key points.

00:33:33.380 --> 00:33:37.520 align:middle line:84%
So eventually, there
will be a book.

00:33:37.520 --> 00:33:59.860 align:middle line:90%


00:33:59.860 --> 00:34:03.960 align:middle line:84%
So now I want to do
this more generally.

00:34:03.960 --> 00:34:06.120 align:middle line:90%
So we take a power series.

00:34:06.120 --> 00:34:10.540 align:middle line:84%
So we have an as a sequence, and
we're looking at a power series

00:34:10.540 --> 00:34:11.980 align:middle line:90%
like this.

00:34:11.980 --> 00:34:13.270 align:middle line:90%
So this is a power series.

00:34:13.270 --> 00:34:21.620 align:middle line:90%


00:34:21.620 --> 00:34:31.300 align:middle line:84%
And so just to remind you,
the radius of convergence

00:34:31.300 --> 00:34:37.340 align:middle line:90%
is given as follows.

00:34:37.340 --> 00:34:44.940 align:middle line:84%
So we take M, and M is
defined to be the lim

00:34:44.940 --> 00:34:52.860 align:middle line:84%
sup as n goes to
infinity of the n-th root

00:34:52.860 --> 00:34:57.500 align:middle line:90%
of absolute value of an.

00:34:57.500 --> 00:35:01.420 align:middle line:84%
And then the radius of
convergence, so R here,

00:35:01.420 --> 00:35:07.140 align:middle line:84%
is then 1 over M with
this usual convention

00:35:07.140 --> 00:35:10.380 align:middle line:84%
that if M is
infinity, this is 0.

00:35:10.380 --> 00:35:13.320 align:middle line:90%
If M is 0, this is infinity.

00:35:13.320 --> 00:35:18.480 align:middle line:84%
And so then we have,
again, that we have that--

00:35:18.480 --> 00:35:23.780 align:middle line:84%
so we have that the
series here, so if you're

00:35:23.780 --> 00:35:31.460 align:middle line:84%
looking at this k equal
to 0 up to n of an xn,

00:35:31.460 --> 00:35:49.420 align:middle line:84%
this here converts to
this limit here uniformly

00:35:49.420 --> 00:35:54.100 align:middle line:84%
on each interval
of this form here,

00:35:54.100 --> 00:36:01.580 align:middle line:84%
where L here is
strictly less than 1.

00:36:01.580 --> 00:36:07.101 align:middle line:84%
And this is, again,
is Weinstrass M-test.

00:36:07.101 --> 00:36:19.632 align:middle line:90%


00:36:19.632 --> 00:36:24.060 align:middle line:84%
Now what I'm interested
in is I'm interested in.

00:36:24.060 --> 00:36:27.140 align:middle line:84%
So I want to be
able to calculate

00:36:27.140 --> 00:36:28.600 align:middle line:90%
the derivative of this.

00:36:28.600 --> 00:36:32.820 align:middle line:90%


00:36:32.820 --> 00:36:41.740 align:middle line:84%
So we define a function f by
that f of x is equal to the sum

00:36:41.740 --> 00:36:44.200 align:middle line:84%
here from k equal
to 0 to infinity.

00:36:44.200 --> 00:36:52.860 align:middle line:84%
So this is the power
series x so k, like that.

00:36:52.860 --> 00:37:05.220 align:middle line:84%
And we want a formula
for the derivative.

00:37:05.220 --> 00:37:11.060 align:middle line:84%
And in fact, I want the
formula for any derivative of--

00:37:11.060 --> 00:37:14.310 align:middle line:84%
so say the M derivative
of this function.

00:37:14.310 --> 00:37:22.420 align:middle line:90%


00:37:22.420 --> 00:37:25.900 align:middle line:90%
So now I look at--

00:37:25.900 --> 00:37:28.380 align:middle line:84%
so we had take
this power series,

00:37:28.380 --> 00:37:33.030 align:middle line:84%
and I'm looking at the power
series that is given by--

00:37:33.030 --> 00:37:38.320 align:middle line:90%


00:37:38.320 --> 00:37:42.140 align:middle line:84%
so suppose you're looking
at the power series

00:37:42.140 --> 00:37:47.820 align:middle line:84%
where for each term, so you have
in the original power series.

00:37:47.820 --> 00:37:51.580 align:middle line:90%
It's an times x to the n.

00:37:51.580 --> 00:38:03.140 align:middle line:84%
Then I'm looking at n an
times x minus 1 like this.

00:38:03.140 --> 00:38:12.440 align:middle line:90%
And here, I'm summing from 1--

00:38:12.440 --> 00:38:15.180 align:middle line:90%


00:38:15.180 --> 00:38:19.980 align:middle line:84%
I mean, it doesn't matter--
sum from 0, so 0 to infinity,

00:38:19.980 --> 00:38:22.980 align:middle line:90%
like that.

00:38:22.980 --> 00:38:25.940 align:middle line:84%
Now the radius of
convergence for this-- so

00:38:25.940 --> 00:38:27.920 align:middle line:84%
what is the radius
of convergence?

00:38:27.920 --> 00:38:37.140 align:middle line:90%


00:38:37.140 --> 00:38:42.420 align:middle line:84%
The radius of
convergence for this

00:38:42.420 --> 00:38:50.920 align:middle line:84%
is the n-th root of n times
a to the n, like this.

00:38:50.920 --> 00:38:54.660 align:middle line:90%


00:38:54.660 --> 00:39:00.700 align:middle line:84%
And this thing here is the same
as n to the power 1 over n times

00:39:00.700 --> 00:39:06.580 align:middle line:90%
the n-th root of an, like this.

00:39:06.580 --> 00:39:12.220 align:middle line:84%
Now this thing here, if
you're looking at n like this,

00:39:12.220 --> 00:39:14.180 align:middle line:90%
this here is--

00:39:14.180 --> 00:39:21.500 align:middle line:84%
you can write this thing here as
E, and then it's log n over n.

00:39:21.500 --> 00:39:26.460 align:middle line:84%
This here, as n goes to
infinity, converges to 0.

00:39:26.460 --> 00:39:32.660 align:middle line:84%
So this thing here converges
to 1 by E to the 1.

00:39:32.660 --> 00:39:35.780 align:middle line:84%
And so you have
that lim sup here.

00:39:35.780 --> 00:39:46.220 align:middle line:84%
So the lim sup of the n-th
root of n times an, like this--

00:39:46.220 --> 00:39:49.820 align:middle line:84%
this thing here is
because this here, you

00:39:49.820 --> 00:39:54.200 align:middle line:84%
can write this as
the same as lim sup.

00:39:54.200 --> 00:39:58.140 align:middle line:84%
n goes to infinity.
n goes to infinity.

00:39:58.140 --> 00:40:02.420 align:middle line:84%
It's the same as the n-th
root of this thing here times

00:40:02.420 --> 00:40:04.220 align:middle line:90%
the n-th root of--

00:40:04.220 --> 00:40:05.120 align:middle line:90%
like this.

00:40:05.120 --> 00:40:06.940 align:middle line:90%
This here converts to 1.

00:40:06.940 --> 00:40:12.380 align:middle line:84%
So it really just converges--
so it's equal to the lim sup

00:40:12.380 --> 00:40:19.380 align:middle line:84%
as n goes to infinity
of the n-th root of n.

