WEBVTT

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[SQUEAKING]

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[RUSTLING]

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[CLICKING]

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TOBIAS COLDING: OK.

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So let me first
remind you about--

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we'll be looking-- so last
time we were looking at-- we

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had a sequence of
functions on an interval I.

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And we have a function
f on that same interval.

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And then we talked about
two notions of convergence.

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One was the pointwise
convergence.

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So this meant that--

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so we say that this
sequence converges

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to f pointwise if,
for all x fixed,

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you're looking at the
sequence fn of x--

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so x is fixed--

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and that this here
converges to f of x.

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So that was the
pointwise convergence.

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And the second convergence
that we talked about

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was uniform convergence.

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So this is 2,
uniform convergence.

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And so we say that
this sequence here

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converges to f uniformly if,
for all epsilon greater than 0,

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there exists an N so that if
you're further out than N,

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then the difference
between fn of x and f of x

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is smaller than epsilon.

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And this here has
to hold for all x.

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And so, again, uniform refers
to that it's for all x.

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So it's uniform in x.

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And so there was
one example that

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was particularly illuminating.

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And that was that we
took-- so if I here

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was the integral from
0 to 1 and if we're

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looking at the function fn of x,
that was just x to the power n.

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And f of x is then the
function that is 0 unless--

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so 0 if x here is between
0 and strictly less than 1,

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and 1 if x is equal to 1.

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And so the picture was that--

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so the picture was that you
have this sequence here.

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They are defined on the
interval from 0 to 1.

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They all end up at 1.

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And then as n becomes
larger and larger,

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these functions become more and
more steep towards 1, like that.

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And so then we had that
this sequence fn converges

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to f pointwise,
because if you fixed

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x, then really these values
here converge either to--

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if x is not equal to 1,
then as n becomes large,

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they converge to 0.

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If n is 1, then the fn
of 1, that's always 1.

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So it's clear that it's
converging pointwise.

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But fn does not converge.

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Does not converge
to f uniformly.

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And the reason why it
didn't converge uniformly

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was that we saw that for each--

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by the intermediate
value theorem,

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if we were looking at 1/2 here,
then for each of the function

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there would be an xn so
that the value at xn was 1.

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Was a half, sorry.

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So you define xn so that
the value of this is a half.

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But now, if you're looking
f of x minus f of xn

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like that and if
this-- sorry-- is n,

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then this difference here
is actually just a half.

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And this difference
here should be small.

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If n was sufficiently large,
it should be small for all x.

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But it's not.

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We've used one particular
x to show that it wasn't.

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OK.

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That was just a quick
review of some of the things

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we talked about last time.

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Now, let's get to theorem.

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And so maybe also one more
thing about this example

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is that you see that these
functions here, these functions

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fn, they're all continuous.

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But the limit is not continuous.

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So pointwise.

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So note that-- so note that
pointwise convergence is not

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enough to guarantee that limits
of continuous functions--

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that the limit of continuous
function is continuous.

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OK.

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So that's what this
example illustrates.

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So now, instead, we have
the following theorem.

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So we have this interval,
and we have a sequence fn,

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and we have f all
defined on this interval.

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And if we assume that all of
these fn's are continuous,

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and b, we assume that
the convergence here,

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the convergence of
fn to f is uniform,

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then the claim is that then
f here is also continuous.

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OK.

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So let's try to prove that.

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So pointwise convergence
is not enough to guarantee

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that the limit is continuous.

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Uniform convergence is enough.

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Now, let's see.

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So let's prove that.

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So given epsilon greater than
0, there exists capital N such

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that if little n is bigger
or equal to capital N,

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then fn of dx minus f of x is
smaller than epsilon over 3

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for all x.

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This just follows that the
sequence converge uniformly.

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So this is the first thing.

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And the second thing is--

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so this was, since fn
converges to f uniformly.

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The second thing is that--

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so now we have n.

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This here holds for all n
bigger or equal to capital N.

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But in particular, it holds
for capital N. So now,

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since f capital
N is continuous--

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so this is a fixed
function now--

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then for any fixed x0, we
have that there exists a delta

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greater than 0, such that if x
minus x0 is smaller than delta,

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then this function-- the value
at these two points differ

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at most--

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so this is for the fn.

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The value at these two
points differ at most

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by epsilon over 3.

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So again, we have
a sequence, fn,

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that converges
uniformly to some f.

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We want to prove that
this f is continuous.

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So we just need to prove
that for each x0 fixed,

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it's continuous at x0.

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First, I'm using
that the sequence

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is converging uniformly.

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So given this epsilon,
there exists this capital N

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so that if you're further
out, then you have this.

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I'm not even going to use
the part that is further out.

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I'm just going to
pick this capital N.

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And so then I'm using that
this f capital N is continuous,

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and it's continuous at x0.

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So I have this.

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And so now we need to estimate--

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we now need to estimate
the difference.

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So what we're
really interested is

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in f, but the f
capital N, that's

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going to help us estimate the
difference between these two

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numbers.

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And so these two numbers--

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so x here, x0 was
this fixed point

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that we want to show that f
is continuous at that point.

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And the delta, well, the
delta came from f capital N.

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So we're looking at this
x, this [? closed, ?]

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where the delta was
given by f capital N.

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And now we use the
triangle inequality.

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So this difference here is--

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so you may as well think
about this one here.

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And you could compare it with
the value at the same point.

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So I'm just writing down--

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I'm writing this difference
down as a sum of things.

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And then afterwards, I use
the triangle inequality.

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So here, minus f
capital N of x0.

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And then I'm adding back this
here again f capital N of x0.

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And I'm comparing
this with f of x0.

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So you see that here, this is
really the same because here I'm

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subtracting this thing
that I didn't have,

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but I'm adding it back,
subtracting this thing that I

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didn't have, but
I'm adding it back.

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So I'm just left with those
two things, which is that.

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And so now we use the
triangle inequality,

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that this is now
bounded by f of x

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minus fN of x plus fN of x minus
f capital N of x0, like that,

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plus, and then f capital
N of x0 minus f of x0,

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with an absolute
value sign like that.

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Now, this thing here is
smaller than epsilon over 3.

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And that came from that it's
evaluated at the same point

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and the convergence was uniform.

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So it really was
the first part here.

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So that is less
than epsilon over 3.

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This one here comes from that
the difference between x and x0

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is less than delta
and that this function

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fN was continuous at x0.

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So this is another
epsilon over delta.

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This is this second part here.

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And then the last
here is, again,

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the same that gave
us this bound,

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namely that the
convergence was uniform

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and is evaluated
at the same point.

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So you have that.

00:15:37.580 --> 00:15:44.300 align:middle line:84%
And so what we've proven here
is that for this given x0,

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if the difference between x
and x0 is less than delta,

00:15:49.980 --> 00:15:53.480 align:middle line:84%
then the difference in the
images is less than epsilon.

00:15:53.480 --> 00:16:01.380 align:middle line:84%
So this means that the function
f is continuous at x0 and x0

00:16:01.380 --> 00:16:05.309 align:middle line:90%
was arbitrary.

00:16:05.309 --> 00:16:17.890 align:middle line:84%
Now, the first application of
this is that suppose you take--

00:16:17.890 --> 00:16:22.110 align:middle line:90%


00:16:22.110 --> 00:16:24.110 align:middle line:84%
suppose you're looking
at the following example.

00:16:24.110 --> 00:16:27.340 align:middle line:90%


00:16:27.340 --> 00:16:33.740 align:middle line:84%
xn of x is the sum
here from k equal to 0

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to n of xk over k factorial.

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Suppose you're looking
at xn like this.

00:16:43.330 --> 00:16:53.850 align:middle line:84%
Then the xn here of x,
they are all continuous.

00:16:53.850 --> 00:16:55.770 align:middle line:90%
They are sum of polynomials.

00:16:55.770 --> 00:16:57.570 align:middle line:84%
They're just a
polynomial, actually

00:16:57.570 --> 00:17:04.069 align:middle line:84%
the sum of what's called
homogeneous polynomial.

00:17:04.069 --> 00:17:06.410 align:middle line:84%
But they are
themselves polynomial.

00:17:06.410 --> 00:17:08.109 align:middle line:90%
So they are all continuous.

00:17:08.109 --> 00:17:12.730 align:middle line:90%


00:17:12.730 --> 00:17:15.410 align:middle line:90%
And Weierstrass M-test.

00:17:15.410 --> 00:17:27.089 align:middle line:84%
So by Weierstrass M-test
that we proved last time--

00:17:27.089 --> 00:17:30.370 align:middle line:90%


00:17:30.370 --> 00:17:33.010 align:middle line:84%
by Weierstrass M-test,
the convergence

00:17:33.010 --> 00:17:40.900 align:middle line:84%
here to E, where E here is
the exponential function.

00:17:40.900 --> 00:17:44.880 align:middle line:84%
So it's this power
series sum from k

00:17:44.880 --> 00:17:53.060 align:middle line:84%
equal to 0 to infinity of x to
the power k over k factorial.

00:17:53.060 --> 00:17:55.480 align:middle line:84%
This convergence
here is uniform.

00:17:55.480 --> 00:18:02.100 align:middle line:84%
It's uniform assuming that you
do it on a compact interval.

00:18:02.100 --> 00:18:18.820 align:middle line:84%
So it's uniform on any
fixed interval of the form,

00:18:18.820 --> 00:18:24.600 align:middle line:90%
say, minus L to L.

00:18:24.600 --> 00:18:27.120 align:middle line:84%
So if you're fixing
an interval like this,

00:18:27.120 --> 00:18:30.320 align:middle line:90%
then the convergence is uniform.

00:18:30.320 --> 00:18:36.160 align:middle line:84%
And so this means that since
these guys here are continuous,

00:18:36.160 --> 00:18:40.380 align:middle line:84%
then it implies that this
one here is also continuous.

00:18:40.380 --> 00:18:47.088 align:middle line:90%


00:18:47.088 --> 00:18:50.610 align:middle line:84%
So this is implied by the
theorem that we just proved.

00:18:50.610 --> 00:18:55.840 align:middle line:90%


00:18:55.840 --> 00:18:59.760 align:middle line:90%
So now this will--

00:18:59.760 --> 00:19:02.480 align:middle line:90%
uniform convergence.

00:19:02.480 --> 00:19:08.160 align:middle line:84%
There's another way of thinking
about uniform convergence that,

00:19:08.160 --> 00:19:13.490 align:middle line:90%
in a way, makes it more natural.

00:19:13.490 --> 00:19:16.900 align:middle line:90%


00:19:16.900 --> 00:19:21.120 align:middle line:84%
So remember that
if we looked at--

00:19:21.120 --> 00:19:22.920 align:middle line:84%
so if we take an
interval-- let's

00:19:22.920 --> 00:19:28.440 align:middle line:84%
say that this is an interval
from a to b. a and b

00:19:28.440 --> 00:19:31.200 align:middle line:90%
are real numbers.

00:19:31.200 --> 00:19:35.750 align:middle line:84%
Then we looked at the space
of continuous functions

00:19:35.750 --> 00:19:38.750 align:middle line:90%
on this interval.

00:19:38.750 --> 00:19:41.570 align:middle line:84%
And this space had
a natural metric.

