1 00:00:06,787 --> 00:00:07,370 PROFESSOR: Hi. 2 00:00:07,370 --> 00:00:08,980 Welcome back to recitation. 3 00:00:08,980 --> 00:00:12,220 In lecture you've been doing definite integration 4 00:00:12,220 --> 00:00:13,730 for the last couple of lectures. 5 00:00:13,730 --> 00:00:16,420 And you've just started with the fundamental theorem 6 00:00:16,420 --> 00:00:17,800 of calculus. 7 00:00:17,800 --> 00:00:20,687 So, that gives us this whole powerful tool 8 00:00:20,687 --> 00:00:22,020 to compute a bunch of integrals. 9 00:00:22,020 --> 00:00:25,710 So, with that in mind, I've got a couple questions for you. 10 00:00:25,710 --> 00:00:27,950 So compute the definite integrals. 11 00:00:27,950 --> 00:00:33,100 The integral from pi over 6 to pi over 3 of tan x dx. 12 00:00:33,100 --> 00:00:37,820 And the integral of minus pi over 3 to pi over 3 of tan x 13 00:00:37,820 --> 00:00:38,430 dx. 14 00:00:38,430 --> 00:00:40,290 So why don't you pause the video, 15 00:00:40,290 --> 00:00:42,497 take a couple minutes to work on those, come back 16 00:00:42,497 --> 00:00:43,830 and we'll work on them together. 17 00:00:51,221 --> 00:00:51,720 All right. 18 00:00:51,720 --> 00:00:52,490 Welcome back. 19 00:00:52,490 --> 00:00:55,390 So, as we were saying we have a couple 20 00:00:55,390 --> 00:00:56,770 of definite integrals here. 21 00:00:56,770 --> 00:01:01,280 So one tool for definite integrals is Riemann sums. 22 00:01:01,280 --> 00:01:05,540 So, in principle, we could write down a Riemann sum for, say, 23 00:01:05,540 --> 00:01:06,980 this first integral here. 24 00:01:06,980 --> 00:01:09,540 And then try and compute it by trying to compute the sum 25 00:01:09,540 --> 00:01:11,990 and taking a limit of it. 26 00:01:11,990 --> 00:01:15,210 But I think it's pretty clear that, for a function like tan 27 00:01:15,210 --> 00:01:18,560 x, that's going to be really, really hard to do. 28 00:01:18,560 --> 00:01:21,380 So we want to not use Riemann sums here. 29 00:01:21,380 --> 00:01:23,840 And the way we can not use Riemann sums 30 00:01:23,840 --> 00:01:25,636 is using this great tool that we have, 31 00:01:25,636 --> 00:01:27,510 which is the fundamental theorem of calculus. 32 00:01:27,510 --> 00:01:29,343 So the fundamental theorem of calculus says, 33 00:01:29,343 --> 00:01:32,020 when you have a definite integral, instead of computing 34 00:01:32,020 --> 00:01:35,040 Riemann sums, what you can do is compute an antiderivative 35 00:01:35,040 --> 00:01:39,640 and use the antiderivative to find out what the integral is. 36 00:01:39,640 --> 00:01:41,830 Just compare two values of the antiderivative 37 00:01:41,830 --> 00:01:44,380 and that'll give you the value of the definite integral. 38 00:01:44,380 --> 00:01:48,890 So, in particular, let's do this first integral first. 39 00:01:48,890 --> 00:01:57,850 So we have the integral from pi over 6 to pi over 3 of tan 40 00:01:57,850 --> 00:02:00,380 x dx. 41 00:02:00,380 --> 00:02:03,240 Well, so, we know what the antiderivative of tan x is. 42 00:02:03,240 --> 00:02:05,220 We did that in an earlier recitation. 43 00:02:05,220 --> 00:02:07,770 So that's ln of cosine x. 44 00:02:07,770 --> 00:02:10,750 Or ln of the absolute value of cosine x. 45 00:02:10,750 --> 00:02:12,900 So, the fundamental theorem of calculus 46 00:02:12,900 --> 00:02:14,870 says that the value of this definite integral, 47 00:02:14,870 --> 00:02:16,540 in order to compute it, we just take 48 00:02:16,540 --> 00:02:20,600 the difference of that antiderivative at pi over 3 49 00:02:20,600 --> 00:02:21,740 and at pi over 6. 50 00:02:21,740 --> 00:02:24,170 So, by the fundamental theorem of calculus 51 00:02:24,170 --> 00:02:29,130 this is equal to ln of the absolute value of cosine 52 00:02:29,130 --> 00:02:41,530 x for x between pi over 6 and pi over 3. 53 00:02:41,530 --> 00:02:43,760 So, OK, so this, you know, this is this notation 54 00:02:43,760 --> 00:02:45,490 that Professor Jerison introduced. 55 00:02:45,490 --> 00:02:47,030 So what does this actually mean? 56 00:02:47,030 --> 00:02:54,000 It's just a shorthand for ln of the absolute value of cosine 57 00:02:54,000 --> 00:02:59,990 of pi over 3 minus ln of the absolute value 58 00:02:59,990 --> 00:03:03,224 of cosine of pi over 6. 