00:40:19.380 --> 00:40:24.660 align:middle line:84%
And that was what we
call M originally.

00:40:24.660 --> 00:40:30.740 align:middle line:84%
So this lim sup is the
same as this lim sup.

00:40:30.740 --> 00:40:33.940 align:middle line:84%
So this means that M
for this new sequence

00:40:33.940 --> 00:40:36.700 align:middle line:84%
is the same as M for
the old sequence.

00:40:36.700 --> 00:40:42.260 align:middle line:84%
So this means that the radius of
convergence for the new sequence

00:40:42.260 --> 00:40:44.500 align:middle line:84%
is equal to the
radius of convergence

00:40:44.500 --> 00:40:45.846 align:middle line:90%
from the old sequence.

00:40:45.846 --> 00:40:49.500 align:middle line:90%


00:40:49.500 --> 00:40:54.460 align:middle line:84%
So if you take the
derivative term by term

00:40:54.460 --> 00:40:56.900 align:middle line:84%
and you form this
new power series,

00:40:56.900 --> 00:40:59.900 align:middle line:84%
then it has the same
radius of convergence

00:40:59.900 --> 00:41:01.230 align:middle line:90%
as the original passes.

00:41:01.230 --> 00:41:05.340 align:middle line:90%


00:41:05.340 --> 00:41:08.680 align:middle line:90%
And so now you can iterate this.

00:41:08.680 --> 00:41:12.300 align:middle line:90%


00:41:12.300 --> 00:41:13.760 align:middle line:90%
So you can iterate this.

00:41:13.760 --> 00:41:21.860 align:middle line:90%


00:41:21.860 --> 00:41:23.940 align:middle line:90%
So you can take the--

00:41:23.940 --> 00:41:26.700 align:middle line:84%
so this is just taking
the derivative term

00:41:26.700 --> 00:41:29.180 align:middle line:90%
by term one time.

00:41:29.180 --> 00:41:33.260 align:middle line:84%
If you now take the
derivative, suppose

00:41:33.260 --> 00:41:36.500 align:middle line:84%
you're starting with
this sequence here.

00:41:36.500 --> 00:41:40.460 align:middle line:84%
So you're starting
with this power series.

00:41:40.460 --> 00:41:45.220 align:middle line:84%
And you're taking the
derivative term by term.

00:41:45.220 --> 00:41:48.460 align:middle line:84%
Then you get as we
did up there, you're

00:41:48.460 --> 00:41:50.620 align:middle line:90%
getting this power series.

00:41:50.620 --> 00:41:55.490 align:middle line:84%
So now you take a derivative
again term by term.

00:41:55.490 --> 00:42:02.100 align:middle line:90%


00:42:02.100 --> 00:42:04.640 align:middle line:90%
So you're getting this right.

00:42:04.640 --> 00:42:09.340 align:middle line:84%
And the thing is that each
time the radius of convergence

00:42:09.340 --> 00:42:22.820 align:middle line:84%
for this same radius of
convergence, these two here--

00:42:22.820 --> 00:42:26.300 align:middle line:90%
same radius of convergence--

00:42:26.300 --> 00:42:35.540 align:middle line:84%
it's because of the same
principle, same radius,

00:42:35.540 --> 00:42:37.080 align:middle line:90%
and so on.

00:42:37.080 --> 00:42:38.150 align:middle line:90%
And so you can continue.

00:42:38.150 --> 00:42:40.860 align:middle line:90%


00:42:40.860 --> 00:42:46.940 align:middle line:84%
And if you do this,
if you do this M time,

00:42:46.940 --> 00:42:48.760 align:middle line:90%
then you're getting n--

00:42:48.760 --> 00:42:54.080 align:middle line:90%


00:42:54.080 --> 00:43:00.380 align:middle line:84%
so if you do this
M times, then you

00:43:00.380 --> 00:43:10.260 align:middle line:84%
get that this thing here is x
minus M, and you're getting an.

00:43:10.260 --> 00:43:23.100 align:middle line:84%
And here, you're getting n
minus 1, n minus 2, up to n

00:43:23.100 --> 00:43:25.720 align:middle line:90%
minus M plus 1.

00:43:25.720 --> 00:43:28.980 align:middle line:90%


00:43:28.980 --> 00:43:32.260 align:middle line:90%
So you're getting that.

00:43:32.260 --> 00:43:33.860 align:middle line:90%
So that is after--

00:43:33.860 --> 00:43:35.600 align:middle line:90%
this is when you do it n times.

00:43:35.600 --> 00:43:37.420 align:middle line:84%
And so again, these
here will have

00:43:37.420 --> 00:43:39.040 align:middle line:90%
the same radius of convergence.

00:43:39.040 --> 00:43:48.820 align:middle line:90%


00:43:48.820 --> 00:43:53.660 align:middle line:84%
Now this thing here, if I want
to write this a little bit

00:43:53.660 --> 00:43:57.740 align:middle line:84%
more compactly, if I thinking
about this thing here, n

00:43:57.740 --> 00:44:04.580 align:middle line:84%
minus 2 up to n
minus M plus 1, I

00:44:04.580 --> 00:44:08.760 align:middle line:84%
can write this thing
here as n factorial.

00:44:08.760 --> 00:44:12.020 align:middle line:90%


00:44:12.020 --> 00:44:14.440 align:middle line:90%
But then I'm getting all these--

00:44:14.440 --> 00:44:21.040 align:middle line:84%
so if I wrote it as n factorial,
then I would also have--

00:44:21.040 --> 00:44:22.680 align:middle line:90%
it would keep going like this.

00:44:22.680 --> 00:44:30.120 align:middle line:84%
And the next one here
would be n minus M.

00:44:30.120 --> 00:44:33.180 align:middle line:84%
So if I write it-- so I can
write this thing here times

00:44:33.180 --> 00:44:36.400 align:middle line:90%
this factorial is equal to that.

00:44:36.400 --> 00:44:36.900 align:middle line:90%
Yeah?

00:44:36.900 --> 00:44:38.740 align:middle line:90%
Sorry.

00:44:38.740 --> 00:44:41.340 align:middle line:90%
AUDIENCE: [INAUDIBLE]

00:44:41.340 --> 00:44:50.300 align:middle line:90%


00:44:50.300 --> 00:44:53.340 align:middle line:84%
TOBIAS COLDING: So I think you
were complaining about one thing

00:44:53.340 --> 00:44:57.780 align:middle line:84%
that I sort of
pushed under the rug.

00:44:57.780 --> 00:45:09.060 align:middle line:84%
And that is the following, that
if you take the way we defined--

00:45:09.060 --> 00:45:13.780 align:middle line:84%
so if you take a power
series, again, like this,

00:45:13.780 --> 00:45:20.340 align:middle line:84%
and you define the
radius of convergence,

00:45:20.340 --> 00:45:24.380 align:middle line:84%
then you define it
from this n element.

00:45:24.380 --> 00:45:26.460 align:middle line:84%
I think that's what
you're complaining about.

00:45:26.460 --> 00:45:30.380 align:middle line:84%
And so you take the
coefficient to the n power.

00:45:30.380 --> 00:45:32.860 align:middle line:90%
That's not exactly what I did.

