WEBVTT

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Every field that measures anything
keeps meeting the same curve.

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Biologists find it in heights, physicists
in noise, pollsters in polls: a symmetric

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bell, over and over, in data that has no
business agreeing about anything.

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Today we find out

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where that bell comes from, and the
answer is one theorem about averages.

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So let me build a world
with no bell in it anywhere.

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Here is a population:

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the number of sales
a small shop makes in a day.

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Most days are quiet, and one
sale is the commonest day of all,

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at thirty-two percent.

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Two sales happen on twenty-two
percent of days, and three on sixteen.

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Then the tail begins:

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four, five, six,

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and every so often
a wild day of seven sales.

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Two numbers will follow us all lecture.

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The mean, mu, is two point eight,
the balance point of the whole shape.

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And the standard deviation, sigma,

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is one point eight, the typical distance
a single day lands from that mean.

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And look at the shape itself.

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It is lopsided:

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the tail runs off to the right,
and a seven sits far from everything else.

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Nothing about this picture is symmetric,
and nothing about it is a bell.

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Now the destination.

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This curve on the right is the normal
curve: the bell that every one

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of those fields keeps finding, symmetric
about its middle and thin in both tails.

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Keep the two pictures side by side,

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because together they
are the whole lecture.

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The claim is that the lopsided shop
on the left will manufacture the bell

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on the right, and the machine
that does it is averaging.

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Take four days at random,
average them, and keep the average.

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Do it again and again,
and watch what the averages do.

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Here is the machine we ended on, and
its one rule: draw four days at random,

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average them, and keep
nothing but the average.

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On the left, the population we draw from.

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On the right, an empty frame
where the averages will live.

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First sample.

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The shop hands us a two,

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a one, a five, and a three, and there
they are, sitting on the population.

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Now the arithmetic, in full.

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Two plus one plus five
plus three is eleven,

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and eleven over four
is two point seven five.

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That is the sample mean, written x
bar, and it is the only thing we keep.

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Over it goes.

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The tick marks two point
seven five on the new axis,

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and then the whole sample becomes one gray
brick, standing in the bin it landed in.

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The four days that made it are gone.

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Again.

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A one, a four, and a pair of twos:

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the sum is nine, nine
over four is two point two five,

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and a second brick lands just
to the left of the first.

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Once more: a six,
a one, a three, and a two.

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Twelve over four is three
exactly, and a third brick lands.

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Now a lucky draw.

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A seven comes up,
with a one, a one, and a two.

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Add them: eleven again, so the average
is two point seven five, again.

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Even a wild day,

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averaged with three quiet ones, gets
dragged back to the middle of the pile.

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From here, let it run.

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Sample, average, brick.

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Sample, average, brick.

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Five more spins
of that loop, five more bricks,

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and already the pile stands tallest
in the middle and thin at both ends.

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Nine averages hint
at a shape without showing it.

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To see it properly we need not nine
but dozens, so let the machine take

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over and run while we watch.

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Sixty-four averages now:

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the machine kept sampling while we
talked, and every average left its brick.

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Look at the wall they built.

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It stands tallest just short of three,
and it falls away on both sides.

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Set the wall against where it came from.

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The population leans left
and drags its tail out to seven.

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The averages have no tail worth
the name: past four and a half,

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the bins are simply empty.

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Averaging erased the skew,
and the question is how.

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So watch a lucky sample
try to build a tail.

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A seven comes up, and with it
a one, a two, and a three.

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Their average: thirteen over four,
which is three and a quarter.

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The seven hauled it to the right, and
the quiet days hauled it straight back.

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Averaging is a tug
of war, and the middle wins.

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An average out at seven would need
all four draws to be sevens at once,

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and each has probability
zero point zero five.

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Multiply the four together:
about six chances in a million.

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That is why the wall
is dead long before seven.

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Now bring back the curve from the opening
minute and lay it over the wall.

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This is the normal curve,
and it hugs the bricks.

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A lopsided population, pushed
through nothing but averaging,

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has manufactured the bell.