00:19:41.570 --> 00:19:45.950 align:middle line:84%
So I'm using here that both
endpoints are included.

00:19:45.950 --> 00:19:50.380 align:middle line:84%
This space here has
a natural metric.

00:19:50.380 --> 00:19:56.830 align:middle line:90%


00:19:56.830 --> 00:20:02.270 align:middle line:84%
And that metric is that if
you take two functions--

00:20:02.270 --> 00:20:06.070 align:middle line:84%
two continuous functions--
on the interval, then

00:20:06.070 --> 00:20:09.310 align:middle line:84%
the distance between
these two functions

00:20:09.310 --> 00:20:21.270 align:middle line:84%
is just the max of the
difference between the two

00:20:21.270 --> 00:20:22.090 align:middle line:90%
functions.

00:20:22.090 --> 00:20:30.510 align:middle line:90%


00:20:30.510 --> 00:20:33.780 align:middle line:84%
The difference--
again, why is this?

00:20:33.780 --> 00:20:35.900 align:middle line:90%
The difference is continuous.

00:20:35.900 --> 00:20:39.620 align:middle line:84%
So this means that
the maximum is--

00:20:39.620 --> 00:20:41.040 align:middle line:90%
the difference is continuous.

00:20:41.040 --> 00:20:42.660 align:middle line:84%
So this is a
continuous function,

00:20:42.660 --> 00:20:45.740 align:middle line:84%
and it's still continuous
if you take absolute value.

00:20:45.740 --> 00:20:49.060 align:middle line:84%
And so this means that the
maximum by the extreme value

00:20:49.060 --> 00:20:50.105 align:middle line:90%
theorem is achieved.

00:20:50.105 --> 00:20:53.500 align:middle line:90%


00:20:53.500 --> 00:20:57.340 align:middle line:84%
And so this here was a
natural distance between them.

00:20:57.340 --> 00:21:02.300 align:middle line:84%
Now to say that
the sequence here--

00:21:02.300 --> 00:21:08.500 align:middle line:84%
to say that the sequence
fn is converging uniformly,

00:21:08.500 --> 00:21:12.340 align:middle line:84%
you can think about that
in terms of this distance.

00:21:12.340 --> 00:21:16.080 align:middle line:84%
So we have the
following proposition.

00:21:16.080 --> 00:21:21.260 align:middle line:90%


00:21:21.260 --> 00:21:30.060 align:middle line:84%
fn converge uniformly
to f if and only

00:21:30.060 --> 00:21:53.210 align:middle line:84%
if fn converges to f in the
metric space with this metric.

00:21:53.210 --> 00:21:56.290 align:middle line:90%


00:21:56.290 --> 00:21:59.060 align:middle line:90%
Now, why is this the case?

00:21:59.060 --> 00:22:01.420 align:middle line:90%
So this is just that--

00:22:01.420 --> 00:22:07.540 align:middle line:84%
so proof of that is really just
a one-liner because you see that

00:22:07.540 --> 00:22:08.620 align:middle line:90%
to say that--

00:22:08.620 --> 00:22:11.620 align:middle line:90%


00:22:11.620 --> 00:22:18.700 align:middle line:84%
so that f of x minus
fn of x is less than

00:22:18.700 --> 00:22:34.450 align:middle line:84%
or equal to epsilon for all x
if this here is the case, where

00:22:34.450 --> 00:22:42.250 align:middle line:84%
this is equivalent to saying
that the distance between fn

00:22:42.250 --> 00:22:48.270 align:middle line:84%
and an f is less than or
equal to epsilon for all x.

00:22:48.270 --> 00:22:51.930 align:middle line:90%


00:22:51.930 --> 00:22:54.850 align:middle line:84%
Because if this is
the case for all x,

00:22:54.850 --> 00:22:57.830 align:middle line:84%
then the maximum is less
than or equal to epsilon.

00:22:57.830 --> 00:22:59.410 align:middle line:90%
This was the maximum.

00:22:59.410 --> 00:23:02.090 align:middle line:84%
And on the other hand, if
the maximum, well, then it

00:23:02.090 --> 00:23:04.090 align:middle line:90%
holds for each x.

00:23:04.090 --> 00:23:06.130 align:middle line:90%
So this is sort of a tautology.

00:23:06.130 --> 00:23:08.910 align:middle line:90%


00:23:08.910 --> 00:23:14.250 align:middle line:84%
And so now we see, of course,
that if the sequence-- so you

00:23:14.250 --> 00:23:15.730 align:middle line:90%
have that.

00:23:15.730 --> 00:23:23.050 align:middle line:84%
But this means-- so this
means that if the sequence--

00:23:23.050 --> 00:23:36.660 align:middle line:84%
therefore, if the sequence fn
converges to f uniformly, well,

00:23:36.660 --> 00:23:39.760 align:middle line:84%
then it means that
for all epsilon,

00:23:39.760 --> 00:23:44.040 align:middle line:84%
if we're sufficiently far
out, then this here can be--

00:23:44.040 --> 00:23:47.180 align:middle line:84%
for any given epsilon, if
you're sufficiently far out,

00:23:47.180 --> 00:23:49.828 align:middle line:84%
this here can be made less
than or equal to epsilon, which

00:23:49.828 --> 00:23:51.620 align:middle line:84%
means that this error
can be made less than

00:23:51.620 --> 00:23:54.720 align:middle line:84%
or equal to epsilon if
you're sufficiently far out.

00:23:54.720 --> 00:23:57.600 align:middle line:84%
So you see that if this
converges uniformly, then

00:23:57.600 --> 00:24:04.680 align:middle line:84%
it implies that this
thing here converges to 0.

00:24:04.680 --> 00:24:06.800 align:middle line:84%
But that's exactly
what it means,

00:24:06.800 --> 00:24:14.010 align:middle line:84%
that this sequence fn converges
to f in the metric space.

00:24:14.010 --> 00:24:23.040 align:middle line:90%


00:24:23.040 --> 00:24:24.410 align:middle line:90%
And the other way around.

00:24:24.410 --> 00:24:27.280 align:middle line:90%


00:24:27.280 --> 00:24:30.840 align:middle line:84%
If this sequence
converges, fn converges

00:24:30.840 --> 00:24:33.000 align:middle line:84%
to f in the metric
space, this is

00:24:33.000 --> 00:24:36.480 align:middle line:84%
equivalent to saying
that this here goes to 0.

00:24:36.480 --> 00:24:39.560 align:middle line:84%
But if this here
goes to 0, this means

00:24:39.560 --> 00:24:42.480 align:middle line:84%
that if you're sufficiently
far out-- for a given

00:24:42.480 --> 00:24:44.360 align:middle line:84%
epsilon, if you're
sufficiently far out,

00:24:44.360 --> 00:24:46.980 align:middle line:84%
this here is less than
or equal to epsilon.

00:24:46.980 --> 00:24:49.400 align:middle line:84%
But it means that this
here is less than epsilon.

00:24:49.400 --> 00:24:54.080 align:middle line:84%
So that means it really
converges uniformly.

00:24:54.080 --> 00:24:56.445 align:middle line:90%
OK.

00:24:56.445 --> 00:25:01.920 align:middle line:84%
And that's in a way that
makes it much more natural.

00:25:01.920 --> 00:25:04.680 align:middle line:90%
I mean, yeah.

00:25:04.680 --> 00:25:11.920 align:middle line:84%
So it makes uniform
convergence much more natural.

00:25:11.920 --> 00:25:16.840 align:middle line:84%
So now let's prove
the next term.

00:25:16.840 --> 00:25:21.040 align:middle line:84%
So for this theorem,
we're going to think

00:25:21.040 --> 00:25:27.570 align:middle line:84%
about uniform convergence
in terms of this metric

00:25:27.570 --> 00:25:31.510 align:middle line:84%
and in terms of convergence
in this metric space.

00:25:31.510 --> 00:25:36.210 align:middle line:84%
So this theorem
is the next thing.

00:25:36.210 --> 00:25:41.990 align:middle line:84%
Let's say that if you take
an interval from a to b

00:25:41.990 --> 00:25:45.350 align:middle line:84%
and you're looking at
the continuous function

00:25:45.350 --> 00:25:50.110 align:middle line:84%
and you equip it with this
metric that we talked about,

00:25:50.110 --> 00:25:54.290 align:middle line:84%
then this here is this space,
which is a metric space.

00:25:54.290 --> 00:26:03.300 align:middle line:84%
So this metric space
is a Cauchy complete.

00:26:03.300 --> 00:26:13.250 align:middle line:90%


00:26:13.250 --> 00:26:16.390 align:middle line:84%
So remember, Cauchy
complete in a metric space

00:26:16.390 --> 00:26:20.670 align:middle line:84%
means that if you take a
Cauchy sequence-- so just let

00:26:20.670 --> 00:26:22.950 align:middle line:90%
me just recall here over here.

00:26:22.950 --> 00:26:24.590 align:middle line:90%
So Cauchy.

00:26:24.590 --> 00:26:34.070 align:middle line:84%
So if x comma d
is a metric space,

00:26:34.070 --> 00:27:00.270 align:middle line:84%
then Cauchy complete means
that any Cauchy sequence

00:27:00.270 --> 00:27:01.450 align:middle line:90%
is convergent.

00:27:01.450 --> 00:27:07.030 align:middle line:90%


00:27:07.030 --> 00:27:10.490 align:middle line:84%
That's what it means to
be a Cauchy complete.

00:27:10.490 --> 00:27:17.070 align:middle line:84%
And of course, an example of
a Cauchy complete metric space

00:27:17.070 --> 00:27:21.610 align:middle line:84%
was just if we took R
with the usual metric.

00:27:21.610 --> 00:27:26.532 align:middle line:90%


00:27:26.532 --> 00:27:29.240 align:middle line:90%
So what we have here is--

00:27:29.240 --> 00:27:30.520 align:middle line:90%
so let's try to prove this.

00:27:30.520 --> 00:27:33.460 align:middle line:90%


00:27:33.460 --> 00:27:35.000 align:middle line:90%
So we need to prove.

00:27:35.000 --> 00:27:38.340 align:middle line:90%
So this here is now--

00:27:38.340 --> 00:27:51.460 align:middle line:84%
we need to prove that if this
here is a Cauchy sequence,

00:27:51.460 --> 00:28:04.566 align:middle line:84%
then there exists a function
that is also continuous.

00:28:04.566 --> 00:28:07.580 align:middle line:90%


00:28:07.580 --> 00:28:22.050 align:middle line:84%
And so this sequence here
converging to f in the metric d.

00:28:22.050 --> 00:28:23.930 align:middle line:90%
That's what we need to prove.

00:28:23.930 --> 00:28:31.890 align:middle line:84%
So in particular, we need to
first construct a function, f.

00:28:31.890 --> 00:28:36.090 align:middle line:90%


00:28:36.090 --> 00:28:40.320 align:middle line:84%
So now let's try first
to construct a function.

00:28:40.320 --> 00:28:47.890 align:middle line:90%


00:28:47.890 --> 00:29:01.400 align:middle line:84%
So we first construct
f as follows.

00:29:01.400 --> 00:29:07.090 align:middle line:90%


00:29:07.090 --> 00:29:11.570 align:middle line:90%
Well, if you fix x--

00:29:11.570 --> 00:29:16.490 align:middle line:84%
so x is something, a
point in the interval.

