1 00:00:00,000 --> 00:00:06,930 2 00:00:06,930 --> 00:00:07,370 PROFESSOR: Hi. 3 00:00:07,370 --> 00:00:08,980 Welcome back to recitation. 4 00:00:08,980 --> 00:00:12,470 In lecture you've been doing definite integration for the 5 00:00:12,470 --> 00:00:13,730 last couple of lectures. 6 00:00:13,730 --> 00:00:15,610 And you've just started with the 7 00:00:15,610 --> 00:00:17,800 fundamental theorem of calculus. 8 00:00:17,800 --> 00:00:21,370 So, that gives us this whole powerful tool to compute a 9 00:00:21,370 --> 00:00:22,020 bunch of integrals. 10 00:00:22,020 --> 00:00:25,710 So, with that in mind I've got a couple questions for you. 11 00:00:25,710 --> 00:00:27,950 So compute the definite integrals. 12 00:00:27,950 --> 00:00:33,100 The integral from pi over 6 to pi over 3 of tan x dx. 13 00:00:33,100 --> 00:00:36,570 And the integral of minus pi over 3 to pi 14 00:00:36,570 --> 00:00:38,430 over 3 of tan x dx. 15 00:00:38,430 --> 00:00:41,170 So why don't you pause the video, take a couple minutes 16 00:00:41,170 --> 00:00:42,920 to work on those, come back and we'll 17 00:00:42,920 --> 00:00:44,170 work on them together. 18 00:00:44,170 --> 00:00:51,270 19 00:00:51,270 --> 00:00:51,720 All right. 20 00:00:51,720 --> 00:00:52,490 Welcome back. 21 00:00:52,490 --> 00:00:55,520 So, as we were saying we have a couple of 22 00:00:55,520 --> 00:00:56,770 definite integrals here. 23 00:00:56,770 --> 00:01:01,570 So one tool for definite integrals is Riemann sums. So, 24 00:01:01,570 --> 00:01:05,540 in principle, we could write down a Riemann sum for, say, 25 00:01:05,540 --> 00:01:06,980 this first integral here. 26 00:01:06,980 --> 00:01:09,750 And then try and compute it by trying to compute the sum and 27 00:01:09,750 --> 00:01:11,990 taking a limit of it. 28 00:01:11,990 --> 00:01:15,210 But I think it's pretty clear that, for a function like tan 29 00:01:15,210 --> 00:01:18,560 x, that's going to be really, really hard to do. 30 00:01:18,560 --> 00:01:21,380 So we want to not use Riemann sums here. 31 00:01:21,380 --> 00:01:24,760 And the way we can not use Riemann sums is using this 32 00:01:24,760 --> 00:01:26,020 great tool that we have, which is the 33 00:01:26,020 --> 00:01:27,510 fundamental theorem of calculus. 34 00:01:27,510 --> 00:01:29,820 So the fundamental theorem of calculus says, when you have a 35 00:01:29,820 --> 00:01:33,140 definite integral, instead of computing Riemann sums, what 36 00:01:33,140 --> 00:01:35,630 you can do is compute an antiderivative and use the 37 00:01:35,630 --> 00:01:39,640 antiderivative to find out what the integral is. 38 00:01:39,640 --> 00:01:42,160 Just compare two values with the antiderivative and that'll 39 00:01:42,160 --> 00:01:44,380 give you the value of the definite integral. 40 00:01:44,380 --> 00:01:49,140 So, in particular, let's do this first integral first. So 41 00:01:49,140 --> 00:01:55,160 we have the integral from pi over 6 to pi 42 00:01:55,160 --> 00:02:00,380 over 3 of tan x dx. 43 00:02:00,380 --> 00:02:03,240 Well, so, we know what the antiderivative of tan x is. 44 00:02:03,240 --> 00:02:05,220 We did that in an earlier recitation. 45 00:02:05,220 --> 00:02:07,770 So that's ln of cosine x. 46 00:02:07,770 --> 00:02:10,750 Or ln of the absolute value of cosine x. 47 00:02:10,750 --> 00:02:13,710 So, the fundamental theorem of calculus says that the value 48 00:02:13,710 --> 00:02:16,340 of this definite integral, in order to compute it, we just 49 00:02:16,340 --> 00:02:20,600 take the difference of that antiderivative at pi over 3 50 00:02:20,600 --> 00:02:21,740 and at pi over 6. 51 00:02:21,740 --> 00:02:26,310 So, by the fundamental theorem of calculus this is equal to 52 00:02:26,310 --> 00:02:36,270 ln of the absolute value of cosine x for x between pi over 53 00:02:36,270 --> 00:02:41,530 6 and pi over 3. 54 00:02:41,530 --> 00:02:43,990 So, OK, so this, you know, this is this notation that 55 00:02:43,990 --> 00:02:45,490 Professor Jerison introduced. 56 00:02:45,490 --> 00:02:47,030 So what does this actually mean? 57 00:02:47,030 --> 00:02:52,300 It's just a shorthand for ln of the absolute value of 58 00:02:52,300 --> 00:03:00,120 cosine of pi over 3 minus ln of the absolute value of 59 00:03:00,120 --> 00:03:03,390 cosine of pi over 6. 60 00:03:03,390 --> 00:03:05,470 Now, we could leave our answer like this but we can also 61 00:03:05,470 --> 00:03:08,090 manipulate it and put it in a little nicer form. 62 00:03:08,090 --> 00:03:11,950 So, cosine of pi over 3 is-- 63 00:03:11,950 --> 00:03:14,070 oh, I'm sorry I've made a mistake. 