1 00:00:00 --> 00:00:00 2 00:00:00 --> 00:00:02 The following content is provided under a Creative 3 00:00:02 --> 00:00:03 Commons license. 4 00:00:03 --> 00:00:06 Your support will help MIT OpenCourseWare continue to 5 00:00:06 --> 00:00:09 offer high quality educational resources for free. 6 00:00:09 --> 00:00:12 To make a donation or to view additional materials from 7 00:00:12 --> 00:00:15 hundreds of MIT courses, visit MIT OpenCourseWare 8 00:00:15 --> 00:00:21 at ocw.mit.edu. 9 00:00:21 --> 00:00:23 PROFESSOR: And this last little bit is something 10 00:00:23 --> 00:00:25 which is not yet on the Web. 11 00:00:25 --> 00:00:27 But, anyway, when I was walking out of the room last time, I 12 00:00:27 --> 00:00:32 noticed that I'd written down the wrong formula for c1 - c1. 13 00:00:32 --> 00:00:35 There's a misprint, there's a minus sign that's wrong. 14 00:00:35 --> 00:00:39 I claimed last time that c1 - c2 was + 1/2. 15 00:00:39 --> 00:00:40 But, actually, it's - 1/2. 16 00:00:40 --> 00:00:42 If you go through the calculation that we did with 17 00:00:42 --> 00:00:46 the antiderivative of sine x cosine x, we get these 18 00:00:46 --> 00:00:48 two possible answers. 19 00:00:48 --> 00:00:52 And if they're to be equal, then if we just subtract them 20 00:00:52 --> 00:00:56 we get c1 - c2 + 1/2 = 0. 21 00:00:56 --> 00:01:01 So c1 - c2 = 1/2. 22 00:01:01 --> 00:01:03 So, those are all of the correction. 23 00:01:03 --> 00:01:06 Again, everything here will be on the Web. 24 00:01:06 --> 00:01:14 But just wanted to make it all clear to you. 25 00:01:14 --> 00:01:15 So here we are. 26 00:01:15 --> 00:01:19 This is our last day of the second unit, Applications 27 00:01:19 --> 00:01:22 of Differentiation. 28 00:01:22 --> 00:01:30 And I have one of the most fun topics to introduce to you. 29 00:01:30 --> 00:01:32 Which is differential equations. 30 00:01:32 --> 00:01:35 Now, we have a whole course on differential equations, 31 00:01:35 --> 00:01:38 which is called 18.03. 32 00:01:38 --> 00:01:43 And so we're only going to do just a little bit. 33 00:01:43 --> 00:01:52 But I'm going to teach you one technique. 34 00:01:52 --> 00:01:58 Which fits in precisely with what we've been doing already. 35 00:01:58 --> 00:02:05 Which is differentials. 36 00:02:05 --> 00:02:13 The first and simplest kind of differential equation dy/dx 37 00:02:13 --> 00:02:16 = some function, f (x). 38 00:02:16 --> 00:02:19 Now, that's a perfectly good differential equation. 39 00:02:19 --> 00:02:25 And we already discussed last time that the solution; that 40 00:02:25 --> 00:02:27 is, the function y, is going to be the antiderivative, 41 00:02:27 --> 00:02:33 or the integral, of x. 42 00:02:33 --> 00:02:36 Now, for the purposes of today, we're going to consider 43 00:02:36 --> 00:02:40 this problem to be solved. 44 00:02:40 --> 00:02:41 That is, you can always do this. 45 00:02:41 --> 00:02:44 You can always take antiderivatives. 46 00:02:44 --> 00:02:52 And for our purposes now, that is for now, we only have one 47 00:02:52 --> 00:03:08 technique to find antiderivatives. 48 00:03:08 --> 00:03:15 And that's called substitution. 49 00:03:15 --> 00:03:20 It has a very small variant, which we called 50 00:03:20 --> 00:03:27 advanced guessing. 51 00:03:27 --> 00:03:29 And that works just as well. 52 00:03:29 --> 00:03:32 And that's basically all that you'll ever need to do. 53 00:03:32 --> 00:03:35 As a practical matter, these are the ones 54 00:03:35 --> 00:03:36 you'll face for now. 55 00:03:36 --> 00:03:38 Ones that you can actually see what the answer is, or you'll 56 00:03:38 --> 00:03:42 have to make a substitution. 