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rLlZpnT02ZU
if you do it for each simple event, it's little x.
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It's actually simple.
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Now, if we have continuous random variables-- so
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by the way, I didn't mention, but discrete means Bernoulli.
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Binomial, but not only those that have finite support,
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like Bernoulli has support of size 2,
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binomial NP has support of size n--
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there's n possible values it can take-- but also Poisson.
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Poisson distribution can take an infinite number
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of values, all the positive integers,
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non-negative integers.
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And so now we have also the continuous ones,
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such as Gaussian, exponential.
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And what characterizes those guys is that they
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have a probability density.
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So the density, remember the way I
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use my density is when I want to compute
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the probability of belonging to some event A.
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The probability of X falling to some subset of the real line A
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is simply the integral of the density on this set.
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That's the famous area under the curve thing.
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So since for each possible value, the probability at X--
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so I hope you remember that stuff.
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That's just probably something that you
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must remember from probability.
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But essentially, we know that the probability that X is equal
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to little x is 0 for a continuous random variable,
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for all possible X's.
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There's just none of them that actually gets weight.
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So what we have to do is to describe the fact that it's
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in some little region.
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So the probability that it's in some interval, say, a, b, this
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is the integral between A and B of f theta of X, dx.
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So I have this density, such as the Gaussian one.
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And the probability that I belong to the interval a,
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b is just the area under the curve between A and B.
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If you don't remember that, please take immediate remedy.
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So this function f, just like P, is non-negative.
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And rather than summing to 1, it integrates to 1
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when I integrate it over the entire sample space E.
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And now the total variation, well, it
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takes basically the same form.
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I said that you essentially replace sums
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by integrals when you're dealing with densities.
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And here, it's just saying, rather than having
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1/2 of the sum of the absolute values,
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you have 1/2 of the integral of the absolute value
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of the difference.
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Again, if I give you two densities
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and if you're not too bad at calculus, which you will often
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be, because there's lots of them you can actually not compute.
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But if I gave you, for example, two Gaussian densities,
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exponential minus x squared, blah, blah, blah, and I say,
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just compute the total variation distance,
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you could actually write it as an integral.
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Now, whether you can actually reduce this integral
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to some particular number is another story.
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But you could technically do it.
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So now, you have actually a handle on this thing
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and you could technically ask Mathematica,
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whereas asking Mathematica to take
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the max over all possible events is going to be difficult.
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All right.
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So the total variation has some properties.
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So let's keep on the board the definition that
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involves, say, the densities.
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So think Gaussian in your mind.
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And you have two Gaussians, one with mean theta
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and one with mean theta prime.
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And I'm looking at the total variation between those two
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guys.
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So if I look at P theta minus--
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sorry.
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TV between P theta and P theta prime, this
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is equal to 1/2 of the integral between f theta, f theta prime.
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And when I don't write it--
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so I don't write the X, dx but it's there.
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And then I integrate over E.
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So what is this thing doing for me?
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It's just saying, well, if I have-- so
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think of two Gaussians.
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For example, I have one that's here and one that's here.
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So this is let's say f theta, f theta prime.
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This guy is doing what?
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It's computing the absolute value of the difference
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between f and f theta prime.
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You can check for yourself that graphically, this I
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can represent as an area not under the curve,
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but between the curves.
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So this is this guy.
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Now, this guy is really the integral of the absolute value.
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So this thing here, this area, this
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is 2 times the total variation.
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The scaling 1/2 really doesn't matter.
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It's just if I want to have an actual correspondence
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between the maximum and the other guy, I have to do this.
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So this is what it looks like.
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So we have this definition.
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And so we have a couple of properties that come into this.
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The first one is that it's symmetric.