64 00:03:14,070 --> 00:03:16,562 So it's not ln of absolute value cosine x. 65 00:03:16,562 --> 00:03:19,160 It's minus ln of absolute value of cosine x. 66 00:03:19,160 --> 00:03:20,460 Sorry about that. 67 00:03:20,460 --> 00:03:24,580 So this is minus ln cosine pi over 3 plus-- 68 00:03:24,580 --> 00:03:27,320 OK, so minus and minus there is plus. 69 00:03:27,320 --> 00:03:28,050 All right. 70 00:03:28,050 --> 00:03:30,580 Sorry about that. 71 00:03:30,580 --> 00:03:32,243 OK, so, good. 72 00:03:32,243 --> 00:03:33,060 All right. 73 00:03:33,060 --> 00:03:35,500 And we can pick up where I was in the middle of my sentence 74 00:03:35,500 --> 00:03:38,670 and OK, so we can just evaluate this by just 75 00:03:38,670 --> 00:03:39,110 evaluating. 76 00:03:39,110 --> 00:03:42,640 So cosine of pi over 3, that's going to be 1/2. 77 00:03:42,640 --> 00:03:45,820 So this is minus ln and absolute value of 78 00:03:45,820 --> 00:03:47,500 1/2 is just a 1/2. 79 00:03:47,500 --> 00:03:53,980 Plus cosine of pi over 6 is square root of 3 over 2. 80 00:03:53,980 --> 00:03:56,530 So plus ln square root of 3 over 2. 81 00:03:56,530 --> 00:03:59,170 And now you can use your logarithm rules to combine 82 00:03:59,170 --> 00:04:01,220 those into a single expression. 83 00:04:01,220 --> 00:04:06,440 So this is equal to ln of square root of 3. 84 00:04:06,440 --> 00:04:09,540 Or you could even use one more logarithm rule if you wanted. 85 00:04:09,540 --> 00:04:13,990 So this is equal to 1/2 ln of 3. 86 00:04:13,990 --> 00:04:17,340 So all of those are, you know, equivalent expressions for the 87 00:04:17,340 --> 00:04:19,740 same number, which is the value of 88 00:04:19,740 --> 00:04:22,050 this definite integral. 89 00:04:22,050 --> 00:04:24,440 OK, so, for the second integral now, we can do 90 00:04:24,440 --> 00:04:28,650 exactly the same thing if we wanted to. 91 00:04:28,650 --> 00:04:30,560 And it'll be a very similar process. 92 00:04:30,560 --> 00:04:35,920 You'll write down this antiderivative here, you'll 93 00:04:35,920 --> 00:04:37,380 take the difference in values. 94 00:04:37,380 --> 00:04:39,230 We can also do something a little bit 95 00:04:39,230 --> 00:04:40,550 clever for this one. 96 00:04:40,550 --> 00:04:43,980 Which is, definite integrals have some geometric 97 00:04:43,980 --> 00:04:45,350 interpretation, right? 98 00:04:45,350 --> 00:04:48,430 And if you think about the function tan x-- 99 00:04:48,430 --> 00:04:52,020 so we could put up a little graph here-- 100 00:04:52,020 --> 00:04:57,930 so in between minus pi over 3 and pi over 3, tan x maybe 101 00:04:57,930 --> 00:05:02,490 looks something like this. 102 00:05:02,490 --> 00:05:04,400 Yeah, you know, give or take. 103 00:05:04,400 --> 00:05:06,080 OK, so what's important about this? 104 00:05:06,080 --> 00:05:08,450 Well tan x is an odd function. 105 00:05:08,450 --> 00:05:10,190 And this interval from-- 106 00:05:10,190 --> 00:05:15,990 this is minus pi over 3 to pi over 3, and this is the curve 107 00:05:15,990 --> 00:05:19,380 y equals tan x. 108 00:05:19,380 --> 00:05:20,850 So this is an odd function. 109 00:05:20,850 --> 00:05:29,390 So the integral in question is this positive area minus this 110 00:05:29,390 --> 00:05:30,510 negative area. 111 00:05:30,510 --> 00:05:32,970 But since it's an odd function, it's symmetric. 112 00:05:32,970 --> 00:05:34,890 So those two cancel out perfectly. 113 00:05:34,890 --> 00:05:36,740 So for the second one, you could do the same 114 00:05:36,740 --> 00:05:37,570 process that we did. 115 00:05:37,570 --> 00:05:40,210 But you can also use a little bit of geometric reasoning to 116 00:05:40,210 --> 00:05:45,290 realize that this second one is just equal to 0. 117 00:05:45,290 --> 00:05:49,010 In either case, doing either of these integral with Riemann 118 00:05:49,010 --> 00:05:51,330 sums would be really atrocious. 119 00:05:51,330 --> 00:05:54,630 So, in both cases, what we're really happy about is that we 120 00:05:54,630 --> 00:05:58,480 have these other tools that allow us to evaluate definite 121 00:05:58,480 --> 00:06:02,370 integrals without going back to the Riemann definition of 122 00:06:02,370 --> 00:06:05,060 the integral. 123 00:06:05,060 --> 00:06:07,810 So, I'm going to stop there. 124 00:06:07,810 --> 00:06:07,901