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6. Continous Distributions 6. Continous Distributions Chris Piech and Mehran Sahami May 2017 So far, all random variables we have seen have been discrete. In all the cases we have seen in CS109 this meant that our RVs could only take on integer values. Now it’s time for continuous random variables which can take on values in the real number domain (R). Continuous random variables can be used to represent measurements with arbitrary precision (eg height, weight, time). 1 Probability Density Functions In the world of discrete random variables, the most important property of a random variable was its probability mass function (PMF) that would tell you the probability of the random variable taking on any value. When we move to the world of continuous random variables, we are going to need to rethink this basic concept. If I were to ask you, what is the probability of a child being born with weight exactly = 3:523112342234 kilos, you might recognize that question as ridiculous. No child will have precisely that weight. Real values can have infinite precision and as such it is a bit mind boggling to think about the probability that a random variable takes on a specific value. The PMF doesn’t apply. We need another idea. In the continuous world, every random variable has a Probability Density Function (PDF) which says how likely it is that a random variable takes on a particular value, relative to other values that it could take on. The PDF has the nice property that you can integrate over it to find the probability that the random variable takes on values within a range (a;b). X is a Continuous Random Variable if there is a Probability Density Function (PDF) f (x) for −¥ ≤ x ≤ ¥ such that: Z b P(a ≤ X ≤ b) = f (x)dx a The following properties must also hold. These preserve the axiom that P(a ≤ X ≤ b) is a probability: 0 ≤ P(a ≤ X ≤ b) ≤ 1 P(−¥ < X < ¥) = 1 A common misconception is to think of f (x) as a probability. It is instead what we call a probability density. It represents probability/unit of X. Generally this is only meaningful when we either take an integral over the PDF or we compare probability densities. As we mentioned when motivating probability densities, the probability that a continuous random variable takes on a specific value (to infinite precision) is 0. Z a P(X = a) = f (x)dx = 0 a That is pretty different than in the discrete world where we often talked about the probability of a random variable taking on a particular value. 1 2 Cumulative Distribution Function Having a probability density is great, but it means we are going to have to solve an integral every single time we want to calculate a probability. To avoid this unfortunate fate, we are going to use a standard called a cumulative distribution function (CDF). The CDF is a function which takes in a number and returns the probability that a random variable takes on a value less than that number. It has the pleasant property that, if we have a CDF for a random variable, we don’t need to integrate to answer probability questions! For a continuous random variable X the Cumulative Distribution Function, written F(a) is: Z a FX (a) = P(X ≤ a) = f (x)dx −¥ Why is the CDF the probability that a random variable takes on a value less than the input value as opposed to greater than? It is a matter of convention. But it is a useful convention. Most probability questions can be solved simply by knowing the CDF (and taking advantage of the fact that the integral over the range −¥ to ¥ is 1. Here are a few examples of how you can answer probability questions by just using a CDF: Probability Query Solution Explanation P(X < a) F(a) That is the definition of the CDF P(X ≤ a) F(a) Trick question. P(X = a) = 0 P(X > a) 1 − F(a) P(X < a) + P(X > a) = 1 P(a < X < b) F(b) − F(a) F(a) + P(a < X < b) = F(b) The continuous distribution also exists for discrete random variables, but there is less utility to a CDF in the discrete world as none of our discrete random variables had “closed form” (eg without any summation) functions for the CDF: a FX (a) = ∑ P(X = i) i=1 Example 1 Let X be a continuous random variable (CRV) with PDF: ( C(4x − 2x2) when 0 < x < 2 f (x) = 0 otherwise In this function, C is a constant. What value is C? Since we know that the PDF must sum to 1: Z 2 C(4x − 2x2)dx = 1 0 3 2 2 2x C 2x − = 1 3 0 16 C 8 − − 0 = 1 3 And if you solve the equation for C you find that C = 3=8. 