59 00:03:03,224 --> 00:03:04,890 Now, we could leave our answer like this 60 00:03:04,890 --> 00:03:07,090 but we can also manipulate it and put it 61 00:03:07,090 --> 00:03:08,090 in a little nicer form. 62 00:03:08,090 --> 00:03:14,070 So, cosine of pi over 3 is-- oh, I'm sorry I've made a mistake. 63 00:03:14,070 --> 00:03:16,562 So it's not ln of absolute value cosine x. 64 00:03:16,562 --> 00:03:19,160 It's minus ln of absolute value of cosine x. 65 00:03:19,160 --> 00:03:20,460 Sorry about that. 66 00:03:20,460 --> 00:03:24,920 So this is minus ln cosine pi over 3 plus-- OK, so 67 00:03:24,920 --> 00:03:27,320 minus and minus there is plus. 68 00:03:27,320 --> 00:03:28,050 All right. 69 00:03:28,050 --> 00:03:30,580 Sorry about that. 70 00:03:30,580 --> 00:03:32,243 OK, so, good. 71 00:03:32,243 --> 00:03:33,042 All right. 72 00:03:33,042 --> 00:03:35,500 And we can pick up where I was in the middle of my sentence 73 00:03:35,500 --> 00:03:39,110 and OK, so we can just evaluate this by just evaluating. 74 00:03:39,110 --> 00:03:42,640 So cosine of pi over 3, that's going to be 1/2. 75 00:03:42,640 --> 00:03:47,500 So this is minus ln and absolute value of 1/2 is just a 1/2. 76 00:03:47,500 --> 00:03:53,980 Plus cosine of pi over 6 is square root of 3 over 2. 77 00:03:53,980 --> 00:03:56,530 So plus ln square root of 3 over 2. 78 00:03:56,530 --> 00:03:58,630 And now you can use your logarithm rules 79 00:03:58,630 --> 00:04:01,220 to combine those into a single expression. 80 00:04:01,220 --> 00:04:06,440 So this is equal to ln of square root of 3. 81 00:04:06,440 --> 00:04:09,540 Or you could even use one more logarithm rule if you wanted. 82 00:04:09,540 --> 00:04:13,990 So this is equal to 1/2 ln of 3. 83 00:04:13,990 --> 00:04:17,090 So all of those are, you know, equivalent expressions 84 00:04:17,090 --> 00:04:19,240 for the same number, which is the value 85 00:04:19,240 --> 00:04:22,050 of this definite integral. 86 00:04:22,050 --> 00:04:24,060 OK, so, for the second integral now, we 87 00:04:24,060 --> 00:04:28,650 can do exactly the same thing if we wanted to. 88 00:04:28,650 --> 00:04:30,560 And it'll be a very similar process. 89 00:04:30,560 --> 00:04:35,540 You'll write down this antiderivative here, 90 00:04:35,540 --> 00:04:37,380 you'll take the difference in values. 91 00:04:37,380 --> 00:04:40,550 We can also do something a little bit clever for this one. 92 00:04:40,550 --> 00:04:43,050 Which is, definite integrals have 93 00:04:43,050 --> 00:04:45,350 some geometric interpretation, right? 94 00:04:45,350 --> 00:04:47,120 And if you think about the function tan 95 00:04:47,120 --> 00:04:52,020 x-- so we could put up a little graph here-- 96 00:04:52,020 --> 00:04:57,110 so in between minus pi over 3 and pi over 3, 97 00:04:57,110 --> 00:05:02,490 tan x maybe looks something like this. 98 00:05:02,490 --> 00:05:04,400 Yeah, you know, give or take. 99 00:05:04,400 --> 00:05:06,080 OK, so what's important about this? 100 00:05:06,080 --> 00:05:08,450 Well tan x is an odd function. 101 00:05:08,450 --> 00:05:14,520 And this interval from-- this is minus pi over 3 to pi over 3, 102 00:05:14,520 --> 00:05:19,380 and this is the curve y equals tan x. 103 00:05:19,380 --> 00:05:20,850 So this is an odd function. 104 00:05:20,850 --> 00:05:28,630 So the integral in question is this positive area 105 00:05:28,630 --> 00:05:30,510 minus this negative area. 106 00:05:30,510 --> 00:05:32,970 But since it's an odd function, it's symmetric. 107 00:05:32,970 --> 00:05:34,890 So those two cancel out perfectly. 108 00:05:34,890 --> 00:05:37,070 So for the second one, you could do the same process 109 00:05:37,070 --> 00:05:37,570 that we did. 110 00:05:37,570 --> 00:05:40,090 But you can also use a little bit of geometric reasoning 111 00:05:40,090 --> 00:05:45,290 to realize that this second one is just equal to 0. 112 00:05:45,290 --> 00:05:48,390 In either case, doing either of these integral 113 00:05:48,390 --> 00:05:51,330 with Riemann sums would be really atrocious. 114 00:05:51,330 --> 00:05:54,300 So, in both cases, what we're really happy about 115 00:05:54,300 --> 00:05:56,370 is that we have these other tools that 116 00:05:56,370 --> 00:05:59,890 allow us to evaluate definite integrals without going back 117 00:05:59,890 --> 00:06:05,060 to the Riemann definition of the integral. 118 00:06:05,060 --> 00:06:07,401 So, I'm going to stop there.