00:45:32.860 --> 00:45:34.780 align:middle line:84%
Is that what you're
complaining about?

00:45:34.780 --> 00:45:36.560 align:middle line:90%
And that doesn't matter.

00:45:36.560 --> 00:45:39.980 align:middle line:84%
And the thing is
so when you define

00:45:39.980 --> 00:45:46.220 align:middle line:84%
the radius of convergence, you
took this n power, like this.

00:45:46.220 --> 00:45:52.380 align:middle line:84%
But there was a coefficient to
where this here was to the n.

00:45:52.380 --> 00:45:55.300 align:middle line:84%
When I'm doing it
over here, there's

00:45:55.300 --> 00:45:56.960 align:middle line:90%
two ways of dealing with it.

00:45:56.960 --> 00:46:00.380 align:middle line:84%
One is the one you suggest,
and the other one-- and that

00:46:00.380 --> 00:46:04.060 align:middle line:84%
was why I put it on
slipped it under the rock.

00:46:04.060 --> 00:46:09.260 align:middle line:84%
Is that that's
the way the radius

00:46:09.260 --> 00:46:11.500 align:middle line:84%
this with the radius
of convergence,

00:46:11.500 --> 00:46:15.060 align:middle line:84%
it comes from comparing it
with the geometric series.

00:46:15.060 --> 00:46:16.900 align:middle line:84%
And then it really
doesn't matter

00:46:16.900 --> 00:46:19.820 align:middle line:84%
for this term in terms of x
whether you have shifted it

00:46:19.820 --> 00:46:20.440 align:middle line:90%
or not.

00:46:20.440 --> 00:46:26.040 align:middle line:84%
But if you do it, if you
do it as you're suggesting,

00:46:26.040 --> 00:46:32.860 align:middle line:84%
which would be totally fine,
so then this thing here, what

00:46:32.860 --> 00:46:36.420 align:middle line:84%
you really should have done
is that we should have thought

00:46:36.420 --> 00:46:40.460 align:middle line:84%
about this n, an,
and then we should

00:46:40.460 --> 00:46:44.680 align:middle line:84%
take this here, and
instead of the n root,

00:46:44.680 --> 00:46:46.600 align:middle line:84%
we should take the
n minus 1 root.

00:46:46.600 --> 00:46:49.580 align:middle line:90%
But that doesn't matter either.

00:46:49.580 --> 00:46:51.920 align:middle line:84%
That's going to
be the same also.

00:46:51.920 --> 00:46:54.860 align:middle line:84%
So either way, you can check
either of these two things.

00:46:54.860 --> 00:46:57.260 align:middle line:84%
And I was thinking
about the first

00:46:57.260 --> 00:46:58.890 align:middle line:90%
and where it's coming from.

00:46:58.890 --> 00:47:12.300 align:middle line:90%


00:47:12.300 --> 00:47:14.720 align:middle line:84%
Sorry, now I lost
my thread here.

00:47:14.720 --> 00:47:21.780 align:middle line:84%
So I was just observing that if
you can write the n factorial

00:47:21.780 --> 00:47:26.740 align:middle line:84%
as first taking all
of these factors

00:47:26.740 --> 00:47:30.140 align:middle line:84%
and then taking n
minus 1, so this

00:47:30.140 --> 00:47:37.340 align:middle line:84%
means that n factorial
divided by n minus 1,

00:47:37.340 --> 00:47:48.500 align:middle line:84%
so n minus m factorial, this is
equal to n minus 1, n minus 2,

00:47:48.500 --> 00:47:53.320 align:middle line:84%
down to n minus m
plus 1, like that.

00:47:53.320 --> 00:47:56.780 align:middle line:90%


00:47:56.780 --> 00:48:00.020 align:middle line:84%
But you see, that's exactly
what we have done here.

00:48:00.020 --> 00:48:04.860 align:middle line:84%
So this thing here, so
what I conclude from this

00:48:04.860 --> 00:48:33.220 align:middle line:84%
is that if I take a
power series like this,

00:48:33.220 --> 00:48:42.020 align:middle line:84%
and I take the derivative term
by term, and I do this M times,

00:48:42.020 --> 00:48:50.420 align:middle line:84%
then this is what I get is n
factorial n minus M factorial

00:48:50.420 --> 00:49:05.800 align:middle line:90%
and then an xn n minus M.

00:49:05.800 --> 00:49:10.180 align:middle line:84%
So this is when we do it term
by term, taking the derivative.

00:49:10.180 --> 00:49:13.940 align:middle line:84%
And we already have
that these here have

00:49:13.940 --> 00:49:15.720 align:middle line:90%
the same radius of convergence.

00:49:15.720 --> 00:49:23.580 align:middle line:90%


00:49:23.580 --> 00:49:28.830 align:middle line:84%
And so now we have
the following theorem.

00:49:28.830 --> 00:49:32.660 align:middle line:90%


00:49:32.660 --> 00:49:35.580 align:middle line:84%
Then if you take a
power series, so you

00:49:35.580 --> 00:49:42.600 align:middle line:84%
take a power series like this,
R is the radius of convergence.

00:49:42.600 --> 00:49:54.260 align:middle line:90%


00:49:54.260 --> 00:49:58.700 align:middle line:84%
And if L here is strictly
less than some positive number

00:49:58.700 --> 00:50:02.740 align:middle line:84%
but strictly less than
the radius of convergence,

00:50:02.740 --> 00:50:13.000 align:middle line:84%
then these guys
here converge to--

00:50:13.000 --> 00:50:16.780 align:middle line:84%
so when you're summing,
when you take a finite sum,

00:50:16.780 --> 00:50:27.130 align:middle line:84%
these converge to this
uniformly, but not only these.

00:50:27.130 --> 00:50:36.540 align:middle line:90%


00:50:36.540 --> 00:50:41.860 align:middle line:84%
But not only that, but
you also have that--

00:50:41.860 --> 00:51:04.490 align:middle line:84%
more interesting-- you have that
this sequence here, k minus M--

00:51:04.490 --> 00:51:21.010 align:middle line:84%
k factorial divided by k minus
M factorial ak xk minus M,

00:51:21.010 --> 00:51:24.250 align:middle line:84%
that these sequence
here converge

00:51:24.250 --> 00:51:29.130 align:middle line:90%
uniformly to the derivative.

00:51:29.130 --> 00:51:40.090 align:middle line:84%
This here is f of x to the
M derivative of x of f.

00:51:40.090 --> 00:51:41.670 align:middle line:84%
So we have that
these functions--

00:51:41.670 --> 00:51:45.170 align:middle line:84%
but that we already proved
that these functions converge,

00:51:45.170 --> 00:51:59.250 align:middle line:84%
and their derivative here
converge uniformly, like this,

00:51:59.250 --> 00:52:00.300 align:middle line:90%
on the same interval.

00:52:00.300 --> 00:52:06.746 align:middle line:90%


00:52:06.746 --> 00:52:10.130 align:middle line:90%
Now why is this the case?

00:52:10.130 --> 00:52:13.270 align:middle line:84%
So this here is
again it's following.

00:52:13.270 --> 00:52:15.280 align:middle line:90%
So this follows the proof--

00:52:15.280 --> 00:52:19.090 align:middle line:90%


00:52:19.090 --> 00:52:22.850 align:middle line:90%
follows from the same theorem--

00:52:22.850 --> 00:52:31.370 align:middle line:84%
follows from the theorem
we proved earlier,

00:52:31.370 --> 00:52:32.160 align:middle line:90%
we showed earlier.