57 00:03:42 --> 00:03:48 Now, the first tricky example, or the first maybe interesting 58 00:03:48 --> 00:03:50 example of a differential equation, which I'll call 59 00:03:50 --> 00:04:07 Example 2, is going to be the following. (d / dx + x)y = 0. 60 00:04:07 --> 00:04:10 So that's our first differential equation that 61 00:04:10 --> 00:04:12 were going to try to solve. 62 00:04:12 --> 00:04:18 Apart from this standard antiderivative approach. 63 00:04:18 --> 00:04:24 This operation here has a name. 64 00:04:24 --> 00:04:26 This actually has a name, it's called the 65 00:04:26 --> 00:04:33 annihilation operator. 66 00:04:33 --> 00:04:43 And it's called that in quantum mechanics. 67 00:04:43 --> 00:04:46 And there's a corresponding creation operator where you 68 00:04:46 --> 00:04:50 change the sign from plus to minus. 69 00:04:50 --> 00:04:53 And this is one of the simplest differential equations. 70 00:04:53 --> 00:04:56 The reason why it's studied in quantum mechanics all it that 71 00:04:56 --> 00:05:00 it has very simple solutions that you can just write out. 72 00:05:00 --> 00:05:02 So we're going to solve this equation. 73 00:05:02 --> 00:05:06 It's the one that governs the ground state of the 74 00:05:06 --> 00:05:08 harmonic oscillator. 75 00:05:08 --> 00:05:11 So it has a lot of fancy words associated with it, but it's a 76 00:05:11 --> 00:05:13 fairly simple differential equation and it works 77 00:05:13 --> 00:05:17 perfectly by the method that we're going to propose. 78 00:05:17 --> 00:05:23 So the first step in this solution is just to rewrite the 79 00:05:23 --> 00:05:29 equation by putting one of the terms on the right-hand side. 80 00:05:29 --> 00:05:35 So this is dy / dx = - x y. 81 00:05:35 --> 00:05:38 Now, here is where you see the difference between this type of 82 00:05:38 --> 00:05:41 equation and the previous type. 83 00:05:41 --> 00:05:44 In the previous equation, we just had a function of x 84 00:05:44 --> 00:05:45 on the right-hand side. 85 00:05:45 --> 00:05:50 But here, the rate of change depends on both x and y. 86 00:05:50 --> 00:05:52 So it's not clear at all that we can solve this 87 00:05:52 --> 00:05:55 kind of equation. 88 00:05:55 --> 00:05:58 But there is a remarkable trick which works very 89 00:05:58 --> 00:05:59 well in this case. 90 00:05:59 --> 00:06:02 Which is to use multiplication. 91 00:06:02 --> 00:06:04 To use this idea of differential that we 92 00:06:04 --> 00:06:06 talked about last time. 93 00:06:06 --> 00:06:14 Namely, we divide by y and multiply by dx. 94 00:06:14 --> 00:06:17 So now we've separated the equation. 95 00:06:17 --> 00:06:20 We've separated out the differentials. 96 00:06:20 --> 00:06:23 And what's going to be important for us is that the 97 00:06:23 --> 00:06:27 left-hand side is expressed solely in terms of y and the 98 00:06:27 --> 00:06:30 right-hand side is expressed solely in terms of x. 99 00:06:30 --> 00:06:33 And we'll go through this in careful detail. 100 00:06:33 --> 00:06:36 So now, the idea is if you've set up the equation in terms of 101 00:06:36 --> 00:06:40 differentials as opposed to ratios of differentials, or 102 00:06:40 --> 00:06:44 rates of change, now I can use Leibniz's notation and 103 00:06:44 --> 00:06:47 integrate these differentials. 104 00:06:47 --> 00:06:55 Take their antiderivatives. 105 00:06:55 --> 00:07:02 And we know what each of these is. 106 00:07:02 --> 00:07:17 Namely, the left-hand side is just - ah. well, that's tough. 107 00:07:17 --> 00:07:24 OK. 108 00:07:24 --> 00:07:29 I had an au pair who actually did a lot of Tae Kwan Do. 109 00:07:29 --> 00:07:31 She could definitely defeat any of you in any 110 00:07:31 --> 00:07:35 encounter, I promise. 111 00:07:35 --> 00:07:35 OK. 112 00:07:35 --> 00:07:37 Anyway. 