1 00:00:00,000 --> 00:00:00,900 2 00:00:00,900 --> 00:00:04,429 I think it's very important to have as many ways as possible 3 00:00:04,429 --> 00:00:06,449 to view a certain type of problem, so I want to introduce 4 00:00:06,450 --> 00:00:07,410 you to a different way. 5 00:00:07,410 --> 00:00:10,710 Some people might have taught this first, but the way I 6 00:00:10,710 --> 00:00:15,850 taught it in the first integral video is kind of the way that I 7 00:00:15,849 --> 00:00:17,100 always think about when I do the problems. 8 00:00:17,100 --> 00:00:19,330 But sometimes, it's more useful to think about it the way I'm 9 00:00:19,329 --> 00:00:21,029 about to show you, and maybe you won't see the difference, 10 00:00:21,030 --> 00:00:22,530 or maybe you'll say, oh, Sal, those are just the 11 00:00:22,530 --> 00:00:24,010 exact same thing. 12 00:00:24,010 --> 00:00:26,420 Someone actually emailed me and told me that I should make it 13 00:00:26,420 --> 00:00:28,360 so I can scroll things, and I said, oh, that's not 14 00:00:28,359 --> 00:00:28,809 too hard to do. 15 00:00:28,809 --> 00:00:32,140 So I just did that, and I scrolled my drawing. 16 00:00:32,140 --> 00:00:34,820 But anyway, let's say we have a surface in 3 dimensions. 17 00:00:34,820 --> 00:00:36,119 It's a function of x and y. 18 00:00:36,119 --> 00:00:38,059 You give me a coordinate down here, and I'll tell you 19 00:00:38,060 --> 00:00:40,240 how high the surface is at that point. 20 00:00:40,240 --> 00:00:43,329 And we want to figure out the volume under that surface. 21 00:00:43,329 --> 00:00:44,879 So. 22 00:00:44,880 --> 00:00:49,359 We can very easily figure out the volume of a very small 23 00:00:49,359 --> 00:00:52,210 column underneath the surface. 24 00:00:52,210 --> 00:00:55,870 So this whole volume is what we're trying to figure out, 25 00:00:55,869 --> 00:00:57,019 right, between the dotted lines. 26 00:00:57,020 --> 00:00:59,050 I think you can see it. 27 00:00:59,049 --> 00:01:01,729 You have some experience visualizing this right now. 28 00:01:01,729 --> 00:01:05,939 So let's say that I have a little area here. 29 00:01:05,939 --> 00:01:09,549 We could call that da. 30 00:01:09,549 --> 00:01:12,239 Let me see if I can draw this. 31 00:01:12,239 --> 00:01:15,429 Let's say we have a little area down here, a little 32 00:01:15,430 --> 00:01:17,780 square in the x-y plane. 33 00:01:17,780 --> 00:01:23,579 And it's, depending on how you view it, this side of it is dx, 34 00:01:23,579 --> 00:01:27,480 its length is dx, and the height, you could say, 35 00:01:27,480 --> 00:01:29,700 on that side, is dy. 36 00:01:29,700 --> 00:01:30,390 Right? 37 00:01:30,390 --> 00:01:33,099 Because it's a little small change in y there, and it's a 38 00:01:33,099 --> 00:01:36,489 little small change in x here. 39 00:01:36,489 --> 00:01:40,059 And its area, the area of this little square, is 40 00:01:40,060 --> 00:01:42,799 going to be dx times dy. 41 00:01:42,799 --> 00:01:47,719 And if we wanted to figure out the volume of the solid between 42 00:01:47,719 --> 00:01:52,090 this little area and the surface, we could just multiply 43 00:01:52,090 --> 00:01:54,939 this area times the function. 44 00:01:54,939 --> 00:01:55,250 Right? 45 00:01:55,250 --> 00:01:57,209 Because the height at this point is going to be the 46 00:01:57,209 --> 00:01:59,089 value of the function, roughly, at this point. 47 00:01:59,090 --> 00:01:59,299 Right? 48 00:01:59,299 --> 00:02:00,640 This is going to be an approximation, and then we're 49 00:02:00,640 --> 00:02:01,450 going to take an infinite sum. 50 00:02:01,450 --> 00:02:03,219 I think you know where this is going. 