00:29:16.490 --> 00:29:20.590 align:middle line:84%
And now look at
this sequence fn.

00:29:20.590 --> 00:29:24.490 align:middle line:90%
This is now a regular sequence.

00:29:24.490 --> 00:29:28.010 align:middle line:84%
But if you're looking
at the sequence,

00:29:28.010 --> 00:29:38.090 align:middle line:84%
then we have that fn of x minus
fm of x, if you have n and m

00:29:38.090 --> 00:29:41.650 align:middle line:84%
like this, then
the difference here

00:29:41.650 --> 00:29:47.530 align:middle line:84%
is less than or equal
to the max where

00:29:47.530 --> 00:29:59.570 align:middle line:84%
this is for all z in
the interval of fn

00:29:59.570 --> 00:30:11.386 align:middle line:90%
of z minus fm of z, like that.

00:30:11.386 --> 00:30:17.520 align:middle line:84%
Because of course, it's like
in particular if z was x.

00:30:17.520 --> 00:30:18.830 align:middle line:90%
So you have clearly this.

00:30:18.830 --> 00:30:21.720 align:middle line:90%


00:30:21.720 --> 00:30:23.680 align:middle line:90%
But now you see that--

00:30:23.680 --> 00:30:27.420 align:middle line:90%
so I claim that this means--

00:30:27.420 --> 00:30:43.040 align:middle line:84%
so I claim that this implies
that this sequence here--

00:30:43.040 --> 00:30:45.720 align:middle line:90%
sorry, this sequence here.

00:30:45.720 --> 00:30:50.160 align:middle line:84%
fn of x, this
sequence here, which

00:30:50.160 --> 00:30:53.000 align:middle line:90%
is a sequence of real numbers--

00:30:53.000 --> 00:30:55.480 align:middle line:90%
these here are real numbers--

00:30:55.480 --> 00:31:06.350 align:middle line:84%
that this here is a Cauchy
sequence of real numbers.

00:31:06.350 --> 00:31:13.120 align:middle line:90%


00:31:13.120 --> 00:31:16.610 align:middle line:90%
Why is that the case?

00:31:16.610 --> 00:31:24.250 align:middle line:84%
Well, it's the case
because given--

00:31:24.250 --> 00:31:28.150 align:middle line:90%
so this is just because given--

00:31:28.150 --> 00:31:43.070 align:middle line:84%
so this is the case because
given epsilon greater than 0,

00:31:43.070 --> 00:31:56.300 align:middle line:84%
since fn is a Cauchy sequence
in the metric space--

00:31:56.300 --> 00:32:00.434 align:middle line:90%


00:32:00.434 --> 00:32:02.710 align:middle line:90%
in this metric space--

00:32:02.710 --> 00:32:14.590 align:middle line:84%
then there exist capital N so
that if little n and little m

00:32:14.590 --> 00:32:17.910 align:middle line:84%
are bigger than capital
N, then the difference

00:32:17.910 --> 00:32:19.530 align:middle line:90%
between these guys--

00:32:19.530 --> 00:32:23.410 align:middle line:84%
sorry, the difference
between this function here

00:32:23.410 --> 00:32:28.890 align:middle line:84%
and that function is
less than epsilon.

00:32:28.890 --> 00:32:32.230 align:middle line:84%
This is because they
were Cauchy sequence.

00:32:32.230 --> 00:32:35.450 align:middle line:84%
And so now this thing
here is, of course--

00:32:35.450 --> 00:32:38.090 align:middle line:84%
this thing here, that's
what we just saw.

00:32:38.090 --> 00:32:39.990 align:middle line:90%
This is the maximum.

00:32:39.990 --> 00:32:48.950 align:middle line:84%
So this is bigger than when you
evaluate it in just one point,

00:32:48.950 --> 00:32:51.390 align:middle line:90%
like that.

00:32:51.390 --> 00:33:00.510 align:middle line:84%
And so this proof
that when x is fixed,

00:33:00.510 --> 00:33:04.870 align:middle line:84%
these guys here is a Cauchy
sequence of real numbers.

00:33:04.870 --> 00:33:06.270 align:middle line:90%
So now we use--

00:33:06.270 --> 00:33:20.740 align:middle line:84%
since R here is
Cauchy complete and fn

00:33:20.740 --> 00:33:29.340 align:middle line:84%
of x is a Cauchy
sequence, then it

00:33:29.340 --> 00:33:37.340 align:middle line:84%
means that the sequence fn of
x, that this is converging,

00:33:37.340 --> 00:33:42.860 align:middle line:84%
and it's converging to some
number, to just one number.

00:33:42.860 --> 00:33:49.540 align:middle line:84%
And that number we
can call f of x.

00:33:49.540 --> 00:33:55.420 align:middle line:84%
So we just defined f to be
the limit of the sequence.

00:33:55.420 --> 00:33:58.220 align:middle line:84%
And that's well defined because
there's just one number.

00:33:58.220 --> 00:34:02.140 align:middle line:84%
So for each x it
gives you a number.

00:34:02.140 --> 00:34:03.020 align:middle line:90%
OK.

00:34:03.020 --> 00:34:04.970 align:middle line:90%
So now what we have proven is--

00:34:04.970 --> 00:34:08.340 align:middle line:90%


00:34:08.340 --> 00:34:11.139 align:middle line:90%
so now we have a candidate.

00:34:11.139 --> 00:34:16.090 align:middle line:90%
So namely, we have shown that--

00:34:16.090 --> 00:34:18.889 align:middle line:84%
so now what we
have proven here is

00:34:18.889 --> 00:34:24.330 align:middle line:90%
that we have found a function.

00:34:24.330 --> 00:34:29.610 align:middle line:84%
So we have now proven
that this sequence here is

00:34:29.610 --> 00:34:32.889 align:middle line:90%
converging to some function f.

00:34:32.889 --> 00:34:35.830 align:middle line:84%
The convergence
is just pointwise.

00:34:35.830 --> 00:34:39.409 align:middle line:90%


00:34:39.409 --> 00:34:44.130 align:middle line:84%
And we don't know whether this
function is continuous or not.

00:34:44.130 --> 00:34:45.670 align:middle line:90%
The convergence is pointwise.

00:34:45.670 --> 00:34:52.130 align:middle line:84%
This is just because
for each fixed x, f of x

00:34:52.130 --> 00:34:58.636 align:middle line:84%
was defined so that it was a
limit of these guys, fn of x.

00:34:58.636 --> 00:35:04.290 align:middle line:84%
So now we need to promote this
convergence that was pointwise,

00:35:04.290 --> 00:35:06.930 align:middle line:84%
and we need to promote
the convergence

00:35:06.930 --> 00:35:08.830 align:middle line:90%
to uniform convergence.

00:35:08.830 --> 00:35:11.370 align:middle line:90%


00:35:11.370 --> 00:35:12.590 align:middle line:90%
So now we need--

00:35:12.590 --> 00:35:18.650 align:middle line:90%


00:35:18.650 --> 00:35:22.970 align:middle line:84%
so given epsilon
greater than 0, again,

00:35:22.970 --> 00:35:27.410 align:middle line:84%
since these guys,
fn, was a Cauchy

00:35:27.410 --> 00:35:38.130 align:middle line:90%
sequence in the metric space--

00:35:38.130 --> 00:35:43.410 align:middle line:90%
in this metric space--

00:35:43.410 --> 00:35:52.650 align:middle line:84%
then as we saw over there,
there exists capital N

00:35:52.650 --> 00:35:59.090 align:middle line:84%
so that if little n and little m
are bigger than this capital N,

00:35:59.090 --> 00:36:05.170 align:middle line:84%
then the difference
between these two, fn

00:36:05.170 --> 00:36:15.680 align:middle line:84%
of x minus fm of x, this thing
here, is less than or equal to--

00:36:15.680 --> 00:36:18.320 align:middle line:90%
and I'm using epsilon over 2--

00:36:18.320 --> 00:36:19.380 align:middle line:90%
for all x.

00:36:19.380 --> 00:36:26.456 align:middle line:90%


00:36:26.456 --> 00:36:30.120 align:middle line:90%
So you have that.

00:36:30.120 --> 00:36:36.960 align:middle line:84%
But now this here
holds for all m and n.

00:36:36.960 --> 00:36:39.960 align:middle line:90%
Let's just fix n.

00:36:39.960 --> 00:36:41.800 align:middle line:90%
And now we can use that.

00:36:41.800 --> 00:36:43.360 align:middle line:90%
It's still true.

00:36:43.360 --> 00:36:45.720 align:middle line:90%
I can still let m vary.

00:36:45.720 --> 00:36:56.400 align:middle line:84%
And so if you let m go-- so
fixed n bigger than capital N.

00:36:56.400 --> 00:37:04.870 align:middle line:90%
And let little m go to infinity.

00:37:04.870 --> 00:37:09.590 align:middle line:84%
Well, this has just
some fixed number.

00:37:09.590 --> 00:37:14.430 align:middle line:84%
But as m goes to infinity,
this here goes to f of x.

00:37:14.430 --> 00:37:17.510 align:middle line:84%
And so since this difference
is always less than or equal

00:37:17.510 --> 00:37:22.630 align:middle line:84%
to epsilon over 2,
it's also the case

00:37:22.630 --> 00:37:29.870 align:middle line:84%
that the difference
here of the limit

00:37:29.870 --> 00:37:33.930 align:middle line:84%
is less than or equal
to epsilon over 2.

00:37:33.930 --> 00:37:36.330 align:middle line:90%
So you have this here for all x.

00:37:36.330 --> 00:37:41.110 align:middle line:90%


00:37:41.110 --> 00:37:48.270 align:middle line:84%
This is just letting m
go through to the limit.

00:37:48.270 --> 00:37:54.790 align:middle line:84%
But this, of course, says
that the max, if you will--

00:37:54.790 --> 00:37:55.770 align:middle line:90%
so you have that.

00:37:55.770 --> 00:38:01.270 align:middle line:84%
So this implies
that the max of fn

00:38:01.270 --> 00:38:07.190 align:middle line:84%
of x minus f of x,
that this thing here,

00:38:07.190 --> 00:38:12.390 align:middle line:84%
where x is now in this interval,
that this is less than or equal

00:38:12.390 --> 00:38:12.920 align:middle line:90%
to epsilon.

00:38:12.920 --> 00:38:15.942 align:middle line:90%


00:38:15.942 --> 00:38:17.670 align:middle line:90%
But this is the same.

00:38:17.670 --> 00:38:24.210 align:middle line:84%
This here is just the
distance between fn and f.

00:38:24.210 --> 00:38:28.790 align:middle line:84%
So say that this distance
here is less than--

00:38:28.790 --> 00:38:31.210 align:middle line:90%
I guess I had epsilon over 2.

00:38:31.210 --> 00:38:36.990 align:middle line:84%
So it means that this thing here
is strictly less than epsilon.

00:38:36.990 --> 00:38:39.290 align:middle line:84%
It's actually less than or
equal to epsilon over 2.

00:38:39.290 --> 00:38:41.870 align:middle line:84%
So it's strictly
less than epsilon.