113 00:07:37 --> 00:07:38 So, let's go back. 114 00:07:38 --> 00:07:41 We want to take the antiderivative of this. 115 00:07:41 --> 00:07:48 So remember, this is the function whose 116 00:07:48 --> 00:07:50 derivative is 1 / y. 117 00:07:50 --> 00:07:52 And now there's a slight novelty here. 118 00:07:52 --> 00:07:55 Here we're differentiating the variables x, and here we're 119 00:07:55 --> 00:07:58 differentiating the variable as y. 120 00:07:58 --> 00:08:02 So the antiderivative here is ln y. 121 00:08:02 --> 00:08:07 And the antiderivative on the other side is - x^2 / 2. 122 00:08:07 --> 00:08:10 And they differ by a constant. 123 00:08:10 --> 00:08:17 So we have this relationship here. 124 00:08:17 --> 00:08:19 Now, that's almost the end of the story. 125 00:08:19 --> 00:08:23 We have to exponentiate to express y in terms of x. 126 00:08:23 --> 00:08:29 So, e ^ ln y = e ^ -x^2 / 2 + c. 127 00:08:29 --> 00:08:37 And now I can rewrite that as y = I'll write as A e ^ - 128 00:08:37 --> 00:08:43 x^2 / 2, where a = e ^c. 129 00:08:43 --> 00:08:46 And incidentally, we're just taking the case 130 00:08:46 --> 00:08:48 y positive here. 131 00:08:48 --> 00:08:51 We'll talk about what happens when y is negative 132 00:08:51 --> 00:08:55 in a few minutes. 133 00:08:55 --> 00:08:58 So here's the answer to the question, almost, except 134 00:08:58 --> 00:09:02 for this fact that I picked out y positive. 135 00:09:02 --> 00:09:11 Really, the solution is y = ae ^ - x^2 / 2. 136 00:09:11 --> 00:09:19 Any constant, a; a positive, negative, or 0. 137 00:09:19 --> 00:09:22 Any constant will do. 138 00:09:22 --> 00:09:24 And we should double-check that to make sure. 139 00:09:24 --> 00:09:32 If you take dy / d x right, that's going to be a 140 00:09:32 --> 00:09:36 d/ dx ( e^ -x ^2 / 2). 141 00:09:36 --> 00:09:40 And now by the chain rule, you can see that this is a times 142 00:09:40 --> 00:09:44 the factor of - x, that's the derivative of the exponent, 143 00:09:44 --> 00:09:48 with respect to x times the exponential. 144 00:09:48 --> 00:09:50 And now you just rearrange that. 145 00:09:50 --> 00:09:54 That's - x y. 146 00:09:54 --> 00:09:55 So it does check. 147 00:09:55 --> 00:09:57 These are solutions to the question. 148 00:09:57 --> 00:09:58 The a didn't matter. 149 00:09:58 --> 00:10:05 It didn't matter whether it was positive or negative. 150 00:10:05 --> 00:10:09 This function is known as the normal distribution, so it fits 151 00:10:09 --> 00:10:12 beautifully with a lot of probability and probabilistic 152 00:10:12 --> 00:10:15 interpretation of quantum mechanics. 153 00:10:15 --> 00:10:22 This is sort of the, where the particle is. 154 00:10:22 --> 00:10:26 So next, what I'd like to do is just go through the 155 00:10:26 --> 00:10:30 method in general and point out when it works. 156 00:10:30 --> 00:10:33 And then I'll make a few comments just to make sure 157 00:10:33 --> 00:10:37 that you understand the technicalities of dealing 158 00:10:37 --> 00:10:39 with constants and so forth. 159 00:10:39 --> 00:10:42 So, first of all, the general method of separation 160 00:10:42 --> 00:10:53 of variables. 161 00:10:53 --> 00:10:55 And here's when it works. 162 00:10:55 --> 00:10:59 It works when you're faced with a differential equation 163 00:10:59 --> 00:11:03 of the form f (x) g( y). 164 00:11:03 --> 00:11:05 That's the situation that we had. 165 00:11:05 --> 00:11:08 And I'll just illustrate that. 166 00:11:08 --> 00:11:09 Just to remind you here. 167 00:11:09 --> 00:11:11 Here's our equation. 