51 00:02:03,219 --> 00:02:04,170 But let me do that. 52 00:02:04,170 --> 00:02:10,479 Let me at least draw the little column that I want to show you. 53 00:02:10,479 --> 00:02:16,689 So that's one end of it, that's another end of it, that's the 54 00:02:16,689 --> 00:02:21,840 front end of it, that's the other end of it. 55 00:02:21,840 --> 00:02:25,659 So we have a little figure that looks something like that. 56 00:02:25,659 --> 00:02:28,180 A little column, right? 57 00:02:28,180 --> 00:02:30,400 It intersects the top of the surface. 58 00:02:30,400 --> 00:02:33,950 And the volume of this column, not too difficult. 59 00:02:33,949 --> 00:02:38,419 It's going to be this little area down here, which is, 60 00:02:38,419 --> 00:02:39,359 we could call that da. 61 00:02:39,360 --> 00:02:41,870 62 00:02:41,870 --> 00:02:43,300 Sometimes written like that. da. 63 00:02:43,300 --> 00:02:44,564 It's a little area. 64 00:02:44,564 --> 00:02:47,889 And we're going to multiply that area times the height of 65 00:02:47,889 --> 00:02:51,279 this column, and that's the function at that point. 66 00:02:51,280 --> 00:02:56,259 So it's f of x and y. 67 00:02:56,259 --> 00:02:58,969 And of course, we could have also written it as, this 68 00:02:58,969 --> 00:03:02,590 da is just dx times dy, or dy times dx. 69 00:03:02,590 --> 00:03:04,920 I'm going to write it in every different way. 70 00:03:04,919 --> 00:03:08,259 So we could also have written this as f of 71 00:03:08,259 --> 00:03:12,509 xy times dx times dy. 72 00:03:12,509 --> 00:03:14,729 And of course, since multiplication is associative, 73 00:03:14,729 --> 00:03:21,139 I could have also written it as f of xy times dy dx. 74 00:03:21,139 --> 00:03:24,269 These are all equivalent, and these all represent the volume 75 00:03:24,270 --> 00:03:29,010 of this column, that's the between this little area 76 00:03:29,009 --> 00:03:31,549 here and the surface. 77 00:03:31,550 --> 00:03:35,980 So now, if we wanted to figure out the volume of the entire 78 00:03:35,979 --> 00:03:37,849 surface, we have a couple of things we could do. 79 00:03:37,849 --> 00:03:42,120 We could add up all of the volumes in the x-direction, 80 00:03:42,120 --> 00:03:45,230 between the lower x-bound and the upper x-bound, and then 81 00:03:45,229 --> 00:03:49,329 we'd have kind of a thin sheet, although it will already have 82 00:03:49,330 --> 00:03:51,710 some depth, because we're not adding up just the x's. 83 00:03:51,710 --> 00:03:53,060 There's also a dy back there. 84 00:03:53,060 --> 00:03:56,870 So we would have a volume of a figure that would extend from 85 00:03:56,870 --> 00:04:03,170 the lower x all the way to the upper x, go back dy, 86 00:04:03,169 --> 00:04:04,209 and come back here. 87 00:04:04,210 --> 00:04:07,390 If we wanted to sum up all the dx's. 88 00:04:07,389 --> 00:04:11,049 And if we wanted to do that, which expression would we use? 89 00:04:11,050 --> 00:04:15,800 Well, we would be summing with respect to x first, so we could 90 00:04:15,800 --> 00:04:17,040 use this expression, right? 91 00:04:17,040 --> 00:04:19,629 92 00:04:19,629 --> 00:04:21,034 And actually, we could write it here, but it 93 00:04:21,035 --> 00:04:21,970 just becomes confusing. 94 00:04:21,970 --> 00:04:24,880 If we're summing with respect to x, but we have the 95 00:04:24,879 --> 00:04:26,110 dy written here first. 96 00:04:26,110 --> 00:04:28,430 It's really not incorrect, but it just becomes a little 97 00:04:28,430 --> 00:04:30,740 ambiguous, are we summing with respect to x or y. 98 00:04:30,740 --> 00:04:32,430 But here, we could say, OK. 99 00:04:32,430 --> 00:04:36,139 If we want to sum up all the dx's first, let's do that. 100 00:04:36,139 --> 00:04:38,889 We're taking the sum with respect to x, and let me, I'm 101 00:04:38,889 --> 00:04:41,269 going to write down the actual, normally I just write numbers 102 00:04:41,269 --> 00:04:44,209 here, but I'm going to say, well, the lower bound here is x 103 00:04:44,209 --> 00:04:51,319 is equal to a, and the upper bound here is x is equal to b. 104 00:04:51,319 --> 00:04:54,649 105 00:04:54,649 --> 00:04:57,379 And that'll give us the volume of, you could imagine a 106 00:04:57,379 --> 00:04:59,329 sheet with depth, right? 