00:38:41.870 --> 00:38:45.810 align:middle line:84%
But that's exactly what it
means for this sequence here.

00:38:45.810 --> 00:38:48.350 align:middle line:90%
So this is the same.

00:38:48.350 --> 00:39:01.650 align:middle line:84%
This is the same as saying that
fn converges to f uniformly.

00:39:01.650 --> 00:39:10.040 align:middle line:90%


00:39:10.040 --> 00:39:13.180 align:middle line:84%
Sorry, here, i should
have taken the sup.

00:39:13.180 --> 00:39:16.380 align:middle line:84%
The reason why I
should take the sup

00:39:16.380 --> 00:39:21.200 align:middle line:84%
here is that f is
just a function.

00:39:21.200 --> 00:39:24.600 align:middle line:84%
It's not necessarily
continuous at this stage.

00:39:24.600 --> 00:39:27.420 align:middle line:84%
But it was clearly
the case with the sup.

00:39:27.420 --> 00:39:30.940 align:middle line:84%
So the maximum a priori
may not be achieved yet.

00:39:30.940 --> 00:39:34.340 align:middle line:84%
But now you see
that they converge.

00:39:34.340 --> 00:39:39.460 align:middle line:84%
These fn converge
to f uniformly.

00:39:39.460 --> 00:39:42.760 align:middle line:84%
And these guys here
was continuous.

00:39:42.760 --> 00:39:45.940 align:middle line:90%
These are continuous.

00:39:45.940 --> 00:39:49.060 align:middle line:84%
So this implies
that by this theorem

00:39:49.060 --> 00:39:54.700 align:middle line:84%
we just proved, that
f is also continuous.

00:39:54.700 --> 00:39:57.060 align:middle line:84%
And so you see that--
so now you have

00:39:57.060 --> 00:40:00.520 align:middle line:84%
that the limit is
indeed in the space.

00:40:00.520 --> 00:40:06.180 align:middle line:84%
And we already proved here that
the convergence to this limit

00:40:06.180 --> 00:40:11.600 align:middle line:84%
is uniform, which means
that it's in the metric.

00:40:11.600 --> 00:40:15.375 align:middle line:90%


00:40:15.375 --> 00:40:18.840 align:middle line:90%
The next thing is that--

00:40:18.840 --> 00:40:22.660 align:middle line:84%
so this here was just a
little bit different way

00:40:22.660 --> 00:40:24.660 align:middle line:84%
of thinking about
uniform convergence,

00:40:24.660 --> 00:40:28.780 align:middle line:84%
that you think about it more
abstractly as a convergence

00:40:28.780 --> 00:40:30.200 align:middle line:90%
in a metric space.

00:40:30.200 --> 00:40:33.020 align:middle line:84%
And it's a useful way
of thinking about it.

00:40:33.020 --> 00:40:34.700 align:middle line:84%
The next thing we
want to look at

00:40:34.700 --> 00:40:41.740 align:middle line:84%
is how this uniform
convergence gives you

00:40:41.740 --> 00:40:44.640 align:middle line:90%
a way of computing things.

00:40:44.640 --> 00:40:50.020 align:middle line:84%
So in particular, if you
have some power series.

00:40:50.020 --> 00:40:54.340 align:middle line:84%
And we talked about that
a little bit last time.

00:40:54.340 --> 00:40:56.580 align:middle line:90%
We didn't prove anything.

00:40:56.580 --> 00:41:00.180 align:middle line:84%
But one of the
motivation for this

00:41:00.180 --> 00:41:03.570 align:middle line:84%
is that suppose you take
a power series, like this.

00:41:03.570 --> 00:41:08.220 align:middle line:90%


00:41:08.220 --> 00:41:11.050 align:middle line:84%
And we'll return to
this in just a second.

00:41:11.050 --> 00:41:13.930 align:middle line:84%
But suppose you take a
power series, like this,

00:41:13.930 --> 00:41:17.470 align:middle line:84%
and you are inside the
radius of convergence.

00:41:17.470 --> 00:41:21.790 align:middle line:90%
So inside radius of convergence.

00:41:21.790 --> 00:41:26.850 align:middle line:90%


00:41:26.850 --> 00:41:29.250 align:middle line:84%
So you know that this
thing here makes sense,

00:41:29.250 --> 00:41:33.410 align:middle line:84%
that this, for each
x, gives you a number.

00:41:33.410 --> 00:41:35.070 align:middle line:90%
And so it gives you a function.

00:41:35.070 --> 00:41:37.450 align:middle line:84%
And so you're
interested in, what

00:41:37.450 --> 00:41:39.770 align:middle line:84%
is the derivative
of that function?

00:41:39.770 --> 00:41:43.470 align:middle line:84%
And what is the integral
of that function?

00:41:43.470 --> 00:41:46.730 align:middle line:84%
How do we integrate it, and
how do we take the derivative?

00:41:46.730 --> 00:41:48.530 align:middle line:84%
And the thing that
worries you a bit

00:41:48.530 --> 00:41:52.750 align:middle line:84%
is that if it was just a finite
sum, it would be trivial.

00:41:52.750 --> 00:41:54.850 align:middle line:90%
But it's an infinite sum.

00:41:54.850 --> 00:41:57.070 align:middle line:90%
And so is it OK--

00:41:57.070 --> 00:42:00.330 align:middle line:84%
so the natural
question is, is it OK?

00:42:00.330 --> 00:42:02.760 align:middle line:84%
If you want to take
the derivative,

00:42:02.760 --> 00:42:06.960 align:middle line:84%
can you interchange
this infinite sum

00:42:06.960 --> 00:42:08.920 align:middle line:90%
with taking derivative?

00:42:08.920 --> 00:42:12.920 align:middle line:84%
And likewise, if you want to
integrate this infinite sum,

00:42:12.920 --> 00:42:18.640 align:middle line:84%
is it OK to interchange
the infinite sum taking

00:42:18.640 --> 00:42:19.920 align:middle line:90%
the integral?

00:42:19.920 --> 00:42:23.840 align:middle line:90%
And the answer is, it's OK.

00:42:23.840 --> 00:42:25.720 align:middle line:90%
So let's see that.

00:42:25.720 --> 00:42:27.960 align:middle line:90%
So we do this.

00:42:27.960 --> 00:42:29.880 align:middle line:84%
So we have two
versions of this, one

00:42:29.880 --> 00:42:32.680 align:middle line:84%
that's dealing with
taking integrals

00:42:32.680 --> 00:42:36.060 align:middle line:84%
and another version that
deals with taking derivatives.

00:42:36.060 --> 00:42:45.300 align:middle line:90%


00:42:45.300 --> 00:42:49.440 align:middle line:84%
And so the first
thing is that I take--

00:42:49.440 --> 00:42:52.960 align:middle line:84%
so the first theorem
is the following,

00:42:52.960 --> 00:42:56.860 align:middle line:84%
that I have some
interval from a to b.

00:42:56.860 --> 00:43:02.200 align:middle line:90%


00:43:02.200 --> 00:43:08.000 align:middle line:84%
And then I have a
sequence of functions, fn,

00:43:08.000 --> 00:43:13.000 align:middle line:90%
that are integrable.

00:43:13.000 --> 00:43:17.920 align:middle line:84%
They may not be continuous,
they're just integrable.

00:43:17.920 --> 00:43:23.320 align:middle line:84%
So in particular,
they are bounded.

00:43:23.320 --> 00:43:32.380 align:middle line:84%
And then I have that fn here
converges to f uniformly.

00:43:32.380 --> 00:43:37.720 align:middle line:90%


00:43:37.720 --> 00:43:41.060 align:middle line:90%
And I want to prove that--

00:43:41.060 --> 00:43:52.220 align:middle line:84%
so the claim is that
fn is also integrable.

00:43:52.220 --> 00:43:55.280 align:middle line:90%


00:43:55.280 --> 00:44:07.210 align:middle line:84%
And the integral of f is equal
to the limit of these integrals.

00:44:07.210 --> 00:44:20.950 align:middle line:90%


00:44:20.950 --> 00:44:24.390 align:middle line:84%
Sorry, in particular, of
course, those integrals

00:44:24.390 --> 00:44:26.230 align:middle line:90%
here has a limit.

00:44:26.230 --> 00:44:27.530 align:middle line:90%
It's part of the statement.

00:44:27.530 --> 00:44:51.690 align:middle line:90%


00:44:51.690 --> 00:44:52.190 align:middle line:90%
OK.

00:44:52.190 --> 00:44:58.060 align:middle line:90%


00:44:58.060 --> 00:44:58.560 align:middle line:90%
Right.

00:44:58.560 --> 00:45:02.540 align:middle line:90%


00:45:02.540 --> 00:45:05.710 align:middle line:84%
So what do we want to--
what do we need to prove?

00:45:05.710 --> 00:45:06.210 align:middle line:90%
So prove.

00:45:06.210 --> 00:45:10.280 align:middle line:90%


00:45:10.280 --> 00:45:12.220 align:middle line:90%
So we want to show--

00:45:12.220 --> 00:45:21.200 align:middle line:84%
so we first want to show
that f is integrable.

00:45:21.200 --> 00:45:26.420 align:middle line:90%


00:45:26.420 --> 00:45:28.900 align:middle line:84%
And we had our criteria
for doing that.

00:45:28.900 --> 00:45:31.840 align:middle line:90%
So we're using the criteria.

00:45:31.840 --> 00:45:42.210 align:middle line:84%
So we can use that
all we need to show--

00:45:42.210 --> 00:45:47.580 align:middle line:90%


00:45:47.580 --> 00:45:59.060 align:middle line:84%
to show-- is the following, that
given epsilon greater than 0,

00:45:59.060 --> 00:46:06.900 align:middle line:84%
there exists a partition
P of the interval from a

00:46:06.900 --> 00:46:18.900 align:middle line:84%
to b, so that the upper sum of
f with respect to this partition

00:46:18.900 --> 00:46:25.300 align:middle line:84%
minus the lower sum of f with
respect to the same partition,

00:46:25.300 --> 00:46:28.620 align:middle line:84%
that this thing here
is less than epsilon.

00:46:28.620 --> 00:46:30.000 align:middle line:90%
That's all we need to prove.

00:46:30.000 --> 00:46:31.300 align:middle line:90%
We need to prove it.

00:46:31.300 --> 00:46:33.540 align:middle line:84%
For each epsilon,
we need to prove

00:46:33.540 --> 00:46:35.240 align:middle line:90%
that there exists a partition.

00:46:35.240 --> 00:46:38.820 align:middle line:84%
So if we have that,
then we already

00:46:38.820 --> 00:46:43.580 align:middle line:90%
know that then f is integrable.

00:46:43.580 --> 00:46:46.480 align:middle line:84%
So that's just achieved
this first task.

00:46:46.480 --> 00:46:48.720 align:middle line:84%
And then, afterwards,
we need to prove that.

00:46:48.720 --> 00:47:05.923 align:middle line:90%


00:47:05.923 --> 00:47:06.423 align:middle line:90%
Right.

00:47:06.423 --> 00:47:06.930 align:middle line:90%
OK.

00:47:06.930 --> 00:47:09.970 align:middle line:90%
So now, how do we prove that?