168 00:11:11 --> 00:11:13 It's in that form. 169 00:11:13 --> 00:11:16 And the function f (x) = - x, and the function 170 00:11:16 --> 00:11:22 g( y) is just y. 171 00:11:22 --> 00:11:26 And now, the way the method works is, this separation step. 172 00:11:26 --> 00:11:30 From here to here, this is the key step. 173 00:11:30 --> 00:11:36 This is the only conceptually remarkable step, which all has 174 00:11:36 --> 00:11:39 to do with the fact that Leibniz fixed his notations up 175 00:11:39 --> 00:11:42 so that this works perfectly. 176 00:11:42 --> 00:11:48 And so that involves taking the y, so dividing by g( y), and 177 00:11:48 --> 00:11:53 multiplying by dx, it's comfortable because it feels 178 00:11:53 --> 00:11:59 like ordinary arithmetic, even though these are differentials. 179 00:11:59 --> 00:12:02 And then, we just antidifferentiate. 180 00:12:02 --> 00:12:09 So we have a function, h, which is the integral of dy/ g( 181 00:12:09 --> 00:12:13 y), and we have another function which is F. 182 00:12:13 --> 00:12:15 Note they are functions of completely different 183 00:12:15 --> 00:12:16 variables here. 184 00:12:16 --> 00:12:20 Integral of f ( x) dx. 185 00:12:20 --> 00:12:23 Now, in our example we did that. 186 00:12:23 --> 00:12:26 We carried out this antidifferentiation, and this 187 00:12:26 --> 00:12:30 function turned out to be ln y, and this function turned 188 00:12:30 --> 00:12:39 out to be - x^2 / 2. 189 00:12:39 --> 00:12:42 And then we write the relationship. 190 00:12:42 --> 00:12:46 Which is that if these are both antiderivatives of the same 191 00:12:46 --> 00:12:48 thing, then they have to differ by a constant. 192 00:12:48 --> 00:12:55 Or, in other words, H ( y) has to equal to F(x) + c. 193 00:12:55 --> 00:13:10 Where c is constant. 194 00:13:10 --> 00:13:16 Now, notice that this kind of equation is what we 195 00:13:16 --> 00:13:20 call an implicit equation. 196 00:13:20 --> 00:13:23 It's not quite a formula for y, directly. 197 00:13:23 --> 00:13:26 It defines y implicitly. 198 00:13:26 --> 00:13:29 That's that top line up here. 199 00:13:29 --> 00:13:33 That's the implicit equation. 200 00:13:33 --> 00:13:35 In order to make it an explicit equation, which is what is 201 00:13:35 --> 00:13:38 underneath, what I have to do is take the inverse. 202 00:13:38 --> 00:13:45 So I write it as y = = H -1( F ( x) + c). 203 00:13:45 --> 00:13:48 Now, in real life the calculus part is often pretty easy. 204 00:13:48 --> 00:13:52 And it can be quite messy to do the inverse operation. 205 00:13:52 --> 00:13:55 So sometimes we just leave it alone in the implicit form. 206 00:13:55 --> 00:13:58 But it's also satisfying, sometimes, to write it 207 00:13:58 --> 00:14:09 in the final form here. 208 00:14:09 --> 00:14:12 Now I've got to give you a few little pieces 209 00:14:12 --> 00:14:14 of commentary before. 210 00:14:14 --> 00:14:16 For those of you walked in a little bit late, this 211 00:14:16 --> 00:14:25 will all be on the Web. 212 00:14:25 --> 00:14:31 So just a few pieces of commentary. 213 00:14:31 --> 00:14:36 So if you like, some remarks. 214 00:14:36 --> 00:14:51 The first remark is that I could have written ln 215 00:14:51 --> 00:14:58 | y| = - x ^2 / 2 + c. 216 00:14:58 --> 00:15:02 We learned last time that the antiderivative works also 217 00:15:02 --> 00:15:02 for the negative values. 218 00:15:02 --> 00:15:08 So this would work for y not equal to 0. 219 00:15:08 --> 00:15:10 Both for positive and negative values. 220 00:15:10 --> 00:15:14 And you can see that that would have captured most of the 221 00:15:14 --> 00:15:15 rest of the solution. 222 00:15:15 --> 00:15:22 Namely, | y| would be = A e ^ - x^2 / 2, by the same 223 00:15:22 --> 00:15:24 reasoning as before. 