00:52:32.160 --> 00:52:36.170 align:middle line:90%


00:52:36.170 --> 00:52:39.570 align:middle line:90%
And let's just go through that.

00:52:39.570 --> 00:52:41.250 align:middle line:90%
So let me go through it.

00:52:41.250 --> 00:52:52.850 align:middle line:84%
So let's assume, first,
that M is equal to 1.

00:52:52.850 --> 00:52:56.698 align:middle line:90%
So I just take one derivative--

00:52:56.698 --> 00:53:02.610 align:middle line:84%
well, then I'm looking
at this sequence here,

00:53:02.610 --> 00:53:08.690 align:middle line:90%
k xk k equal to 0 to n.

00:53:08.690 --> 00:53:15.170 align:middle line:84%
I'm looking at these that
converge to this infinite--

00:53:15.170 --> 00:53:17.910 align:middle line:90%
to converge to f.

00:53:17.910 --> 00:53:21.210 align:middle line:90%


00:53:21.210 --> 00:53:23.890 align:middle line:84%
f, again, is this
infinite power series.

00:53:23.890 --> 00:53:26.710 align:middle line:84%
And I'm looking at the
derivative of these guys.

00:53:26.710 --> 00:53:29.650 align:middle line:90%
So these are these.

00:53:29.650 --> 00:53:38.450 align:middle line:84%
And I know now that these here
converge uniformly and these

00:53:38.450 --> 00:53:41.870 align:middle line:84%
here converge uniformly
the power series--

00:53:41.870 --> 00:53:44.610 align:middle line:90%
that is, this infinite series.

00:53:44.610 --> 00:53:47.170 align:middle line:84%
This here was the
finite part of it.

00:53:47.170 --> 00:53:50.910 align:middle line:84%
And this here is the infinite
part-- the whole thing.

00:53:50.910 --> 00:53:57.170 align:middle line:90%


00:53:57.170 --> 00:53:58.830 align:middle line:90%
So we have that.

00:53:58.830 --> 00:54:03.690 align:middle line:90%


00:54:03.690 --> 00:54:05.830 align:middle line:90%
This means, in particular--

00:54:05.830 --> 00:54:11.690 align:middle line:84%
so this thing here
implies, of course,

00:54:11.690 --> 00:54:18.650 align:middle line:84%
that when you're looking at 0,
when you're looking at 0, if you

00:54:18.650 --> 00:54:23.450 align:middle line:84%
evaluate this thing here at
0, then, in this one here,

00:54:23.450 --> 00:54:28.330 align:middle line:84%
you get in this is the
sequence of functions,

00:54:28.330 --> 00:54:34.830 align:middle line:84%
f of x from before, these
are the fn prime of x.

00:54:34.830 --> 00:54:38.010 align:middle line:90%


00:54:38.010 --> 00:54:40.670 align:middle line:90%
And so now I claim that--

00:54:40.670 --> 00:54:44.030 align:middle line:84%
so the theorem that
we proved earlier

00:54:44.030 --> 00:54:49.130 align:middle line:84%
is that if you take a
sequence of functions that

00:54:49.130 --> 00:54:53.590 align:middle line:84%
are differentiable and the
derivative is continuous--

00:54:53.590 --> 00:54:56.930 align:middle line:84%
these are all polynomials, so
this is definitely the case.

00:54:56.930 --> 00:55:02.370 align:middle line:84%
And we know that
these values here fn--

00:55:02.370 --> 00:55:08.530 align:middle line:84%
in fact, at 0, they're
equal to f of 0.

00:55:08.530 --> 00:55:10.890 align:middle line:90%
So we had three conditions.

00:55:10.890 --> 00:55:14.690 align:middle line:84%
We had that the fn
in some particular

00:55:14.690 --> 00:55:19.730 align:middle line:84%
point that we call x0, this
is now 0, that this converged.

00:55:19.730 --> 00:55:24.210 align:middle line:84%
We have that the f prime
was converging uniformly.

00:55:24.210 --> 00:55:27.090 align:middle line:84%
Well, we know that these
converge uniformly.

00:55:27.090 --> 00:55:30.150 align:middle line:84%
And then we had that the f
prime should be continuous.

00:55:30.150 --> 00:55:31.830 align:middle line:84%
But they were
obviously continuous.

00:55:31.830 --> 00:55:35.090 align:middle line:90%
They were polynomials.

00:55:35.090 --> 00:55:47.170 align:middle line:84%
Then we had that the derivative
converged uniformly and that

00:55:47.170 --> 00:55:50.890 align:middle line:84%
the function that
they converge to--

00:55:50.890 --> 00:55:54.810 align:middle line:84%
the derivative converge and
also the original function

00:55:54.810 --> 00:56:02.490 align:middle line:84%
converge and that the
derivative converge

00:56:02.490 --> 00:56:06.090 align:middle line:84%
uniformly to the
derivative of the function

00:56:06.090 --> 00:56:08.530 align:middle line:90%
that we converge to.

00:56:08.530 --> 00:56:12.330 align:middle line:84%
So you see that this
is just checking

00:56:12.330 --> 00:56:15.950 align:middle line:84%
that we have the three property
from the theorem before.

00:56:15.950 --> 00:56:18.090 align:middle line:84%
And then we get
the two conclusion.

00:56:18.090 --> 00:56:19.850 align:middle line:84%
And the one
conclusion that we're

00:56:19.850 --> 00:56:24.490 align:middle line:84%
interested in is that this
here is then the power

00:56:24.490 --> 00:56:27.130 align:middle line:90%
series for the derivative of f.

00:56:27.130 --> 00:56:35.850 align:middle line:90%


00:56:35.850 --> 00:56:39.290 align:middle line:84%
And then you can do
the same thing with--

00:56:39.290 --> 00:56:49.850 align:middle line:84%
so let me just say that you
can do the same thing if you

00:56:49.850 --> 00:56:51.970 align:middle line:90%
are integrating.

00:56:51.970 --> 00:56:54.270 align:middle line:90%
So here, we proved--

00:56:54.270 --> 00:57:00.170 align:middle line:84%
so suppose you take a sequence
here that is converging to f.

00:57:00.170 --> 00:57:04.330 align:middle line:84%
Well, suppose you take
a power series here.

00:57:04.330 --> 00:57:14.730 align:middle line:84%
Suppose you take this power
series, ak xk k equal to 0.

00:57:14.730 --> 00:57:16.150 align:middle line:90%
So this is the finite--

00:57:16.150 --> 00:57:19.810 align:middle line:90%
this is the power series, sorry.

00:57:19.810 --> 00:57:24.010 align:middle line:84%
And suppose I'm interested in
what is the integral from a

00:57:24.010 --> 00:57:33.770 align:middle line:84%
to b of this power
series f of x dx.

00:57:33.770 --> 00:57:44.930 align:middle line:84%
And here, I'm assuming that a
and b are in the interval, where

00:57:44.930 --> 00:57:48.970 align:middle line:90%
the power series is convergent.