00:47:09.970 --> 00:47:19.530 align:middle line:84%
So the first thing we
observe is that if we take--

00:47:19.530 --> 00:47:21.810 align:middle line:90%
if we're looking at--

00:47:21.810 --> 00:47:26.370 align:middle line:90%
suppose that fn and f--

00:47:26.370 --> 00:47:26.910 align:middle line:90%
here.

00:47:26.910 --> 00:47:36.410 align:middle line:84%
Suppose that fn
of x minus f of x,

00:47:36.410 --> 00:47:45.050 align:middle line:84%
suppose that this thing
here was less than epsilon

00:47:45.050 --> 00:47:51.570 align:middle line:90%
over 3 b minus a.

00:47:51.570 --> 00:47:54.720 align:middle line:90%
Suppose you have that.

00:47:54.720 --> 00:47:57.230 align:middle line:84%
And of course, this
here can be achieved.

00:47:57.230 --> 00:47:59.740 align:middle line:90%


00:47:59.740 --> 00:48:02.606 align:middle line:90%
So epsilon is now given.

00:48:02.606 --> 00:48:04.540 align:middle line:90%
And so you have that.

00:48:04.540 --> 00:48:07.920 align:middle line:90%
So maybe I should just say that.

00:48:07.920 --> 00:48:11.000 align:middle line:90%
So epsilon is given.

00:48:11.000 --> 00:48:22.400 align:middle line:84%
So since fn converges
to f uniformly,

00:48:22.400 --> 00:48:30.280 align:middle line:84%
this means that there
exists capital N

00:48:30.280 --> 00:48:33.760 align:middle line:84%
so that if you're further
out than capital N, then

00:48:33.760 --> 00:48:37.240 align:middle line:84%
actually you have
this thing here.

00:48:37.240 --> 00:48:38.560 align:middle line:90%
b minus b.

00:48:38.560 --> 00:48:39.820 align:middle line:90%
b and a are fixed.

00:48:39.820 --> 00:48:41.480 align:middle line:90%
This is just something fixed.

00:48:41.480 --> 00:48:43.420 align:middle line:90%
So this is just another epsilon.

00:48:43.420 --> 00:48:45.960 align:middle line:90%


00:48:45.960 --> 00:48:46.580 align:middle line:90%
OK.

00:48:46.580 --> 00:48:51.880 align:middle line:84%
So if you have that,
now suppose you take--

00:48:51.880 --> 00:48:55.120 align:middle line:84%
so remember, we
defined, when we did

00:48:55.120 --> 00:48:59.160 align:middle line:84%
the-- when we had the
partition, the partition had

00:48:59.160 --> 00:49:11.040 align:middle line:84%
the dividing point with
dividing points xi.

00:49:11.040 --> 00:49:14.440 align:middle line:84%
So we were looking at
these small intervals

00:49:14.440 --> 00:49:18.560 align:middle line:90%
from xi minus 1 to xi.

00:49:18.560 --> 00:49:22.750 align:middle line:84%
And we're looking at
the sup of the function.

00:49:22.750 --> 00:49:25.600 align:middle line:90%


00:49:25.600 --> 00:49:28.480 align:middle line:84%
So if you're looking
at the sup of-- suppose

00:49:28.480 --> 00:49:34.000 align:middle line:84%
you're looking at-- so this
here is on this little interval.

00:49:34.000 --> 00:49:34.960 align:middle line:90%
But it's for f.

00:49:34.960 --> 00:49:37.480 align:middle line:90%


00:49:37.480 --> 00:49:40.580 align:middle line:84%
But the function f here,
you see the function.

00:49:40.580 --> 00:49:46.080 align:middle line:84%
So you have that f of x,
this function here-- sorry,

00:49:46.080 --> 00:49:47.740 align:middle line:84%
I don't even need
the absolute value.

00:49:47.740 --> 00:49:58.610 align:middle line:84%
But f of x is less than or equal
to fn of x plus, of course,

00:49:58.610 --> 00:50:02.490 align:middle line:90%
f of x minus fn of x.

00:50:02.490 --> 00:50:07.270 align:middle line:90%


00:50:07.270 --> 00:50:12.630 align:middle line:84%
And so this means that
this thing here is--

00:50:12.630 --> 00:50:18.430 align:middle line:84%
this thing here is less
than or equal to fn of x.

00:50:18.430 --> 00:50:22.290 align:middle line:84%
This thing here is bounded
by the absolute value of it.

00:50:22.290 --> 00:50:30.750 align:middle line:90%


00:50:30.750 --> 00:50:33.590 align:middle line:90%
And so this thing here--

00:50:33.590 --> 00:50:36.190 align:middle line:90%
so this is fn of x.

00:50:36.190 --> 00:50:46.870 align:middle line:84%
And this here is just epsilon
over 3 b minus a, like that.

00:50:46.870 --> 00:50:49.660 align:middle line:90%


00:50:49.660 --> 00:50:54.100 align:middle line:84%
So this means that if I take
the sup on this little interval

00:50:54.100 --> 00:50:59.020 align:middle line:84%
of f, then it's bounded by
the sup of this function

00:50:59.020 --> 00:51:00.540 align:middle line:90%
plus that number.

00:51:00.540 --> 00:51:02.300 align:middle line:90%
So I have that--

00:51:02.300 --> 00:51:21.609 align:middle line:90%


00:51:21.609 --> 00:51:28.000 align:middle line:84%
so I have that, again, the sup
of f on this little interval--

00:51:28.000 --> 00:51:31.340 align:middle line:90%


00:51:31.340 --> 00:51:37.900 align:middle line:90%
this is what we call Mi of f--

00:51:37.900 --> 00:51:40.620 align:middle line:90%
that this is less or equal to--

00:51:40.620 --> 00:51:43.380 align:middle line:84%
because of this
inequality, it's less

00:51:43.380 --> 00:51:52.660 align:middle line:84%
than the sup of fn of x on
the same little interval

00:51:52.660 --> 00:51:56.940 align:middle line:90%
plus epsilon over 3 b minus a.

00:51:56.940 --> 00:51:59.940 align:middle line:90%


00:51:59.940 --> 00:52:11.230 align:middle line:84%
And likewise-- so
likewise for the inf.

00:52:11.230 --> 00:52:14.980 align:middle line:90%


00:52:14.980 --> 00:52:19.500 align:middle line:84%
So again, I let
little mi of f, this

00:52:19.500 --> 00:52:22.990 align:middle line:84%
is now the infimum on
this little interval.

00:52:22.990 --> 00:52:25.780 align:middle line:90%


00:52:25.780 --> 00:52:26.940 align:middle line:90%
Oops.

00:52:26.940 --> 00:52:29.540 align:middle line:90%
On this little interval of f.

00:52:29.540 --> 00:52:34.060 align:middle line:90%


00:52:34.060 --> 00:52:35.340 align:middle line:90%
Sorry.

00:52:35.340 --> 00:52:38.780 align:middle line:84%
Here, I wanted to insert
what this thing was.

00:52:38.780 --> 00:52:43.860 align:middle line:84%
So this was M. The notation
for this sup here is Mifn.

00:52:43.860 --> 00:52:53.850 align:middle line:90%


00:52:53.850 --> 00:52:59.770 align:middle line:84%
And the infimum for f on this
little interval, the notation

00:52:59.770 --> 00:53:04.890 align:middle line:84%
for that is this little m, i
referring to the interval, f

00:53:04.890 --> 00:53:06.810 align:middle line:90%
to the function.

00:53:06.810 --> 00:53:14.750 align:middle line:84%
And so similarly, if
you take the infimum,

00:53:14.750 --> 00:53:19.570 align:middle line:84%
and you compare
it to the infimum

00:53:19.570 --> 00:53:26.570 align:middle line:84%
of this fn on the same
interval, then the same argument

00:53:26.570 --> 00:53:34.650 align:middle line:84%
with obvious changes
means that mif here

00:53:34.650 --> 00:53:47.300 align:middle line:84%
is now bigger or equal to mifn
minus epsilon over 3 b minus a.

00:53:47.300 --> 00:53:52.210 align:middle line:90%


00:53:52.210 --> 00:53:55.480 align:middle line:90%
It's the same--

00:53:55.480 --> 00:53:58.920 align:middle line:84%
OK, maybe I'll just explain it,
but it's the same sort of thing,

00:53:58.920 --> 00:54:01.400 align:middle line:90%
that you take--

00:54:01.400 --> 00:54:04.200 align:middle line:84%
oh, maybe I shouldn't
erase this one.

00:54:04.200 --> 00:54:08.200 align:middle line:84%
So it's sort of the same
thing, that you're looking at--

00:54:08.200 --> 00:54:14.280 align:middle line:84%
you have f of x
again is equal to fn

00:54:14.280 --> 00:54:22.280 align:middle line:90%
of x plus fn plus f of x minus.

00:54:22.280 --> 00:54:26.200 align:middle line:90%
So you have obviously this.

00:54:26.200 --> 00:54:32.720 align:middle line:84%
And so this means
that f of x is bigger

00:54:32.720 --> 00:54:39.760 align:middle line:90%
or equal to fn of x minus.

00:54:39.760 --> 00:54:44.960 align:middle line:84%
If you think that this here
becomes negative and the maximum

00:54:44.960 --> 00:54:48.640 align:middle line:84%
it can become negative on
this little interval here--

00:54:48.640 --> 00:54:56.600 align:middle line:84%
on this little interval, the
worst this here can become

00:54:56.600 --> 00:55:01.360 align:middle line:90%
negative is epsilon over--

00:55:01.360 --> 00:55:06.200 align:middle line:84%
actually, on any
interval, it's this.

00:55:06.200 --> 00:55:07.160 align:middle line:90%
Like that.

00:55:07.160 --> 00:55:10.000 align:middle line:90%
So you always have this.

00:55:10.000 --> 00:55:12.040 align:middle line:90%
OK.

00:55:12.040 --> 00:55:16.680 align:middle line:84%
And so if you take now the
infimum on this little interval,

00:55:16.680 --> 00:55:24.120 align:middle line:84%
then you're getting mif
bigger or equal to mifn minus

00:55:24.120 --> 00:55:29.240 align:middle line:90%
epsilon over 3 b minus a.

00:55:29.240 --> 00:55:30.600 align:middle line:90%
So you have that.

00:55:30.600 --> 00:55:32.240 align:middle line:84%
So that's what we
claim over there.

00:55:32.240 --> 00:55:35.040 align:middle line:90%


00:55:35.040 --> 00:55:37.080 align:middle line:90%
OK.

00:55:37.080 --> 00:55:42.030 align:middle line:84%
So we have this thing here, and
we have the corresponding thing.

00:55:42.030 --> 00:55:45.190 align:middle line:84%
This is less than or equal to
the maximum of the function

00:55:45.190 --> 00:55:47.550 align:middle line:90%
on the same interval.

00:55:47.550 --> 00:55:52.810 align:middle line:84%
And then that's-- and
then this equality here,

00:55:52.810 --> 00:55:59.070 align:middle line:84%
this equality here was that it's
bounded by this guy here plus

00:55:59.070 --> 00:56:04.390 align:middle line:90%
epsilon over 3 b minus a.