224 00:15:24 --> 00:15:30 And then that would mean that y = plus or minus A e^ - x^2 / 225 00:15:30 --> 00:15:34 2, which is really just what we got. 226 00:15:34 --> 00:15:38 Because, in fact, I didn't bother with this. 227 00:15:38 --> 00:15:40 Because actually in most - and the reason why going through 228 00:15:40 --> 00:15:43 this, by the way, carefully this time, is that you're going 229 00:15:43 --> 00:15:44 to be faced with this very frequently. 230 00:15:44 --> 00:15:47 The exponential function comes up all the time. 231 00:15:47 --> 00:15:49 And so, therefore, you want to be completely comfortable 232 00:15:49 --> 00:15:52 dealing with it. 233 00:15:52 --> 00:15:55 So this time I had the positive a, while the negative a fits in 234 00:15:55 --> 00:15:57 either this way, or I can throw it in. 235 00:15:57 --> 00:15:59 Because I know that that's going to work that way. 236 00:15:59 --> 00:16:03 But of course, I double-checked to be confident. 237 00:16:03 --> 00:16:07 Now, this still leaves out one value. 238 00:16:07 --> 00:16:11 So, this still leaves out. 239 00:16:11 --> 00:16:13 So, if you like, what I have here now is a is equal to 240 00:16:13 --> 00:16:15 plus or minus capital A. 241 00:16:15 --> 00:16:18 The capital A1 being positive 1. 242 00:16:18 --> 00:16:20 But this still leaves out one case. 243 00:16:20 --> 00:16:23 Which is y = 0. 244 00:16:23 --> 00:16:27 Which is an extremely boring solution, but nevertheless a 245 00:16:27 --> 00:16:28 solution to this problem. 246 00:16:28 --> 00:16:32 If you plug in 0 here for y, you get 0. 247 00:16:32 --> 00:16:34 If you plug in 0 here for y, you get that these 248 00:16:34 --> 00:16:36 two sides are equal. 249 00:16:36 --> 00:16:38 0 = 0. 250 00:16:38 --> 00:16:40 Not a very interesting answer to the question. 251 00:16:40 --> 00:16:42 But it's still an answer. 252 00:16:42 --> 00:16:43 And so y = 0 is left out.. 253 00:16:43 --> 00:16:52 Well, that's not so surprising that we missed that solution. 254 00:16:52 --> 00:16:55 Because in the process of carrying out these 255 00:16:55 --> 00:16:58 operations, I divided by y. 256 00:16:58 --> 00:17:02 I did that right here. 257 00:17:02 --> 00:17:03 So, that's what happens. 258 00:17:03 --> 00:17:06 If you're going to do various non-linear operations; in 259 00:17:06 --> 00:17:08 particular, if you're going to divide by something, if it 260 00:17:08 --> 00:17:10 happens to be 0 you're going to miss that solution. 261 00:17:10 --> 00:17:13 You might have problems with that solution. 262 00:17:13 --> 00:17:16 But we have to live with that because we want to get ahead. 263 00:17:16 --> 00:17:20 And we want to get the formulas for various solutions. 264 00:17:20 --> 00:17:22 So that's the first remark that I wanted to make. 265 00:17:22 --> 00:17:30 And now, the second one is almost related to what I was 266 00:17:30 --> 00:17:33 just discussing right here. 267 00:17:33 --> 00:17:37 That I'm erasing. 268 00:17:37 --> 00:17:39 And that's the following. 269 00:17:39 --> 00:17:52 I could have also written ln y + c1 = - x^2 / 2 + c2. 270 00:17:52 --> 00:17:54 Where c1 and c2 are different constants. 271 00:17:54 --> 00:17:57 When I'm faced with this antidifferentiation, I just 272 00:17:57 --> 00:18:00 taught you last time, that you want to have an 273 00:18:00 --> 00:18:02 arbitrary constant. 274 00:18:02 --> 00:18:06 Here and there, in both slots. 275 00:18:06 --> 00:18:09 So I perfectly well could have written this down. 276 00:18:09 --> 00:18:14 But notice that I can rewrite this as ln y = 277 00:18:14 --> 00:18:20 - x ^2 / 2 + c2 - c1. 278 00:18:20 --> 00:18:22 I can subtract. 279 00:18:22 --> 00:18:25 And then, if I just combine these two guys together and 280 00:18:25 --> 00:18:29 name them c, I have a different constant. 