2 What is P(X > 1) Z ¥ Z 2 3 2 3 2 3 2 2x 3 16 2 1 f (x)dx = (4x − 2x )dx = 2x − = 8 − − 2 − = 1 1 8 8 3 1 8 3 3 2 Example 2 Let X be a random variable which represents the number of days of use before your disk crashes with PDF: ( le−x=100 when x ≥ 0 f (x) = 0 otherwise First, determine l. Recall that R eudu = eu: Z Z −1 le−x=100dx = 1 ) −100l e−x=100dx = 1 100 ¥ −x=100 1 − 100le = 1 ) 100l = 1 ) l = 0 100 What is the P(X < 10)? Z 10 10 1 −x=100 −x=100 −1=10 F(10) = e dx = −e = −e + 1 ≈ 0:095 0 100 0 For a discrete random variable X, the Cumulative Distribution Function (CDF) is defined as: F(a) = P(X ≤ a) where − ¥ < a < ¥ 3 Expectation and Variance For continuous RV X: Z ¥ E[X] = x f (x)dx −¥ Z ¥ E[g(X)] = g(x) f (x)dx −¥ Z ¥ E[Xn] = xn f (x)dx −¥ For both continuous and discrete RVs: E[aX + b] = aE[X] + b Var(X) = E[(X − m)2] = E[X2] − (E[X])2 Var(aX + b) = a2Var(X) 4 Uniform Random Variable The most basic of all the continuous random variables is the uniform random variable, which is equally likely to take on any value in its range (a;b). 3 X is a Uniform Random Variable X ∼ Uni(a;b) if it has PDF: ( 1 when a ≤ x ≤ b f (x) = b−a 0 otherwise Notice how the density (1=(b − a) is exactly the same regardless of the value for x. That makes the density uniform. So why is the PDF (1=(b − a) and not 1? That is the constant that makes it such that the integral over all possible inputs evaluates to 1. The key properties of this RV are: Z b b − a P(a ≤ X ≤ b) = f (x)dx = (for a ≤ a ≤ b ≤ b) a b − a 2 b Z ¥ Z b x x a + b E[X] = x f (x)dx = dx = = −¥ a b − a 2(b − a) a 2 (b − a)2 Var(X) = 12 5 Normal Random Variable The single most important random variable type is the Normal (aka Gaussian) random variable, parametrized by a mean (m) and variance (s 2). If X is a normal variable we write X ∼ N(m;s 2). The normal is important for many reasons: it is generated from the summation of independent random variables and as a result it occurs often in nature. Many things in the world are not distributed normally but data scientists and computer scientists model them as Normal distributions anyways. Why? Because it is the most entropic (conservative) modelling decision that we can make for a random variable while still matching a particular expectation (average value) and variance (spread). The Probability Density Function (PDF) for a Normal X ∼ N(m;s 2) is: −(x−m)2 1 2 fX (x) = p e 2s s 2p Notice the x in the exponent of the PDF function. When x is equal to the mean (m) then e is raised to the power of 0 and the PDF is maximized. By definition a Normal has E[X] = m and Var(X) = s 2. There is no closed form for the integral of the Normal PDF, and as such there is no closed form CDF. However we can use a transformation of any normal to a normal with a precomputed CDF. The result of this mathematical gymnastics is that the CDF for a Normal X ∼ N(m;s 2) is: x − m FX (x) = F s Where F is a precomputed function that represents that CDF of the Standard Normal. Linear Transform If X is a Normal such that X ∼ N(m;s 2) and Y is a linear transform of X such that Y = aX + b then Y is also a Normal where: Y ∼ N(am + b;a2s 2) 4 Projection to Standard Normal For any Normal X we can find a linear transform from X to the standard normal ∼ N(0;1). For any normal, if you subtract the mean (m) of the normal and divide by the standard deviation (s) the result is always the X−m standard normal. We can prove this mathematically. Let W = s : X − m W = Transform X: Subtract by m and diving by s s 1 m = X − Use algebra to rewrite the equation s s 1 m = aX + b Where a = , b = − m s ∼ N(am + b;a2s 2) The linear transform of a Normal is another Normal m m s 2 ∼ N( − ; ) Substituting values in for a and b s s s 2 ∼ N(0;1) The standard normal Using this transform we can express FX (x), the CDF of X, in terms of the known CDF of Z, FZ(x).
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