1 00:00:00,260 --> 00:00:03,320 In this lecture, we will deal with a single topic. 2 00:00:03,320 --> 00:00:07,910 How to find the distribution, that is, the PMF or PDF of a 3 00:00:07,910 --> 00:00:10,880 random variable that is defined as a function of one 4 00:00:10,880 --> 00:00:16,740 or more other random variables with known distributions. 5 00:00:16,740 --> 00:00:18,720 Why is this useful? 6 00:00:18,720 --> 00:00:22,120 Quite often, we construct a model by first defining some 7 00:00:22,120 --> 00:00:24,230 basic random variables. 8 00:00:24,230 --> 00:00:28,340 These random variables usually have simple distributions and 9 00:00:28,340 --> 00:00:31,130 often they are independent. 10 00:00:31,130 --> 00:00:34,780 But we may be interested in the distribution of some more 11 00:00:34,780 --> 00:00:38,510 complicated random variables that are defined in terms of 12 00:00:38,510 --> 00:00:41,740 our basic random variables. 13 00:00:41,740 --> 00:00:45,430 In this lecture, we will develop systematic methods for 14 00:00:45,430 --> 00:00:47,430 the task at hand. 15 00:00:47,430 --> 00:00:50,830 After going through a warm-up, the case of discrete random 16 00:00:50,830 --> 00:00:54,460 variables, we will see that there is a general, very 17 00:00:54,460 --> 00:00:58,750 systematic 2-step procedure that relies on cumulative 18 00:00:58,750 --> 00:01:01,990 distribution functions. 19 00:01:01,990 --> 00:01:04,970 We will pay special attention to the easier case where we 20 00:01:04,970 --> 00:01:08,450 have a linear function of a single random variable. 21 00:01:08,450 --> 00:01:11,370 We will also see that when the function involved is 22 00:01:11,370 --> 00:01:16,650 monotonic, we can bypass CDFs and jump directly to a formula 23 00:01:16,650 --> 00:01:19,430 that is easy to apply. 24 00:01:19,430 --> 00:01:23,070 We will also see an example involving a function of two 25 00:01:23,070 --> 00:01:24,700 random variables. 26 00:01:24,700 --> 00:01:27,440 In such examples, the calculations may be more 27 00:01:27,440 --> 00:01:31,650 complicated but the basic approach based on CDFs is 28 00:01:31,650 --> 00:01:33,840 really the same. 29 00:01:33,840 --> 00:01:36,160 Let me close with a final comment. 30 00:01:36,160 --> 00:01:39,620 Finding the distribution of the function g of X is indeed 31 00:01:39,620 --> 00:01:43,970 possible, but we should only do it when we really need it. 32 00:01:43,970 --> 00:01:48,440 If all we care about is the expected value of g of X we 33 00:01:48,440 --> 00:01:50,570 can just use the expected value rule.