281 00:18:29 --> 00:18:32 In other words, it's superfluous and redundant to 282 00:18:32 --> 00:18:35 have two arbitrary constants here, because they can always 283 00:18:35 --> 00:18:38 be combined into one. 284 00:18:38 --> 00:18:47 So two constants are superfluous. 285 00:18:47 --> 00:18:54 Can always be combined. 286 00:18:54 --> 00:18:56 So we just never do it this first way. 287 00:18:56 --> 00:19:05 It's just extra writing, it's a waste of time. 288 00:19:05 --> 00:19:07 There's one other subtle remark, which you won't 289 00:19:07 --> 00:19:10 actually appreciate until you've done several problems 290 00:19:10 --> 00:19:11 in this direction. 291 00:19:11 --> 00:19:17 Which is that the constant appears additive here, in this 292 00:19:17 --> 00:19:18 first solution to the problem. 293 00:19:18 --> 00:19:22 But when I do this nonlinear operation of exponentiation, 294 00:19:22 --> 00:19:26 it now becomes multiplicative constant. 295 00:19:26 --> 00:19:31 And so, in general, there's a free constant somewhere 296 00:19:31 --> 00:19:31 in the problem. 297 00:19:31 --> 00:19:35 But it's not always an additive constant. 298 00:19:35 --> 00:19:38 It's only an additive constant right at the first step when 299 00:19:38 --> 00:19:39 you take the antiderivative. 300 00:19:39 --> 00:19:41 And then after that, when you do all your other nonlinear 301 00:19:41 --> 00:19:45 operations, it can turn into anything at all. 302 00:19:45 --> 00:19:47 So you should always expect it to be something slightly more 303 00:19:47 --> 00:19:49 interesting than an additive constant. 304 00:19:49 --> 00:19:59 Although occasionally it stays an additive constant. 305 00:19:59 --> 00:20:01 The last little bit of commentary that I want to 306 00:20:01 --> 00:20:06 make just goes back to the original problem here. 307 00:20:06 --> 00:20:09 Which is right here. 308 00:20:09 --> 00:20:11 The example 1. 309 00:20:11 --> 00:20:14 And I want to solve it, even though this is simpleminded. 310 00:20:14 --> 00:20:21 But example 1 via separation. 311 00:20:21 --> 00:20:25 So that you see our variables. 312 00:20:25 --> 00:20:28 So that you see what it does. 313 00:20:28 --> 00:20:34 The situation is this. 314 00:20:34 --> 00:20:36 And the separation just means you put the dx 315 00:20:36 --> 00:20:38 on the other side. 316 00:20:38 --> 00:20:44 So this is dy = = f(x) dx. 317 00:20:44 --> 00:20:54 And then we integrate. 318 00:20:54 --> 00:20:58 And the antiderivative of dy is just y. 319 00:20:58 --> 00:21:03 So this is the solution to the problem. 320 00:21:03 --> 00:21:05 And it's just what we wrote before; it's 321 00:21:05 --> 00:21:07 just a funny notation. 322 00:21:07 --> 00:21:19 And it comes to the same thing as the antiderivative. 323 00:21:19 --> 00:21:23 OK, so now we're going to go on to a trickier problem. 324 00:21:23 --> 00:21:24 A trickier example. 325 00:21:24 --> 00:21:26 We need one or two more just to get some practice 326 00:21:26 --> 00:21:29 with this method. 327 00:21:29 --> 00:21:31 Everybody happy so far? 328 00:21:31 --> 00:21:32 Question. 329 00:21:32 --> 00:21:53 STUDENT: [INAUDIBLE] 330 00:21:53 --> 00:21:55 PROFESSOR: So, the question is, how do we deal 331 00:21:55 --> 00:21:58 with this ambiguity. 332 00:21:58 --> 00:22:03 I'm summarizing very, very, briefly what I heard. 333 00:22:03 --> 00:22:05 Well, you know, sometimes a > 0, sometimes a < 334 00:22:05 --> 00:22:07 0, sometimes it's not. 335 00:22:07 --> 00:22:12 So there's a name for this guy. 336 00:22:12 --> 00:22:20 Which is that this is what's called the general solution. 337 00:22:20 --> 00:22:22 In other words, the whole family of solutions is the 338 00:22:22 --> 00:22:24 answer to the question. 339 00:22:24 --> 00:22:28 Now, it could be that you're given extra information. 