00:57:48.970 --> 00:57:52.610 align:middle line:84%
So this means, of course,
that if you think about it

00:57:52.610 --> 00:57:54.530 align:middle line:90%
that you have here 0.

00:57:54.530 --> 00:57:59.710 align:middle line:84%
You have R. You have here minus
R. And then a and b is lying--

00:57:59.710 --> 00:58:02.170 align:middle line:84%
and so this means that
this whole interval

00:58:02.170 --> 00:58:05.960 align:middle line:84%
is lying comfortably inside
some interval like this.

00:58:05.960 --> 00:58:11.750 align:middle line:90%


00:58:11.750 --> 00:58:18.570 align:middle line:84%
And I'm asking what is the nice
formula for this integral here?

00:58:18.570 --> 00:58:24.090 align:middle line:84%
And so then, well, I
can use not the theorem

00:58:24.090 --> 00:58:27.230 align:middle line:84%
we proved earlier but the
theorem we proved last time.

00:58:27.230 --> 00:58:29.170 align:middle line:90%
And so what is that?

00:58:29.170 --> 00:58:36.290 align:middle line:84%
So if I define fn of x to be
equal to the sum here from k

00:58:36.290 --> 00:58:42.570 align:middle line:90%
equals to 0 to n of ak xk--

00:58:42.570 --> 00:58:45.850 align:middle line:90%
sorry, x to the power k--

00:58:45.850 --> 00:58:49.330 align:middle line:84%
this thing here,
these here converge

00:58:49.330 --> 00:58:55.850 align:middle line:84%
uniformly to f of
x on any interval

00:58:55.850 --> 00:59:00.490 align:middle line:84%
like this when L here is
strictly less than the radius

00:59:00.490 --> 00:59:01.990 align:middle line:90%
of convergence.

00:59:01.990 --> 00:59:04.310 align:middle line:90%
So they converge here uniformly.

00:59:04.310 --> 00:59:07.370 align:middle line:90%


00:59:07.370 --> 00:59:09.210 align:middle line:84%
But the theorem
we proved earlier

00:59:09.210 --> 00:59:14.490 align:middle line:84%
was that if you take a
uniform convergence like this

00:59:14.490 --> 00:59:17.370 align:middle line:84%
and you take a and
b in this interval,

00:59:17.370 --> 00:59:29.970 align:middle line:84%
then the integral of these guys
here converge to the integral

00:59:29.970 --> 00:59:30.930 align:middle line:90%
like this.

00:59:30.930 --> 00:59:34.450 align:middle line:90%
You have this convergence here.

00:59:34.450 --> 00:59:37.170 align:middle line:84%
But these here are
easy to integrate.

00:59:37.170 --> 00:59:42.050 align:middle line:90%


00:59:42.050 --> 00:59:50.170 align:middle line:84%
But because they're
polynomial, so this

00:59:50.170 --> 00:59:56.510 align:middle line:84%
means that the fn
s, the fn of s,

00:59:56.510 --> 01:00:00.530 align:middle line:84%
when you integrate
this from a to b ds,

01:00:00.530 --> 01:00:14.970 align:middle line:84%
these guys are the sum here
of ak sk k equal to 0 to n,

01:00:14.970 --> 01:00:21.930 align:middle line:84%
and then the integral here, ds
from a to b because it's just

01:00:21.930 --> 01:00:23.450 align:middle line:90%
that polynomial.

01:00:23.450 --> 01:00:25.970 align:middle line:84%
And so for polynomial,
well, we can just

01:00:25.970 --> 01:00:35.210 align:middle line:84%
use that it's a sum of
these guys, ak sk ds k

01:00:35.210 --> 01:00:37.930 align:middle line:90%
equals to 0 to n.

01:00:37.930 --> 01:00:46.770 align:middle line:84%
And this thing here,
when we integrate this,

01:00:46.770 --> 01:00:48.170 align:middle line:90%
that's just the--

01:00:48.170 --> 01:00:50.930 align:middle line:84%
I mean, now it doesn't
get much nicer unless you

01:00:50.930 --> 01:00:56.050 align:middle line:90%
make one of them equal to 0.

01:00:56.050 --> 01:00:58.210 align:middle line:90%
So you have this.

01:00:58.210 --> 01:01:08.050 align:middle line:84%
So let me say that if
a here was equal to 0,

01:01:08.050 --> 01:01:12.130 align:middle line:84%
and B was equal to x,
so if that's the case

01:01:12.130 --> 01:01:19.110 align:middle line:84%
and you're looking at this
integral from 0 to x of fn s ds,

01:01:19.110 --> 01:01:25.740 align:middle line:84%
we know that this here converged
to the integral of the power

01:01:25.740 --> 01:01:26.240 align:middle line:90%
series.

01:01:26.240 --> 01:01:28.970 align:middle line:90%


01:01:28.970 --> 01:01:31.310 align:middle line:84%
On the other hand,
this integral here--

01:01:31.310 --> 01:01:44.610 align:middle line:90%


01:01:44.610 --> 01:01:46.730 align:middle line:84%
on the other hand,
this integral here,

01:01:46.730 --> 01:01:56.430 align:middle line:84%
if you're looking at the
sum here and then sum,

01:01:56.430 --> 01:02:06.250 align:middle line:84%
and now the a is 0, b is x,
so then is this here ak xk,

01:02:06.250 --> 01:02:11.130 align:middle line:84%
now when we integrate
this term here,

01:02:11.130 --> 01:02:15.130 align:middle line:84%
we're getting sum here
k equal to 0 to n.

01:02:15.130 --> 01:02:29.750 align:middle line:84%
And then this here becomes ak k
plus 1 x to the power k plus 1.

01:02:29.750 --> 01:02:35.330 align:middle line:90%


01:02:35.330 --> 01:02:38.270 align:middle line:84%
And so you see that
if you're looking at--

01:02:38.270 --> 01:02:45.450 align:middle line:84%
so you see that these guys here
now converge to the integral

01:02:45.450 --> 01:02:51.050 align:middle line:90%
from 0 to x of f of s ds.

01:02:51.050 --> 01:02:53.290 align:middle line:84%
That's what we get
from the theorem.

01:02:53.290 --> 01:02:59.650 align:middle line:84%
So the conclusion here is that
if you take a power series

01:02:59.650 --> 01:03:02.810 align:middle line:84%
and you're looking inside
the radius of convergence,

01:03:02.810 --> 01:03:06.050 align:middle line:84%
then the power series is
differentiable as many times

01:03:06.050 --> 01:03:07.290 align:middle line:90%
as you want.

01:03:07.290 --> 01:03:11.190 align:middle line:84%
And the derivative is
given by a power series.

01:03:11.190 --> 01:03:16.450 align:middle line:84%
And it's just the derivative
of the individual term by term.

01:03:16.450 --> 01:03:21.410 align:middle line:84%
And likewise, if you want
to integrate a power series,

01:03:21.410 --> 01:03:25.397 align:middle line:84%
then the integral, at least
when you're integrating because,

01:03:25.397 --> 01:03:27.230 align:middle line:84%
otherwise, the formula
is not quite as nice,

01:03:27.230 --> 01:03:31.930 align:middle line:84%
but you do get a formula, but
it just doesn't look so nice.

01:03:31.930 --> 01:03:34.910 align:middle line:84%
But the integral
of a power series,

01:03:34.910 --> 01:03:37.680 align:middle line:84%
you can just integrate
it term by term.