107 00:04:59,329 --> 00:05:03,759 The sheet is going to be parallel to the x-axis, right? 108 00:05:03,759 --> 00:05:07,060 And then once we have that sheet, in my video, I think 109 00:05:07,060 --> 00:05:10,280 that's the newspaper people trying to sell me something. 110 00:05:10,279 --> 00:05:11,039 Anyway. 111 00:05:11,040 --> 00:05:13,470 So once we have the sheet, I'll try to draw it here, too, I 112 00:05:13,470 --> 00:05:16,930 don't want to get this picture too muddied up, but once we 113 00:05:16,930 --> 00:05:20,009 have that sheet, then we can integrate those, we can 114 00:05:20,009 --> 00:05:21,360 add up the dy's, right? 115 00:05:21,360 --> 00:05:23,480 Because this width right here is still dy. 116 00:05:23,480 --> 00:05:25,300 We could add up of all the different dy's, and we 117 00:05:25,300 --> 00:05:27,389 would have the volume of the whole figure. 118 00:05:27,389 --> 00:05:30,909 So once we take this sum, then we could take this sum. 119 00:05:30,910 --> 00:05:35,320 Where y is going from it's bottom, which we said with c, 120 00:05:35,319 --> 00:05:39,230 from y is equal to c to y's upper bound, to y 121 00:05:39,230 --> 00:05:42,069 is equal to d. 122 00:05:42,069 --> 00:05:42,689 Fair enough. 123 00:05:42,689 --> 00:05:45,339 And then, once we evaluate this whole thing, we have the 124 00:05:45,339 --> 00:05:49,519 volume of this solid, or the volume under the surface. 125 00:05:49,519 --> 00:05:51,329 Now we could have gone the other way. 126 00:05:51,329 --> 00:05:53,810 I know this gets a little bit messy, but I think 127 00:05:53,810 --> 00:05:54,839 you get what I'm saying. 128 00:05:54,839 --> 00:05:57,185 Let's start with that little da we had originally. 129 00:05:57,185 --> 00:06:00,280 130 00:06:00,279 --> 00:06:04,519 Instead of going this way, instead of summing up the dx's 131 00:06:04,519 --> 00:06:08,909 and getting this sheet, let's sum up the dy's first, right? 132 00:06:08,910 --> 00:06:12,570 So we could take, we're summing in the y-direction first. 133 00:06:12,569 --> 00:06:16,420 We would get a sheet that's parallel to the y-axis, now. 134 00:06:16,420 --> 00:06:21,770 So the top of the sheet would look something like that. 135 00:06:21,769 --> 00:06:25,704 So if we're coming the dy's first, we would take the sum, 136 00:06:25,704 --> 00:06:28,779 we would take the integral with respect to y, and it would be, 137 00:06:28,779 --> 00:06:33,459 the lower bound would be y is equal to c, and the upper 138 00:06:33,459 --> 00:06:36,599 bound is y is equal to d. 139 00:06:36,600 --> 00:06:39,346 And then we would have that sheet with a little depth, the 140 00:06:39,346 --> 00:06:44,790 depth is dx, and then we could take the sum of all of those, 141 00:06:44,790 --> 00:06:46,580 sorry, my throat is dry. 142 00:06:46,579 --> 00:06:50,289 I just had a bunch of almonds to get power to be able 143 00:06:50,290 --> 00:06:52,069 to record these videos. 144 00:06:52,069 --> 00:06:54,230 But once I have one of these sheets, and if I want to sum up 145 00:06:54,230 --> 00:06:58,180 all of the x's, then I could take the infinite sum of 146 00:06:58,180 --> 00:07:02,519 infinitely small columns, or in this view, sheets, infinitely 147 00:07:02,519 --> 00:07:08,199 small depths, and the lower bound is x is equal to a, and 148 00:07:08,199 --> 00:07:10,099 the upper bound is x is equal to b. 149 00:07:10,100 --> 00:07:12,660 And once again, I would have the volume of the figure. 150 00:07:12,660 --> 00:07:15,930 And all I showed you here is that there's two ways of doing 151 00:07:15,930 --> 00:07:17,790 the order of integration. 