00:56:04.390 --> 00:56:09.030 align:middle line:84%
So this is for the little m's,
the little mi's, and the capital

00:56:09.030 --> 00:56:09.790 align:middle line:90%
Mi.

00:56:09.790 --> 00:56:12.030 align:middle line:84%
And now we need
to sum these guys,

00:56:12.030 --> 00:56:17.510 align:middle line:84%
and we need to multiply
those with a delta xi.

00:56:17.510 --> 00:56:20.150 align:middle line:84%
So this means that if
you're looking at-- so

00:56:20.150 --> 00:56:22.910 align:middle line:84%
what we're interested
in is we're

00:56:22.910 --> 00:56:27.870 align:middle line:90%
looking at this times delta xi.

00:56:27.870 --> 00:56:31.710 align:middle line:90%
This gives you the--

00:56:31.710 --> 00:56:37.150 align:middle line:84%
sorry, this gives you the
lower sum of f with respect

00:56:37.150 --> 00:56:41.250 align:middle line:84%
to this partition, where
you're summing here over the i.

00:56:41.250 --> 00:56:43.830 align:middle line:90%


00:56:43.830 --> 00:56:54.470 align:middle line:84%
If you're summing
the sups, then you're

00:56:54.470 --> 00:57:00.150 align:middle line:84%
getting the upper
sum, like that.

00:57:00.150 --> 00:57:07.880 align:middle line:90%
And so now-- so you take--

00:57:07.880 --> 00:57:15.110 align:middle line:90%


00:57:15.110 --> 00:57:20.430 align:middle line:84%
you take this inequality,
this string of inequality,

00:57:20.430 --> 00:57:30.150 align:middle line:84%
and you're just multiplying
by delta xi on both sides.

00:57:30.150 --> 00:57:31.810 align:middle line:90%
And then I'm summing.

00:57:31.810 --> 00:57:33.630 align:middle line:90%
So if I multiply--

00:57:33.630 --> 00:57:36.070 align:middle line:90%
so let's call this here star.

00:57:36.070 --> 00:57:53.840 align:middle line:84%
So multiply star by
delta xi and sum over i.

00:57:53.840 --> 00:57:56.820 align:middle line:84%
If you do that, then
what you get is you're

00:57:56.820 --> 00:58:15.820 align:middle line:84%
getting mifn minus epsilon
over 3 b minus a times this,

00:58:15.820 --> 00:58:18.180 align:middle line:90%
times delta xi.

00:58:18.180 --> 00:58:26.440 align:middle line:84%
This is less than or equal to
mif delta xi, which is less than

00:58:26.440 --> 00:58:28.480 align:middle line:90%
or equal to this one here.

00:58:28.480 --> 00:58:31.460 align:middle line:90%


00:58:31.460 --> 00:58:31.980 align:middle line:90%
Sorry.

00:58:31.980 --> 00:58:34.380 align:middle line:90%
And I should also sum.

00:58:34.380 --> 00:58:40.490 align:middle line:90%
Summing over i, like this.

00:58:40.490 --> 00:58:43.850 align:middle line:84%
And then I have one
more inequality, namely

00:58:43.850 --> 00:58:46.370 align:middle line:90%
this right-hand side.

00:58:46.370 --> 00:58:49.210 align:middle line:90%
So less than or equal to.

00:58:49.210 --> 00:58:50.670 align:middle line:90%
I'm summing over i.

00:58:50.670 --> 00:58:53.890 align:middle line:90%


00:58:53.890 --> 00:59:06.050 align:middle line:84%
And I have-- this is mif plus
epsilon over 3 b minus a times

00:59:06.050 --> 00:59:07.890 align:middle line:90%
delta xi.

00:59:07.890 --> 00:59:12.050 align:middle line:90%


00:59:12.050 --> 00:59:13.690 align:middle line:90%
So we have that.

00:59:13.690 --> 00:59:16.020 align:middle line:84%
Now let's try to figure
out what this means.

00:59:16.020 --> 00:59:22.490 align:middle line:90%


00:59:22.490 --> 00:59:27.250 align:middle line:84%
So this here-- so
now, if you multiply

00:59:27.250 --> 00:59:34.730 align:middle line:84%
this out, the first thing,
the top left corner,

00:59:34.730 --> 00:59:39.210 align:middle line:84%
that gives you-- when you
multiply the bracket out,

00:59:39.210 --> 00:59:46.370 align:middle line:84%
the first term you get is
the mifn times delta xi.

00:59:46.370 --> 00:59:50.650 align:middle line:84%
But that is just the
lower sum with respect

00:59:50.650 --> 00:59:53.730 align:middle line:90%
to the partition P for fn.

00:59:53.730 --> 00:59:56.610 align:middle line:90%


00:59:56.610 --> 01:00:01.230 align:middle line:84%
But then you get another term,
which is you get one other term.

01:00:01.230 --> 01:00:03.530 align:middle line:90%
You get this minus.

01:00:03.530 --> 01:00:08.030 align:middle line:84%
And then you're summing
over the i of epsilon 3

01:00:08.030 --> 01:00:10.920 align:middle line:90%
b minus a times xi.

01:00:10.920 --> 01:00:16.890 align:middle line:90%


01:00:16.890 --> 01:00:27.810 align:middle line:84%
And then it's less than or
equal to the term up there.

01:00:27.810 --> 01:00:34.000 align:middle line:84%
That's just the lower sum of f
with respect to the partition.

01:00:34.000 --> 01:00:38.080 align:middle line:84%
THE next term is
the upper sum of f

01:00:38.080 --> 01:00:40.520 align:middle line:90%
with respect to the partition.

01:00:40.520 --> 01:00:44.100 align:middle line:84%
And then the last
inequality, the first term--

01:00:44.100 --> 01:00:48.420 align:middle line:84%
when you multiply this bracket
out, the first term here is--

01:00:48.420 --> 01:00:52.440 align:middle line:84%
and unfortunately,
there was a missing n.

01:00:52.440 --> 01:00:54.140 align:middle line:90%
I copied it from here.

01:00:54.140 --> 01:00:56.800 align:middle line:90%
Sorry.

01:00:56.800 --> 01:00:57.840 align:middle line:90%
There was a missing n.

01:00:57.840 --> 01:00:59.340 align:middle line:90%
I just copied it from this one.

01:00:59.340 --> 01:01:07.760 align:middle line:90%


01:01:07.760 --> 01:01:12.120 align:middle line:84%
So now when you multiply
this bracket out,

01:01:12.120 --> 01:01:16.800 align:middle line:90%
the first term you get here is--

01:01:16.800 --> 01:01:19.220 align:middle line:84%
so you're getting less than
or equal to the first term

01:01:19.220 --> 01:01:22.000 align:middle line:84%
you get there when you're
summing over the i.

01:01:22.000 --> 01:01:28.240 align:middle line:90%
That's exactly u fn, p.

01:01:28.240 --> 01:01:35.590 align:middle line:84%
And then the second term you
get is this i epsilon over 3 b

01:01:35.590 --> 01:01:37.670 align:middle line:90%
minus a delta xi.

01:01:37.670 --> 01:01:40.430 align:middle line:90%


01:01:40.430 --> 01:01:48.070 align:middle line:84%
Now, this thing here,
when I'm summing here,

01:01:48.070 --> 01:01:51.330 align:middle line:90%
then this is just a constant.

01:01:51.330 --> 01:01:53.590 align:middle line:84%
So I can just pull
that constant out.

01:01:53.590 --> 01:01:55.550 align:middle line:84%
And the sum of
these differences,

01:01:55.550 --> 01:01:58.270 align:middle line:90%
that just gives you b minus a.

01:01:58.270 --> 01:02:02.830 align:middle line:84%
So if you put that in
and it's exactly the same

01:02:02.830 --> 01:02:05.510 align:middle line:84%
you get on this
term, then you have

01:02:05.510 --> 01:02:11.830 align:middle line:84%
that L fn, P minus
epsilon over 3

01:02:11.830 --> 01:02:22.070 align:middle line:84%
is less than or equal to
L f, P, which is less than

01:02:22.070 --> 01:02:28.950 align:middle line:84%
or equal to u f, P. And
this is less than or equal

01:02:28.950 --> 01:02:38.090 align:middle line:90%
to u fn, P plus epsilon over 3.

01:02:38.090 --> 01:02:41.270 align:middle line:90%


01:02:41.270 --> 01:02:42.070 align:middle line:90%
OK.

01:02:42.070 --> 01:02:44.350 align:middle line:90%
Now what have we used so far?

01:02:44.350 --> 01:02:47.470 align:middle line:90%
So far, we have just used--

01:02:47.470 --> 01:02:49.630 align:middle line:90%
P was any partition.

01:02:49.630 --> 01:02:56.430 align:middle line:84%
And all we have used is that
the fn converges to f uniformly.

01:02:56.430 --> 01:02:59.070 align:middle line:84%
And then, for this
given epsilon,

01:02:59.070 --> 01:03:02.190 align:middle line:84%
we chose this capital
N sufficiently large.

01:03:02.190 --> 01:03:05.510 align:middle line:90%


01:03:05.510 --> 01:03:10.910 align:middle line:90%
But now, now you see that--

01:03:10.910 --> 01:03:12.850 align:middle line:90%
now we can just fix--

01:03:12.850 --> 01:03:17.510 align:middle line:90%
so now we just let little n--

01:03:17.510 --> 01:03:21.110 align:middle line:84%
we just said, let this be
equal to this capital N. We

01:03:21.110 --> 01:03:25.890 align:middle line:84%
just need to use it
for one little n.

01:03:25.890 --> 01:03:29.528 align:middle line:90%


01:03:29.528 --> 01:03:31.660 align:middle line:90%
And then we can--

01:03:31.660 --> 01:03:38.060 align:middle line:84%
and now we have that since this
particular function, this one

01:03:38.060 --> 01:03:49.980 align:middle line:84%
function, was integrable,
then there exists a partition.

01:03:49.980 --> 01:03:53.860 align:middle line:84%
But this is now a
partition that comes from,

01:03:53.860 --> 01:03:56.780 align:middle line:84%
that is determined from
this function here.

01:03:56.780 --> 01:04:04.100 align:middle line:84%
But there exists a
partition so that the L--

01:04:04.100 --> 01:04:14.380 align:middle line:84%
sorry, so that the difference
between the upper sum

01:04:14.380 --> 01:04:20.500 align:middle line:84%
for this function minus the
lower sum for this function

01:04:20.500 --> 01:04:25.500 align:middle line:84%
is less than, say,
epsilon over 3.

01:04:25.500 --> 01:04:30.730 align:middle line:90%


01:04:30.730 --> 01:04:35.260 align:middle line:84%
So you see that
this number here--

01:04:35.260 --> 01:04:38.210 align:middle line:90%


01:04:38.210 --> 01:04:43.250 align:middle line:90%
so you see that the difference--

01:04:43.250 --> 01:04:44.910 align:middle line:90%
now I can erase this thing here.

01:04:44.910 --> 01:04:48.210 align:middle line:90%


01:04:48.210 --> 01:04:53.690 align:middle line:90%
So now the first--

01:04:53.690 --> 01:05:05.714 align:middle line:84%
so we observe now that this
number here, because of this,

01:05:05.714 --> 01:05:09.056 align:middle line:84%
this number is always
larger than that.