340 00:22:28 --> 00:22:31 If you're given extra information, that might be, and 341 00:22:31 --> 00:22:34 this is very typical in such problems, you have the rate of 342 00:22:34 --> 00:22:36 change of the function, which is what we've given. 343 00:22:36 --> 00:22:39 But you might also have the place where it starts. 344 00:22:39 --> 00:22:44 Which would be, say, it starts at 3. 345 00:22:44 --> 00:22:46 Now, if you have that extra piece of information, then 346 00:22:46 --> 00:22:50 you can nail down exactly which function it is. 347 00:22:50 --> 00:22:54 If you do that, if you plug in 3, you see that 348 00:22:54 --> 00:22:57 ae ^ - 0^2 / 2 = 3. 349 00:22:57 --> 00:23:00 So a = 3. 350 00:23:00 --> 00:23:06 And the answer is y = 3e ^ -x^2 / 2. 351 00:23:06 --> 00:23:08 And similarly, if it's negative, if it starts out 352 00:23:08 --> 00:23:10 negative, it'll stay negative. 353 00:23:10 --> 00:23:11 For instance. 354 00:23:11 --> 00:23:14 If it starts out 0, it'll stay 0 this particular 355 00:23:14 --> 00:23:16 function here. 356 00:23:16 --> 00:23:18 So the answer to your question is how you deal 357 00:23:18 --> 00:23:19 with the ambiguity. 358 00:23:19 --> 00:23:23 The answer is that you simply say what the solution is. 359 00:23:23 --> 00:23:25 And the solution is not one function, it's a 360 00:23:25 --> 00:23:26 family of functions. 361 00:23:26 --> 00:23:28 It's a list and you have to have what's known 362 00:23:28 --> 00:23:30 as a parameter. 363 00:23:30 --> 00:23:33 And that parameter gets nailed down if you tell me more 364 00:23:33 --> 00:23:35 information about the function. 365 00:23:35 --> 00:23:37 Not the rate of change, but something about the 366 00:23:37 --> 00:23:38 values of the function. 367 00:23:38 --> 00:23:46 368 00:23:46 --> 00:23:53 STUDENT: [INAUDIBLE] 369 00:23:53 --> 00:23:55 PROFESSOR: The general solution is this solution. 370 00:23:55 --> 00:23:56 STUDENT: [INAUDIBLE] 371 00:23:56 --> 00:23:59 PROFESSOR: And I'm showing you here that you could get to 372 00:23:59 --> 00:24:00 most of the general solution. 373 00:24:00 --> 00:24:04 There's one thing that's left out, namely the case a = 0. 374 00:24:04 --> 00:24:08 So, in other words, I would not go through this method. 375 00:24:08 --> 00:24:10 I would only use this, which is simpler. 376 00:24:10 --> 00:24:13 But then I have to understand that I haven't gotten all 377 00:24:13 --> 00:24:15 of the solutions this way. 378 00:24:15 --> 00:24:19 I'm going to need to throw in all the rest of the solutions. 379 00:24:19 --> 00:24:21 So in the back of your head, you always have to have 380 00:24:21 --> 00:24:23 something like this in mind. 381 00:24:23 --> 00:24:25 So that you can generate all the solutions. 382 00:24:25 --> 00:24:28 This is very suggestive, right? 383 00:24:28 --> 00:24:31 The restriction, it turns that the restriction A > 0 is 384 00:24:31 --> 00:24:40 superfluous, is unnecessary. 385 00:24:40 --> 00:24:42 But that, we only get by further thought 386 00:24:42 --> 00:24:46 and by checking. 387 00:24:46 --> 00:24:46 Another question? 388 00:24:46 --> 00:24:47 Over here. 389 00:24:47 --> 00:24:52 STUDENT: [INAUDIBLE] 390 00:24:52 --> 00:24:54 PROFESSOR: The aim of differential equations 391 00:24:54 --> 00:24:55 is to solve them. 392 00:24:55 --> 00:24:59 Just as with algebraic equations. 393 00:24:59 --> 00:25:01 Usually, differential equations are telling you something 394 00:25:01 --> 00:25:05 about the balance between an acceleration and a velocity. 395 00:25:05 --> 00:25:09 If you have a falling object, it might have a resistance. 396 00:25:09 --> 00:25:11 It's telling you something. 397 00:25:11 --> 00:25:14 So, actually, sometimes in applied problems, formulating 398 00:25:14 --> 00:25:16 what differential equation describe this situation 399 00:25:16 --> 00:25:18 is very important. 