01:03:37.680 --> 01:03:41.130 align:middle line:90%


01:03:41.130 --> 01:03:44.610 align:middle line:84%
So now the next thing
we want to talk about--

01:03:44.610 --> 01:03:50.050 align:middle line:84%
and I'm just trying to
set up for next lecture.

01:03:50.050 --> 01:03:54.050 align:middle line:84%
And so we want to talk
about differential equations

01:03:54.050 --> 01:03:58.090 align:middle line:84%
and how we're using
some of the stuff

01:03:58.090 --> 01:04:03.010 align:middle line:84%
that we've proven in this class
to solve differential equation.

01:04:03.010 --> 01:04:05.330 align:middle line:84%
And it's an example
where it may not

01:04:05.330 --> 01:04:13.890 align:middle line:84%
be very obvious that you could
use metric spaces to solve

01:04:13.890 --> 01:04:14.920 align:middle line:90%
a differential equation.

01:04:14.920 --> 01:04:17.490 align:middle line:90%


01:04:17.490 --> 01:04:20.010 align:middle line:84%
But this is
nevertheless the case.

01:04:20.010 --> 01:04:23.920 align:middle line:84%
So we're looking at a
differential equation.

01:04:23.920 --> 01:04:31.250 align:middle line:90%


01:04:31.250 --> 01:04:39.588 align:middle line:84%
So differential equation is an
equation is an equation in--

01:04:39.588 --> 01:04:44.170 align:middle line:90%


01:04:44.170 --> 01:04:57.070 align:middle line:84%
an unknown in an unknown
function and its derivative.

01:04:57.070 --> 01:05:02.570 align:middle line:90%


01:05:02.570 --> 01:05:09.290 align:middle line:84%
So let me give you some
examples of this that you take--

01:05:09.290 --> 01:05:14.450 align:middle line:90%
you're looking at a function f.

01:05:14.450 --> 01:05:18.930 align:middle line:84%
You're trying to find a
function f so that-- so this is

01:05:18.930 --> 01:05:22.330 align:middle line:90%
like the first example.

01:05:22.330 --> 01:05:28.170 align:middle line:84%
You're looking for a function
f so that the derivative is x.

01:05:28.170 --> 01:05:30.250 align:middle line:84%
Well, we already
know that this here,

01:05:30.250 --> 01:05:43.250 align:middle line:84%
the solutions to this f of x
equal to 1/2 x squared plus some

01:05:43.250 --> 01:05:45.450 align:middle line:90%
constant.

01:05:45.450 --> 01:05:48.370 align:middle line:84%
The constant when you take
derivative, you get 0.

01:05:48.370 --> 01:05:52.330 align:middle line:84%
And the derivative of this
thing here gives you x.

01:05:52.330 --> 01:05:56.850 align:middle line:84%
And those are the
only solutions.

01:05:56.850 --> 01:06:01.890 align:middle line:84%
Another example
here is where you're

01:06:01.890 --> 01:06:08.630 align:middle line:84%
taking something that looks
like f prime minus f squared,

01:06:08.630 --> 01:06:10.550 align:middle line:90%
so f of x, like this.

01:06:10.550 --> 01:06:13.890 align:middle line:90%


01:06:13.890 --> 01:06:20.490 align:middle line:84%
And if you're looking at
the function here, f of x

01:06:20.490 --> 01:06:23.570 align:middle line:90%
is equal to 1 minus 1 over x.

01:06:23.570 --> 01:06:29.130 align:middle line:84%
If you take this function here
and now you take the derivative,

01:06:29.130 --> 01:06:33.650 align:middle line:84%
so now I'm using the chain
rule, so I get 1 minus 1,

01:06:33.650 --> 01:06:34.870 align:middle line:90%
like this, squared.

01:06:34.870 --> 01:06:37.210 align:middle line:84%
And then I take the
derivative of this.

01:06:37.210 --> 01:06:40.930 align:middle line:90%
So that's minus 1.

01:06:40.930 --> 01:06:43.930 align:middle line:90%


01:06:43.930 --> 01:06:46.890 align:middle line:90%
So that's minus 1 times minus 1.

01:06:46.890 --> 01:06:54.170 align:middle line:84%
So this here is minus
1 minus x squared.

01:06:54.170 --> 01:06:57.970 align:middle line:84%
And so you see that when
you take this function here,

01:06:57.970 --> 01:06:58.740 align:middle line:90%
the minus sign--

01:06:58.740 --> 01:07:14.130 align:middle line:90%


01:07:14.130 --> 01:07:17.090 align:middle line:90%
I think it should be a plus.

01:07:17.090 --> 01:07:19.730 align:middle line:90%
So when you take--

01:07:19.730 --> 01:07:21.230 align:middle line:90%
no, no, no, it should be minus.

01:07:21.230 --> 01:07:24.290 align:middle line:84%
No, no, that's right,
sorry, yeah, thanks.

01:07:24.290 --> 01:07:25.650 align:middle line:90%
This is wonderful.

01:07:25.650 --> 01:07:30.090 align:middle line:84%
This should have been
a minus like that.

01:07:30.090 --> 01:07:32.790 align:middle line:84%
And so this here is
now is indeed plus.

01:07:32.790 --> 01:07:34.140 align:middle line:90%
And then it's this equation.

01:07:34.140 --> 01:07:43.906 align:middle line:90%


01:07:43.906 --> 01:07:50.850 align:middle line:84%
The next example-- so again,
a differential equation

01:07:50.850 --> 01:07:55.850 align:middle line:84%
is something that involved
an unknown function

01:07:55.850 --> 01:07:59.330 align:middle line:90%
and its derivative.

01:07:59.330 --> 01:08:01.530 align:middle line:84%
So suppose you
take something that

01:08:01.530 --> 01:08:08.010 align:middle line:84%
looks like f, f prime, f
double prime equal to 0.

01:08:08.010 --> 01:08:13.690 align:middle line:84%
If you're taking the function
f equal to some constant,

01:08:13.690 --> 01:08:16.130 align:middle line:90%
this is a solution.

01:08:16.130 --> 01:08:23.090 align:middle line:84%
And if you're taking f equal to,
say, x or some constant times x,

01:08:23.090 --> 01:08:25.370 align:middle line:90%
this is also a solution.

01:08:25.370 --> 01:08:26.670 align:middle line:90%
They're both solutions.

01:08:26.670 --> 01:08:30.970 align:middle line:90%


01:08:30.970 --> 01:08:33.069 align:middle line:84%
And this is just
because the second--

01:08:33.069 --> 01:08:38.090 align:middle line:84%
in this case, the
second derivative is 0.

01:08:38.090 --> 01:08:41.250 align:middle line:84%
So now what we will
be interested in

01:08:41.250 --> 01:08:45.649 align:middle line:84%
is we're going to be
interested in what's

01:08:45.649 --> 01:08:47.710 align:middle line:84%
called an ordinary
differential equation.

01:08:47.710 --> 01:08:52.270 align:middle line:90%
And we only looked at this.

01:08:52.270 --> 01:08:54.840 align:middle line:84%
We only looked at function
of just one variable.

01:08:54.840 --> 01:09:00.330 align:middle line:90%


01:09:00.330 --> 01:09:02.950 align:middle line:84%
So this is what the
ordinary referred to.