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What we built deserves its name.

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The sample mean is itself random:

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a different sample
gives a different average.

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Its distribution, across every sample
you could possibly draw, is called

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the sampling distribution of the mean,
and our histogram is a portrait of it.

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And measure the portrait.

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Its centre sits at two point eight,
the population mean, exactly.

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Its width is zero point nine, and zero
point nine is one point eight divided

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by two: sigma, divided
by the square root of four.

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The sample size has crept into the width,
and that is the theorem knocking.

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Here it is then, in full:

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the Central Limit Theorem.

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Draw samples of size n
from any population at all,

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provided it has a mean mu
and a finite standard deviation sigma.

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As n grows, the distribution of the sample
mean approaches the normal curve, centred

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on mu, with width sigma
over the square root of n.

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That one line is the quantitative heart.

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The width of the bell
of averages is sigma over root n.

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The population's shape is not
in it, and the skew is not in it.

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Only mu, sigma, and n
survive the averaging.

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Let us watch that square
root earn its keep.

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Here is the bell for n equals four,

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centred on the dashed
line at two point eight.

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The bracket underneath is one width of it:

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sigma of x bar,
the quantity our formula computes.

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The computation sits beside it.

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Sigma is one point eight,
the spread we measured back at the start.

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Root four is two.

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And one point eight
over two is zero point nine.

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Now buy more data. Quadruple the sample
to sixteen: root sixteen is four,

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and the width drops to one point
eight over four, zero point four five.

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Watch the bracket shrink
to match the new bell.

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Mark the price of that.

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Four times the data bought exactly
half the width, not a quarter of it.

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The square root is the reason,
and it never relents.

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Quadruple again, to sixty-four.

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Root sixty-four is eight,
and the width is zero point two two five:

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the bell has sharpened into a spike.

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It grows taller as it
narrows because the area

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under every one of these curves is one, so
the probability has nowhere to go but up.

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So this is what averaging
buys, and what it costs.

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It forgets the population's shape
entirely, and it shrinks the noise

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by exactly root n.

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What remains is the fine print, because
a theorem this strong has conditions.

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A theorem this useful earns its fine
print, and there are three clauses.

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Beside them, the shop again,
to test each clause against.

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First: the draws must be independent,
and all from one population.

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Our machine had that by construction.

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Real data, measured over time
or across neighbours, has to earn it.

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Second: sigma must be finite.

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Here is a population that breaks the rule:

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this red tail dies away so slowly

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that the spread is infinite, and averages
drawn from it never settle into any bell.

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No sigma, no theorem.

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Third: how large n must be depends
on the shape you start from.

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Our shop's mild tail
was nearly gone by n equals four;

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a harsher skew takes more averaging.

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The theorem promises
the bell in the limit,

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and the shape decides
the price of getting there.

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Now spend the theorem on the thing
you meet everywhere: the error bar.

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A lab measures something noisy,

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averages n readings, and reports
the average: three point one.

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An honest report also says how far
off that number is likely to be.

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The theorem is the answer.

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That reported average was one draw from
a bell whose width is sigma over root n,

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and here that width is zero point two.

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So draw the bar: from two
point nine to three point three,

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one width each side of the reading.

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That is the error bar, drawn.

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So a quoted plus or minus is not
decoration, and it is not a guess.

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It is this theorem, applied:

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the width of the normal
curve the average came from.

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Wherever an error bar stands,
a bell stands behind it.

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One curve carries the whole lecture.

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Here is the noise in the average,

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sigma over root n,
plotted against the sample size.

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At n equals four it
stood at zero point nine.

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At sixteen, zero point four five.

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At sixty-four, zero point two two five.

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The curve falls like one over root n,

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so each halving of the noise
costs a quadrupling of the data.

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That is why large experiments are large,

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and why the last decimal place
is always the expensive one.

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And that is the Central Limit Theorem.

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Averages forget the shape they
were drawn from, remember the mean,

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and close in on it like root n.

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The bell was never
hiding in the population.

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Averaging builds it, every time.