01:05:09.056 --> 01:05:15.750 align:middle line:84%
And so this means that this
thing here, by this inequality,

01:05:15.750 --> 01:05:19.130 align:middle line:84%
it just tells you that
this is less than--

01:05:19.130 --> 01:05:23.050 align:middle line:84%
that this thing here-- let
me continue here below--

01:05:23.050 --> 01:05:32.010 align:middle line:84%
that this thing here is less
than L fn, P plus epsilon

01:05:32.010 --> 01:05:33.250 align:middle line:90%
over 3.

01:05:33.250 --> 01:05:35.870 align:middle line:84%
This is coming from
that this one here--

01:05:35.870 --> 01:05:38.070 align:middle line:84%
just moving this over
on the other side.

01:05:38.070 --> 01:05:40.530 align:middle line:84%
Then you have that this
is bounded by that.

01:05:40.530 --> 01:05:42.990 align:middle line:84%
And then you have
another epsilon over 3.

01:05:42.990 --> 01:05:46.402 align:middle line:90%


01:05:46.402 --> 01:05:49.930 align:middle line:84%
And so you see that
those two things--

01:05:49.930 --> 01:05:52.010 align:middle line:90%
this here and that here--

01:05:52.010 --> 01:05:56.890 align:middle line:84%
is squeezed in an interval
of length epsilon.

01:05:56.890 --> 01:06:00.690 align:middle line:84%
So this means that the
difference between these two

01:06:00.690 --> 01:06:03.650 align:middle line:90%
is bounded by epsilon.

01:06:03.650 --> 01:06:12.148 align:middle line:84%
So L f with respect to
this partition and u f,

01:06:12.148 --> 01:06:29.220 align:middle line:84%
P, they both lie in an
interval of length epsilon.

01:06:29.220 --> 01:06:31.520 align:middle line:84%
So it means that the
difference between the two.

01:06:31.520 --> 01:06:33.420 align:middle line:90%
So the difference between.

01:06:33.420 --> 01:06:37.240 align:middle line:84%
So this here, which
is always positive.

01:06:37.240 --> 01:06:41.280 align:middle line:84%
But this here, the
difference must be,

01:06:41.280 --> 01:06:42.620 align:middle line:90%
I guess, less than or equal to.

01:06:42.620 --> 01:06:43.420 align:middle line:90%
It doesn't matter.

01:06:43.420 --> 01:06:48.320 align:middle line:90%


01:06:48.320 --> 01:07:01.440 align:middle line:84%
And this proves-- so this show
that f here is integrable.

01:07:01.440 --> 01:07:02.340 align:middle line:90%
It's integrable.

01:07:02.340 --> 01:07:08.440 align:middle line:90%


01:07:08.440 --> 01:07:11.080 align:middle line:84%
Because to show that this
function was integrable,

01:07:11.080 --> 01:07:12.320 align:middle line:90%
we just needed to--

01:07:12.320 --> 01:07:15.280 align:middle line:84%
for a given epsilon, we
needed to find a partition

01:07:15.280 --> 01:07:19.000 align:middle line:84%
so that the difference between
the upper and the lower sum

01:07:19.000 --> 01:07:22.120 align:middle line:84%
was less than or
equal to epsilon.

01:07:22.120 --> 01:07:28.590 align:middle line:90%
So the function f is integrable.

01:07:28.590 --> 01:07:33.950 align:middle line:84%
Now, I claim that it
also proves that--

01:07:33.950 --> 01:07:41.890 align:middle line:84%
it also shows that the
limit is what it should be.

01:07:41.890 --> 01:07:51.910 align:middle line:90%


01:07:51.910 --> 01:07:58.350 align:middle line:84%
Because you see that we now
know that the function--

01:07:58.350 --> 01:08:15.145 align:middle line:84%
so we have now that this
integral of f dx, this exists,

01:08:15.145 --> 01:08:16.770 align:middle line:84%
because we proved
that it's integrable.

01:08:16.770 --> 01:08:18.590 align:middle line:90%
So it means that this exists.

01:08:18.590 --> 01:08:23.510 align:middle line:84%
And this is always
squeezed between--

01:08:23.510 --> 01:08:25.550 align:middle line:84%
for any partition,
it's always squeezed

01:08:25.550 --> 01:08:26.620 align:middle line:90%
between these two things.

01:08:26.620 --> 01:08:31.990 align:middle line:90%


01:08:31.990 --> 01:08:33.970 align:middle line:90%
But now you see that--

01:08:33.970 --> 01:08:40.430 align:middle line:84%
so this means that it
would have to lie--

01:08:40.430 --> 01:08:43.990 align:middle line:84%
in this string of
inequality, it would

01:08:43.990 --> 01:08:47.630 align:middle line:84%
have to lie here, between
these two numbers.

01:08:47.630 --> 01:08:55.729 align:middle line:84%
But this thing here,
if you make this--

01:08:55.729 --> 01:08:58.390 align:middle line:90%
so we have also--

01:08:58.390 --> 01:09:01.670 align:middle line:90%
so what do we have?

01:09:01.670 --> 01:09:14.390 align:middle line:84%
We have that-- so we have
that this integral here,

01:09:14.390 --> 01:09:18.410 align:middle line:84%
from a to b of f
dx, is less than

01:09:18.410 --> 01:09:25.140 align:middle line:84%
or equal to u f with
respect to any partition.

01:09:25.140 --> 01:09:27.300 align:middle line:90%
The same thing here.

01:09:27.300 --> 01:09:33.140 align:middle line:90%
And now, if we let--

01:09:33.140 --> 01:09:36.740 align:middle line:84%
if we looked at--
if we use this--

01:09:36.740 --> 01:09:40.700 align:middle line:84%
if we use, for
this given epsilon,

01:09:40.700 --> 01:09:45.750 align:middle line:84%
that n here is bigger than
capital N, bigger or equal to,

01:09:45.750 --> 01:09:49.060 align:middle line:84%
then we have that
this thing here was

01:09:49.060 --> 01:09:52.540 align:middle line:84%
bounded below from
this inequality

01:09:52.540 --> 01:10:00.780 align:middle line:90%
L fn, P minus epsilon over 3.

01:10:00.780 --> 01:10:04.220 align:middle line:84%
And we had that it was
bounded from above.

01:10:04.220 --> 01:10:11.380 align:middle line:84%
So this is just this inequality
u fn, P plus epsilon over 3.

01:10:11.380 --> 01:10:18.620 align:middle line:84%
And so now we made use of-- and
so we do for this capital N.

01:10:18.620 --> 01:10:23.330 align:middle line:84%
So in particular, it
holds for capital N.

01:10:23.330 --> 01:10:27.250 align:middle line:90%
And now we made use of that.

01:10:27.250 --> 01:10:29.330 align:middle line:84%
So now all I want
to do is here I

01:10:29.330 --> 01:10:36.130 align:middle line:84%
want to estimate the difference
between this integral here

01:10:36.130 --> 01:10:38.730 align:middle line:90%
and this integral here.

01:10:38.730 --> 01:10:48.210 align:middle line:84%
And the integral from a
to b of f capital N. And I

01:10:48.210 --> 01:10:51.530 align:middle line:84%
want to prove that
if I'm very far out,

01:10:51.530 --> 01:10:54.730 align:middle line:90%
that this here is very small.

01:10:54.730 --> 01:10:57.110 align:middle line:90%
But I now make this one here--

01:10:57.110 --> 01:10:59.370 align:middle line:90%
so if I take m--

01:10:59.370 --> 01:11:03.770 align:middle line:84%
when I choose my partition
so that this number here--

01:11:03.770 --> 01:11:06.610 align:middle line:84%
so then I can just make
sure that this number

01:11:06.610 --> 01:11:12.450 align:middle line:84%
here, when I choose
the partition,

01:11:12.450 --> 01:11:15.650 align:middle line:84%
then I just said that I
choose the partition so

01:11:15.650 --> 01:11:23.450 align:middle line:84%
that this thing here minus this
lower here for this capital N,

01:11:23.450 --> 01:11:27.050 align:middle line:84%
that this here was smaller
than epsilon over 3.

01:11:27.050 --> 01:11:29.690 align:middle line:90%
And so this means again--

01:11:29.690 --> 01:11:35.210 align:middle line:84%
but now you see
that this integral

01:11:35.210 --> 01:11:39.330 align:middle line:84%
of this integral here,
this is always squeezed

01:11:39.330 --> 01:11:40.750 align:middle line:90%
between these two numbers.

01:11:40.750 --> 01:11:47.740 align:middle line:84%
So this is always
squeezed like this.

01:11:47.740 --> 01:11:56.640 align:middle line:90%


01:11:56.640 --> 01:12:04.850 align:middle line:84%
And so now you see that this
means that this integral is

01:12:04.850 --> 01:12:08.530 align:middle line:90%
in this interval here.

01:12:08.530 --> 01:12:16.930 align:middle line:84%
But in fact, of course, in
this interval between these two

01:12:16.930 --> 01:12:17.430 align:middle line:90%
numbers--

01:12:17.430 --> 01:12:20.960 align:middle line:90%


01:12:20.960 --> 01:12:24.080 align:middle line:90%
between these two numbers--

01:12:24.080 --> 01:12:27.880 align:middle line:84%
even if there wasn't a
plus in that interval,

01:12:27.880 --> 01:12:31.520 align:middle line:84%
that this integral
here would also lie.

01:12:31.520 --> 01:12:37.040 align:middle line:84%
So it lies even more comfortable
in this larger interval,

01:12:37.040 --> 01:12:39.240 align:middle line:84%
where you're adding
epsilon over 3

01:12:39.240 --> 01:12:41.880 align:middle line:90%
and subtracting epsilon over 3.

01:12:41.880 --> 01:12:46.560 align:middle line:84%
So this integral lie
between these two.

01:12:46.560 --> 01:12:49.350 align:middle line:90%
The same is the case for this.

01:12:49.350 --> 01:12:53.720 align:middle line:90%


01:12:53.720 --> 01:12:56.960 align:middle line:84%
And this interval, I
can have length epsilon.

01:12:56.960 --> 01:12:59.280 align:middle line:84%
So this means that this
difference between these two

01:12:59.280 --> 01:13:01.790 align:middle line:84%
numbers is also
less than epsilon.

01:13:01.790 --> 01:13:09.720 align:middle line:90%


01:13:09.720 --> 01:13:14.080 align:middle line:84%
And so this really proves that
if it was sufficiently far out,

01:13:14.080 --> 01:13:16.920 align:middle line:84%
then the difference
between these two integrals

01:13:16.920 --> 01:13:18.800 align:middle line:90%
was bounded by epsilon.

01:13:18.800 --> 01:13:22.800 align:middle line:84%
So this proves that the
integrals are converging.

01:13:22.800 --> 01:13:25.300 align:middle line:90%
OK?

01:13:25.300 --> 01:13:28.080 align:middle line:84%
Let's look at-- so
how do we use this?

01:13:28.080 --> 01:13:34.940 align:middle line:84%
So what we were interested
in was using this fact

01:13:34.940 --> 01:13:36.980 align:middle line:90%
in the case of a power series.

01:13:36.980 --> 01:13:41.660 align:middle line:84%
So let me just look at
an example for that.