01:09:02.950 --> 01:09:05.569 align:middle line:90%


01:09:05.569 --> 01:09:13.200 align:middle line:84%
So we want to look at ordinary
differential equation.

01:09:13.200 --> 01:09:17.810 align:middle line:90%


01:09:17.810 --> 01:09:23.210 align:middle line:84%
And an ordinary differential
equation is abbreviated by ODE.

01:09:23.210 --> 01:09:26.250 align:middle line:90%


01:09:26.250 --> 01:09:28.250 align:middle line:84%
And if it's not an
ordinary, then it's

01:09:28.250 --> 01:09:32.630 align:middle line:84%
usually a partial
differential equation,

01:09:32.630 --> 01:09:38.350 align:middle line:84%
which involve a function that
is of more than one variable.

01:09:38.350 --> 01:09:42.050 align:middle line:84%
So it will involve what's
called the partial derivative

01:09:42.050 --> 01:09:42.890 align:middle line:90%
of the functions.

01:09:42.890 --> 01:09:48.930 align:middle line:90%


01:09:48.930 --> 01:10:08.770 align:middle line:84%
So the unknown function
will be denoted by y.

01:10:08.770 --> 01:10:11.290 align:middle line:84%
And the equation
that we're looking at

01:10:11.290 --> 01:10:19.210 align:middle line:84%
is that we want some
particular value at, say, 0.

01:10:19.210 --> 01:10:25.610 align:middle line:84%
And then we want the derivative
satisfying an equation.

01:10:25.610 --> 01:10:30.670 align:middle line:84%
And the equation that we're
looking for is that we have--

01:10:30.670 --> 01:10:34.730 align:middle line:90%


01:10:34.730 --> 01:10:38.750 align:middle line:90%
so f here and g are given.

01:10:38.750 --> 01:10:43.430 align:middle line:84%
So think about those as
functions that are given.

01:10:43.430 --> 01:10:46.090 align:middle line:90%
Those are two given functions.

01:10:46.090 --> 01:10:48.770 align:middle line:90%
But they may not be super nice.

01:10:48.770 --> 01:10:53.210 align:middle line:84%
But you know that
f is differentiable

01:10:53.210 --> 01:11:00.590 align:middle line:84%
and the derivative is continuous
and g here is continuous.

01:11:00.590 --> 01:11:03.290 align:middle line:90%


01:11:03.290 --> 01:11:08.010 align:middle line:84%
But in principle, you
know they are given.

01:11:08.010 --> 01:11:09.930 align:middle line:90%
And now you're looking for--

01:11:09.930 --> 01:11:11.590 align:middle line:84%
but it may be very,
very complicated.

01:11:11.590 --> 01:11:16.760 align:middle line:84%
Maybe f is sine or
something like that.

01:11:16.760 --> 01:11:21.720 align:middle line:84%
And so you're looking
for an unknown function y

01:11:21.720 --> 01:11:24.240 align:middle line:84%
so that the derivative--
so you think

01:11:24.240 --> 01:11:27.840 align:middle line:90%
about y as a function of x.

01:11:27.840 --> 01:11:31.480 align:middle line:84%
And the derivative
of y is supposed

01:11:31.480 --> 01:11:36.960 align:middle line:84%
to be equal to f but is now
applied to this unknown function

01:11:36.960 --> 01:11:40.240 align:middle line:90%
and then plus g of x.

01:11:40.240 --> 01:11:43.560 align:middle line:84%
So this here is much more tame,
but this is a bit complicated

01:11:43.560 --> 01:11:47.320 align:middle line:84%
because it involves
the unknown function.

01:11:47.320 --> 01:11:52.160 align:middle line:90%
And so we want to see--

01:11:52.160 --> 01:12:08.290 align:middle line:84%
so we are asking the question,
does this ODE have a solution?

01:12:08.290 --> 01:12:13.480 align:middle line:90%


01:12:13.480 --> 01:12:24.410 align:middle line:90%
And is the solution unique?

01:12:24.410 --> 01:12:30.300 align:middle line:90%


01:12:30.300 --> 01:12:32.920 align:middle line:90%
So we're looking for a function.

01:12:32.920 --> 01:12:35.580 align:middle line:84%
So here's what
we're looking for.

01:12:35.580 --> 01:12:40.160 align:middle line:90%


01:12:40.160 --> 01:12:46.600 align:middle line:84%
We're looking for a function y
defined on some interval into R.

01:12:46.600 --> 01:12:49.300 align:middle line:84%
This function has to
be differentiable.

01:12:49.300 --> 01:12:52.920 align:middle line:90%
So this has to exist.

01:12:52.920 --> 01:13:02.080 align:middle line:84%
A 0 has to be in that interval
because a is just a constant.

01:13:02.080 --> 01:13:17.250 align:middle line:84%
And then we want, obviously,
y to satisfy this equation?

01:13:17.250 --> 01:13:22.560 align:middle line:90%


01:13:22.560 --> 01:13:24.560 align:middle line:90%
That's what we're looking for.

01:13:24.560 --> 01:13:26.560 align:middle line:90%
So this is existence.

01:13:26.560 --> 01:13:29.000 align:middle line:84%
The thing is that
what we will prove

01:13:29.000 --> 01:13:33.940 align:middle line:84%
is that there exists
some interval--

01:13:33.940 --> 01:13:35.540 align:middle line:90%
so we will prove the following.

01:13:35.540 --> 01:13:39.400 align:middle line:90%


01:13:39.400 --> 01:13:42.400 align:middle line:84%
So we prove the
following theorem,

01:13:42.400 --> 01:13:45.280 align:middle line:84%
which has many different
names, and it is

01:13:45.280 --> 01:13:46.730 align:middle line:90%
attributed to various people.

01:13:46.730 --> 01:13:50.360 align:middle line:90%


01:13:50.360 --> 01:13:52.220 align:middle line:90%
But it's I guess.

01:13:52.220 --> 01:13:57.200 align:middle line:90%


01:13:57.200 --> 01:14:08.080 align:middle line:84%
it's most often named the
Picard-Lindelöf theorem.

01:14:08.080 --> 01:14:18.920 align:middle line:84%
And so this is that
given f and g as above,

01:14:18.920 --> 01:14:23.840 align:middle line:84%
so f has to be differentiable
and the derivative continuous g

01:14:23.840 --> 01:14:25.300 align:middle line:90%
just has to be continuous.

01:14:25.300 --> 01:14:28.160 align:middle line:90%


01:14:28.160 --> 01:14:43.880 align:middle line:84%
Then for any a, there exists a
delta greater than 0 such that--

01:14:43.880 --> 01:14:47.360 align:middle line:90%


01:14:47.360 --> 01:14:54.480 align:middle line:84%
and a solution to this
differential equation

01:14:54.480 --> 01:15:05.320 align:middle line:84%
is ODE on the interval
from minus delta to delta.

01:15:05.320 --> 01:15:12.440 align:middle line:84%
So we proved that there exists
a solution near the origin.

01:15:12.440 --> 01:15:15.960 align:middle line:84%
The thing is that a
solution may blow up.

01:15:15.960 --> 01:15:19.580 align:middle line:84%
So it may not exist on
a very long interval.

