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rLlZpnT02ZU
I'm actually stuck.
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This A star is the one that actually maximizes
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the integral of this function.
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So we used the fact that for any function,
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say delta, the integral over A of delta
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is less than the integral over the set of X's
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such that delta of X is non-negative of delta of X, dx.
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And that's an obvious fact, just by picture, say.
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And that's true for all A. Yeah?
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AUDIENCE: [INAUDIBLE] could you use
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like a portion under the axis as like less than
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or equal to the portion above the axis?
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PHILIPPE RIGOLLET: It's actually equal.
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We know that the integral of f minus g--
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the integral of delta is 0.
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So there's actually exactly the same area above and below.
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But yeah, you're right.
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You could go to the extreme cases.
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You're right.
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No.
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It's actually still be true, even if there was--
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if this was a constant, that would still be true.
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Here, I never use the fact that the integral is equal to 0.
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I could shift this function by 1 so that the integral of delta
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is equal to 1, and it would still
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be true that it's maximized when I take A to be
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the set where it's positive.
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Just need to make sure that there is someplace where it is,
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but that's about it.
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Of course, we used this before, when we made this thing.
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But just the last argument, this last fact
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does not require that.
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All right.
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So now we have this notion of--
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I need the--
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OK.
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So we have this notion of distance
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between probability measures.
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I mean, these things are exactly what--
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if I were to be in a formal math class and I said,
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here are the axioms that a distance should satisfy,
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those are exactly those things.
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If it's not satisfying this thing,
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it's called pseudo-distance or quasi-distance or just metric
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or nothing at all, honestly.
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So it's a distance.
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It's symmetric, non-negative, equal to 0,
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if and only if the two arguments are equal, then
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it satisfies the triangle inequality.
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And so that means that we have this actual total variation
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distance between probability distributions.
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And here is now a statistical strategy to implement our goal.
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Remember, our goal was to spit out
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a theta hat, which was close such that P theta
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hat was close to P theta star.
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So hopefully, we were trying to minimize the total variation
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distance between P theta hat and P theta star.
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Now, we cannot do that, because just by this fact, this slide,
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if we wanted to do that directly, we would just take--
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well, let's take theta hat equals theta star and that will
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give me the value 0.
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And that's the minimum possible value we can take.
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The problem is that we don't know
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what the total variation is to something that we don't know.
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We know how to compute total variations if I give you
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the two arguments.
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But here, one of the arguments is not known.
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P theta star is not known to us, so we need to estimate it.
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And so here is the strategy.
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Just build an estimator of the total variation
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distance between P theta and P theta star
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for all candidate theta, all possible theta
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in capital theta.
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Now, if this is a good estimate, then when I minimize it,
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I should get something that's close to P theta star.
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So here's the strategy.
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This is my function that maps theta
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to the total variation between P theta and P theta star.
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I know it's minimized at theta star.
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That's definitely TV of P-- and the value here, the y-axis
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should say 0.
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And so I don't know this guy, so I'm
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going to estimate it by some estimator that
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comes from my data.
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Hopefully, the more data I have, the better this estimator is.
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And I'm going to try to minimize this estimator now.
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And if the two things are close, then the minima
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should be close.
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That's a pretty good estimation strategy.
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The problem is that it's very unclear
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how you would build this estimator of TV,
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of the Total Variation.
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So building estimators, as I said,
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typically consists in replacing expectations by averages.
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But there's no simple way of expressing the total variation
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distance as the expectations with respect
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to theta star of anything.
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So what we're going to do is we're
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going to move from total variation distance
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to another notion of distance that sort of has