01:13:41.660 --> 01:13:47.200 align:middle line:90%


01:13:47.200 --> 01:13:50.360 align:middle line:90%
So suppose that En of x--

01:13:50.360 --> 01:13:54.280 align:middle line:84%
so this is the same as
in the previous example,

01:13:54.280 --> 01:14:00.280 align:middle line:84%
where I'm summing here from
k equal to 0 to n xn over--

01:14:00.280 --> 01:14:03.820 align:middle line:90%
xk, sorry, over k factorial.

01:14:03.820 --> 01:14:08.440 align:middle line:84%
So these are the
functions xn and x--

01:14:08.440 --> 01:14:10.480 align:middle line:90%
sorry, En.

01:14:10.480 --> 01:14:14.230 align:middle line:84%
And the function-- so
this was the function En.

01:14:14.230 --> 01:14:18.110 align:middle line:84%
The function E is just
the exponential function,

01:14:18.110 --> 01:14:24.950 align:middle line:84%
which I think about as the
infinite series, power series,

01:14:24.950 --> 01:14:27.950 align:middle line:90%
like this.

01:14:27.950 --> 01:14:29.530 align:middle line:90%
And now I had--

01:14:29.530 --> 01:14:34.590 align:middle line:84%
so we already observed
that by the Weierstrass.

01:14:34.590 --> 01:14:41.390 align:middle line:90%
So by Weierstrass M-test.

01:14:41.390 --> 01:14:45.150 align:middle line:90%


01:14:45.150 --> 01:14:53.240 align:middle line:84%
By Weierstrass M-test, the En
converges to E on any interval.

01:14:53.240 --> 01:14:56.070 align:middle line:90%


01:14:56.070 --> 01:14:58.110 align:middle line:84%
You have to restrict
the interval.

01:14:58.110 --> 01:15:00.710 align:middle line:84%
But if you're fixing
an interval like this,

01:15:00.710 --> 01:15:05.030 align:middle line:90%
then it's converging uniformly.

01:15:05.030 --> 01:15:07.810 align:middle line:84%
So this is what
Weierstrass M-test gave.

01:15:07.810 --> 01:15:11.174 align:middle line:90%


01:15:11.174 --> 01:15:16.760 align:middle line:84%
And now these functions
here, they are polynomials.

01:15:16.760 --> 01:15:18.120 align:middle line:90%
The En are polynomials.

01:15:18.120 --> 01:15:20.260 align:middle line:90%
So it's easy to integrate them.

01:15:20.260 --> 01:15:29.260 align:middle line:84%
So you have that the
integral here of En dx from,

01:15:29.260 --> 01:15:32.620 align:middle line:84%
let's say, some interval
from a to b, this thing

01:15:32.620 --> 01:15:38.280 align:middle line:84%
here is now equal
to the sum here.

01:15:38.280 --> 01:15:41.580 align:middle line:84%
So now it's just a finite
sum, so you can exchange that.

01:15:41.580 --> 01:15:48.120 align:middle line:84%
And then you're integrating from
a to b of xk over k factorial.

01:15:48.120 --> 01:15:52.380 align:middle line:90%


01:15:52.380 --> 01:15:56.900 align:middle line:84%
And of course, that's
very easy to do.

01:15:56.900 --> 01:15:59.620 align:middle line:90%
So dx.

01:15:59.620 --> 01:16:04.700 align:middle line:84%
And the theorem that we just
proved is that this thing

01:16:04.700 --> 01:16:09.780 align:middle line:84%
here, because the convergence
is uniform, each of these

01:16:09.780 --> 01:16:11.020 align:middle line:90%
is integrable.

01:16:11.020 --> 01:16:16.260 align:middle line:84%
This means that the limit
here is also integrable,

01:16:16.260 --> 01:16:22.900 align:middle line:84%
and the integral of the
exponential function

01:16:22.900 --> 01:16:25.900 align:middle line:90%
is the limit of these integrals.

01:16:25.900 --> 01:16:31.860 align:middle line:84%
And so the point here,
again, is that if you

01:16:31.860 --> 01:16:35.340 align:middle line:84%
have uniform convergence,
then you can--

01:16:35.340 --> 01:16:38.100 align:middle line:84%
I mean, you're using
the uniform convergence

01:16:38.100 --> 01:16:40.900 align:middle line:84%
that we have from
Weierstrass M-test.

01:16:40.900 --> 01:16:45.500 align:middle line:84%
Then we can interchange
this infinite sum

01:16:45.500 --> 01:16:47.920 align:middle line:90%
with taking integrals.

01:16:47.920 --> 01:16:48.420 align:middle line:90%
OK?

01:16:48.420 --> 01:16:51.420 align:middle line:90%


01:16:51.420 --> 01:16:53.500 align:middle line:90%
OK.

01:16:53.500 --> 01:16:55.040 align:middle line:90%
Let me just--

01:16:55.040 --> 01:16:56.880 align:middle line:84%
I had wanted to
do one more thing,

01:16:56.880 --> 01:17:02.220 align:middle line:84%
but I don't have time
to do that quite.

01:17:02.220 --> 01:17:04.320 align:middle line:84%
So I'll pick up
on that next time.

01:17:04.320 --> 01:17:09.240 align:middle line:84%
But let me just observe that
when you're integrating here,

01:17:09.240 --> 01:17:12.730 align:middle line:84%
when you're integrating
this thing here,

01:17:12.730 --> 01:17:14.590 align:middle line:90%
what is the integral of this?

01:17:14.590 --> 01:17:17.050 align:middle line:84%
So when we just
calculating this.

01:17:17.050 --> 01:17:22.410 align:middle line:84%
So you're integrating x
to the k over k factorial.

01:17:22.410 --> 01:17:26.730 align:middle line:84%
When you're integrating a
polynomial, you're looking for--

01:17:26.730 --> 01:17:29.570 align:middle line:84%
you're using the fundamental
theorem of calculus.

01:17:29.570 --> 01:17:32.970 align:middle line:84%
So you're trying to look for
a function whose derivative is

01:17:32.970 --> 01:17:34.090 align:middle line:90%
this.

01:17:34.090 --> 01:17:37.850 align:middle line:84%
Such a function is often
called the antiderivative.

01:17:37.850 --> 01:17:40.170 align:middle line:90%
And so what is that function?

01:17:40.170 --> 01:17:43.610 align:middle line:84%
So a function-- so
if you're looking

01:17:43.610 --> 01:17:48.698 align:middle line:84%
at x to the power
k plus 1, you know

01:17:48.698 --> 01:17:50.490 align:middle line:84%
that you have to--
because it's polynomial,

01:17:50.490 --> 01:17:55.850 align:middle line:84%
you have to add 1
to the exponent.

01:17:55.850 --> 01:18:00.530 align:middle line:84%
And then, when you take
derivatives, this comes down.

01:18:00.530 --> 01:18:06.270 align:middle line:84%
So you have to look
at k plus 1 factorial.

01:18:06.270 --> 01:18:10.240 align:middle line:84%
Because when you take the
derivative, then k plus 1

01:18:10.240 --> 01:18:10.760 align:middle line:90%
comes down.

01:18:10.760 --> 01:18:15.600 align:middle line:84%
And it kills the first
one, and the rest is this.

01:18:15.600 --> 01:18:19.240 align:middle line:84%
And so when you
evaluate this integral,

01:18:19.240 --> 01:18:22.920 align:middle line:84%
then this here is
the antiderivative.

01:18:22.920 --> 01:18:30.460 align:middle line:84%
And you have to insert the
boundary values like this.

01:18:30.460 --> 01:18:31.880 align:middle line:90%
So that would be the integral.

01:18:31.880 --> 01:18:34.440 align:middle line:90%


01:18:34.440 --> 01:18:36.960 align:middle line:90%
So I'll just stop here.

01:18:36.960 --> 01:18:41.960 align:middle line:84%
And next time, I'll go through
the one theorem I didn't get to,

01:18:41.960 --> 01:18:45.940 align:middle line:84%
which is how to interchange
the differentiation.

01:18:45.940 --> 01:18:48.480 align:middle line:90%


01:18:48.480 --> 01:18:51.840 align:middle line:84%
Well, if you take a
sequence of functions

01:18:51.840 --> 01:18:53.960 align:middle line:84%
that converge
uniformly and you want

01:18:53.960 --> 01:18:57.840 align:middle line:84%
to take the derivative
of these, how

01:18:57.840 --> 01:19:00.960 align:middle line:84%
do you relate the
derivative of the sequence

01:19:00.960 --> 01:19:03.672 align:middle line:90%
to the derivative of the limit?

01:19:03.672 --> 01:19:05.000 align:middle line:90%
But it's in the notes.

01:19:05.000 --> 01:19:09.320 align:middle line:84%
I already posted the notes, but
I'll go through that next time.

01:19:09.320 --> 01:19:11.620 align:middle line:90%
Any questions?

01:19:11.620 --> 01:19:12.120 align:middle line:90%
Yeah?

01:19:12.120 --> 01:19:16.925 align:middle line:84%
AUDIENCE: I had a question
about the upper-number sums.

01:19:16.925 --> 01:19:17.800 align:middle line:90%
TOBIAS COLDING: Yeah.

01:19:17.800 --> 01:19:19.230 align:middle line:90%
AUDIENCE: I think there was a--

01:19:19.230 --> 01:19:21.040 align:middle line:84%
[INAUDIBLE] I've seen
lot of difference

01:19:21.040 --> 01:19:23.460 align:middle line:84%
between epsilon and numbers
less than or equal to.

01:19:23.460 --> 01:19:23.880 align:middle line:90%
TOBIAS COLDING: Yeah.

01:19:23.880 --> 01:19:24.520 align:middle line:90%
AUDIENCE: Is that OK?

01:19:24.520 --> 01:19:25.978 align:middle line:84%
TOBIAS COLDING:
That's OK because--

01:19:25.978 --> 01:19:30.760 align:middle line:90%


01:19:30.760 --> 01:19:34.460 align:middle line:84%
I'm not 100% sure I
needed epsilon less than

01:19:34.460 --> 01:19:35.640 align:middle line:90%
or equal to epsilon.

01:19:35.640 --> 01:19:38.400 align:middle line:84%
It doesn't really matter
because you just pick that.

01:19:38.400 --> 01:19:46.440 align:middle line:84%
I had chosen it with the epsilon
over 3 and epsilon over 3 times

01:19:46.440 --> 01:19:47.800 align:middle line:90%
b minus a.

01:19:47.800 --> 01:19:50.100 align:middle line:84%
That was just to
have it worked out

01:19:50.100 --> 01:19:51.700 align:middle line:90%
so it was epsilon in the end.

01:19:51.700 --> 01:19:54.280 align:middle line:84%
But you could, of course,
have chosen it even smaller.

01:19:54.280 --> 01:19:56.840 align:middle line:84%
Then you would have
had strict inequality.

01:19:56.840 --> 01:19:59.880 align:middle line:84%
It's possible it was
actually strict inequality.

01:19:59.880 --> 01:20:00.800 align:middle line:90%
Anyway.

01:20:00.800 --> 01:20:02.050 align:middle line:90%
OK

01:20:02.050 --> 01:20:07.000 align:middle line:90%