152 00:07:17,790 --> 00:07:21,060 Now, another way of saying this, if this little original 153 00:07:21,060 --> 00:07:24,189 square was da, and this is a shorthand that you'll see all 154 00:07:24,189 --> 00:07:27,300 the time, especially in physics textbooks, is that we 155 00:07:27,300 --> 00:07:33,439 are integrating along the domain, right? 156 00:07:33,439 --> 00:07:35,769 Because the x-y plane here is our domain. 157 00:07:35,769 --> 00:07:37,689 So we're going to do a double integral, a two-dimensional 158 00:07:37,689 --> 00:07:40,132 integral, we're saying that the domain here is two-dimensional, 159 00:07:40,132 --> 00:07:48,110 and we're going to take that over f of x and y times da. 160 00:07:48,110 --> 00:07:51,240 And the reason why I want to show you this, is you see this 161 00:07:51,240 --> 00:07:53,829 in physics books all the time. 162 00:07:53,829 --> 00:07:55,300 I don't think it's a great thing to do. 163 00:07:55,300 --> 00:07:58,860 Because it is a shorthand, and maybe it looks simpler, but for 164 00:07:58,860 --> 00:08:00,920 me, whenever I see something that I don't know how to 165 00:08:00,920 --> 00:08:04,180 compute or that's not obvious for me to know how to compute, 166 00:08:04,180 --> 00:08:06,319 it actually is more confusing. 167 00:08:06,319 --> 00:08:09,259 So I wanted to just show you that what you see in this 168 00:08:09,259 --> 00:08:12,079 physics book, when someone writes this, it's the exact 169 00:08:12,079 --> 00:08:14,349 same thing as this or this. 170 00:08:14,350 --> 00:08:18,170 The da could either be dx times dy, or it could either be dy 171 00:08:18,170 --> 00:08:21,420 times dx, and when they do this double integral over domain, 172 00:08:21,420 --> 00:08:24,379 that's the same thing is just adding up all of these squares. 173 00:08:24,379 --> 00:08:26,550 Where we do it here, we're very ordered about it, right? 174 00:08:26,550 --> 00:08:30,579 We go in the x-direction, and then we add all of those up in 175 00:08:30,579 --> 00:08:32,350 the y-direction, and we get the entire volume. 176 00:08:32,350 --> 00:08:34,019 Or we could go the other way around. 177 00:08:34,019 --> 00:08:36,579 When we say that we're just taking the double integral, 178 00:08:36,580 --> 00:08:37,950 first of all, that tells us we're doing it in two 179 00:08:37,950 --> 00:08:40,710 dimensions, over a domain, that leaves it a little bit 180 00:08:40,710 --> 00:08:43,790 ambiguous in terms of how we're going to sum 181 00:08:43,789 --> 00:08:45,429 up all of the da's. 182 00:08:45,429 --> 00:08:47,989 And they do it intentionally in physics books, because you 183 00:08:47,990 --> 00:08:50,750 don't have to do it using Cartesian coordinates, 184 00:08:50,750 --> 00:08:51,720 using x's and y's. 185 00:08:51,720 --> 00:08:53,940 You can do it in polar coordinates, you could do it 186 00:08:53,940 --> 00:08:55,260 a ton of different ways. 187 00:08:55,259 --> 00:08:58,200 But I just wanted to show you, this is another way to 188 00:08:58,200 --> 00:09:00,870 having an intuition of the volume under a surface. 189 00:09:00,870 --> 00:09:04,620 And these are the exact same things as this type of 190 00:09:04,620 --> 00:09:07,840 notation that you might see in a physics book. 191 00:09:07,840 --> 00:09:09,420 Sometimes they won't write a domain, sometimes they'd 192 00:09:09,419 --> 00:09:11,250 write over a surface. 193 00:09:11,250 --> 00:09:12,429 And we'll later do those integrals. 194 00:09:12,429 --> 00:09:15,079 Here the surface is easy, it's a flat plane, but sometimes 195 00:09:15,080 --> 00:09:17,379 it'll end up being a curve or something like that. 196 00:09:17,379 --> 00:09:19,789 But anyway, I'm almost out of time. 197 00:09:19,789 --> 00:09:22,389 I will see you in the next video. 198 00:09:22,389 --> 00:09:23,500