01:15:19.580 --> 01:15:21.540 align:middle line:84%
It may just exist
on a small interval.

01:15:21.540 --> 01:15:25.200 align:middle line:90%
It's all depending on f and g.

01:15:25.200 --> 01:15:28.880 align:middle line:84%
But in particular,
will depend on f.

01:15:28.880 --> 01:15:42.000 align:middle line:84%
And that moreover,
it is unique, meaning

01:15:42.000 --> 01:15:45.680 align:middle line:84%
that if you take
another solution

01:15:45.680 --> 01:15:50.720 align:middle line:84%
defined on the same interval,
then it must be that solution.

01:15:50.720 --> 01:16:00.080 align:middle line:84%
And so now I just have a
minute to-- but we will

01:16:00.080 --> 01:16:02.120 align:middle line:90%
prove this next time anyway.

01:16:02.120 --> 01:16:07.780 align:middle line:84%
But I just want to, as
a teaser, if you will,

01:16:07.780 --> 01:16:19.480 align:middle line:84%
I will just say that
the proof of this

01:16:19.480 --> 01:16:25.260 align:middle line:84%
uses the contraction
mapping theorem.

01:16:25.260 --> 01:16:35.460 align:middle line:90%


01:16:35.460 --> 01:16:38.480 align:middle line:84%
Maybe I will remind
you what it is.

01:16:38.480 --> 01:16:53.160 align:middle line:84%
So recall that the
contraction mapping theorem

01:16:53.160 --> 01:16:54.671 align:middle line:90%
is the following--

01:16:54.671 --> 01:16:58.280 align:middle line:90%


01:16:58.280 --> 01:17:03.560 align:middle line:84%
that suppose you take a
metric space x and d--

01:17:03.560 --> 01:17:07.800 align:middle line:84%
so D is the metric,
x is the space--

01:17:07.800 --> 01:17:12.030 align:middle line:84%
and suppose you take a
map from x to itself.

01:17:12.030 --> 01:17:15.200 align:middle line:90%


01:17:15.200 --> 01:17:18.440 align:middle line:84%
So then T is a map
from x to itself.

01:17:18.440 --> 01:17:25.590 align:middle line:84%
T is said to be a
contracting map.

01:17:25.590 --> 01:17:32.520 align:middle line:90%


01:17:32.520 --> 01:17:37.560 align:middle line:84%
If there exists some
constant, that constant--

01:17:37.560 --> 01:17:38.720 align:middle line:90%
that's key.

01:17:38.720 --> 01:17:42.040 align:middle line:84%
It has to be
strictly less than 1

01:17:42.040 --> 01:17:47.800 align:middle line:84%
so that if you measure
distances between the images,

01:17:47.800 --> 01:17:52.560 align:middle line:84%
so for any x and
y in capital X--

01:17:52.560 --> 01:17:56.440 align:middle line:84%
this is for all x
and y in capital

01:17:56.440 --> 01:18:01.440 align:middle line:84%
X. If you look at the distance
between the images of these two

01:18:01.440 --> 01:18:06.600 align:middle line:84%
points, then it's less than
or equal to this constant that

01:18:06.600 --> 01:18:12.200 align:middle line:84%
is strictly less
than 1, like this.

01:18:12.200 --> 01:18:15.760 align:middle line:90%
So that's a contracting map.

01:18:15.760 --> 01:18:17.920 align:middle line:84%
And the contracting
mapping theorem

01:18:17.920 --> 01:18:21.200 align:middle line:84%
that we prove, I'll remind
you about it again next time,

01:18:21.200 --> 01:18:25.120 align:middle line:84%
but just the contracting
mapping theorem

01:18:25.120 --> 01:18:27.760 align:middle line:84%
that we proved is
that-- so we proved

01:18:27.760 --> 01:18:30.200 align:middle line:84%
the following theorem, which
is a contracting mapping

01:18:30.200 --> 01:18:43.520 align:middle line:84%
theorem, that if x here
is Cauchy complete,

01:18:43.520 --> 01:19:00.000 align:middle line:84%
and T from x to x is
a contracting map,

01:19:00.000 --> 01:19:05.770 align:middle line:90%
then T has a unique.

01:19:05.770 --> 01:19:08.360 align:middle line:90%


01:19:08.360 --> 01:19:09.220 align:middle line:90%
fixed point.

01:19:09.220 --> 01:19:14.940 align:middle line:90%


01:19:14.940 --> 01:19:18.980 align:middle line:84%
So there exists a unique
one-- often write like this--

01:19:18.980 --> 01:19:31.040 align:middle line:84%
there exists one and only one
x0 so that this map takes x0

01:19:31.040 --> 01:19:31.820 align:middle line:90%
to itself.

01:19:31.820 --> 01:19:34.520 align:middle line:84%
So that's a contraction
mapping theorem.

01:19:34.520 --> 01:19:39.800 align:middle line:84%
And so it seems
like what does ODE

01:19:39.800 --> 01:19:42.920 align:middle line:84%
has to do with them,
this abstract concept

01:19:42.920 --> 01:19:44.760 align:middle line:90%
of a metric space?

01:19:44.760 --> 01:19:48.400 align:middle line:84%
So it's tied
together using this.

01:19:48.400 --> 01:19:52.320 align:middle line:90%
And then the space x, it's not--

01:19:52.320 --> 01:19:55.920 align:middle line:90%


01:19:55.920 --> 01:19:59.000 align:middle line:84%
you may think that that's close,
but it's not quite the case.

01:19:59.000 --> 01:20:01.960 align:middle line:84%
You may think that it's
like a continuous function

01:20:01.960 --> 01:20:04.280 align:middle line:90%
on an interval like this.

01:20:04.280 --> 01:20:07.680 align:middle line:90%
That's close.

01:20:07.680 --> 01:20:09.280 align:middle line:84%
You may think that
because that's

01:20:09.280 --> 01:20:11.640 align:middle line:84%
a space we've talked
about a lot, this

01:20:11.640 --> 01:20:13.320 align:middle line:90%
here, with this metric d.

01:20:13.320 --> 01:20:15.920 align:middle line:84%
We talked about with
this maximum distance.

01:20:15.920 --> 01:20:17.860 align:middle line:84%
It's not actually
quite the case.

01:20:17.860 --> 01:20:22.200 align:middle line:84%
It's a little bit more
complicated than this.

01:20:22.200 --> 01:20:25.360 align:middle line:84%
But x is related to
this because x here

01:20:25.360 --> 01:20:33.680 align:middle line:84%
will be a ball around the
function that is constant,

01:20:33.680 --> 01:20:39.200 align:middle line:84%
the function that is
constant a in this space.

01:20:39.200 --> 01:20:44.080 align:middle line:84%
And we have to choose
this R carefully.

01:20:44.080 --> 01:20:46.600 align:middle line:90%
And so that's a space x.

01:20:46.600 --> 01:20:49.940 align:middle line:84%
And now I haven't defined
the function the map g.

01:20:49.940 --> 01:20:51.500 align:middle line:90%
But we'll do that next time.

01:20:51.500 --> 01:20:54.080 align:middle line:84%
And I will remind
you about this also.

01:20:54.080 --> 01:20:56.310 align:middle line:90%
Any questions?

01:20:56.310 --> 01:21:02.000 align:middle line:90%