400 00:25:18 --> 00:25:22 In order to see that that's the right thing, you have to have 401 00:25:22 --> 00:25:25 solved it to see that it fits the data that you're getting. 402 00:25:25 --> 00:25:28 STUDENT: [INAUDIBLE] 403 00:25:28 --> 00:25:31 PROFESSOR: The question is, can you solve for x instead of y. 404 00:25:31 --> 00:25:36 The answer is, sure. 405 00:25:36 --> 00:25:39 That's the same thing as - so that would be the inverse 406 00:25:39 --> 00:25:42 function of the function that we're officially looking for. 407 00:25:42 --> 00:25:43 But yeah, it's legal. 408 00:25:43 --> 00:25:46 In other words, oftentimes we're stuck with just the 409 00:25:46 --> 00:25:49 implicit, some implicit formula and sometimes we're stuck with 410 00:25:49 --> 00:25:54 a formula x is a function of y versus y as a function of x. 411 00:25:54 --> 00:25:58 The way in which the function is specified is something 412 00:25:58 --> 00:26:00 that can be complicated. 413 00:26:00 --> 00:26:04 As you'll see in the next example, it's not necessarily 414 00:26:04 --> 00:26:07 the best thing to think about a function, y as a function of x. 415 00:26:07 --> 00:26:12 Well, in the fourth example. 416 00:26:12 --> 00:26:27 Alright, we're going to go on and do our next example here. 417 00:26:27 --> 00:26:32 So the third example is going to be taken as a 418 00:26:32 --> 00:26:36 kind of geometry problem. 419 00:26:36 --> 00:26:38 I'll draw a picture of it. 420 00:26:38 --> 00:26:44 Suppose you have a curve with the following property. 421 00:26:44 --> 00:26:50 If you take a point on the curve, and you take the ray, 422 00:26:50 --> 00:26:55 you take the ray from the origin to the curve, well, 423 00:26:55 --> 00:26:57 that's not going to be one that I want. 424 00:26:57 --> 00:27:00 I think I'm going to want something which is steeper. 425 00:27:00 --> 00:27:02 Because what I'm going to insist is that the tangent 426 00:27:02 --> 00:27:10 line be twice as steep as the ray from the origin. 427 00:27:10 --> 00:27:22 So, in other words, slope of tangent line equals twice 428 00:27:22 --> 00:27:31 slope of ray from origin. 429 00:27:31 --> 00:27:34 So the slope of this orange line is twice the slope 430 00:27:34 --> 00:27:39 of the pink line. 431 00:27:39 --> 00:27:41 Now, these kinds of geometric problems can be written 432 00:27:41 --> 00:27:48 very succinctly with differential equations. 433 00:27:48 --> 00:27:52 Namely, it's just the following. dy / dx, that's the 434 00:27:52 --> 00:27:56 slope of the tangent line, is equal to, well remember what 435 00:27:56 --> 00:28:00 the slope of this ray is, if this point, I need a notation. 436 00:28:00 --> 00:28:04 At this point is (x, y) which is a point on the curve. 437 00:28:04 --> 00:28:07 So the slope of this pink line is what? 438 00:28:07 --> 00:28:09 STUDENT: [INAUDIBLE] 439 00:28:09 --> 00:28:12 PROFESSOR: y / x. 440 00:28:12 --> 00:28:20 So if it's twice it, there's the equation. 441 00:28:20 --> 00:28:25 OK, now, we only have one method for solving 442 00:28:25 --> 00:28:28 these equations. 443 00:28:28 --> 00:28:29 So let's use it. 444 00:28:29 --> 00:28:31 It says to separate variables. 445 00:28:31 --> 00:28:41 So I write dy / y here = 2 dx / x. 446 00:28:41 --> 00:28:42 That's the basic separation. 447 00:28:42 --> 00:28:47 That's the procedure that we're always going to use. 448 00:28:47 --> 00:28:58 And now if I integrate that, I find that on the right-hand 449 00:28:58 --> 00:29:03 side I have the logarithm of y. 450 00:29:03 --> 00:29:06 And - sorry, on the left-hand side I have the logarithm of y. 451 00:29:06 --> 00:29:10 On the right-hand side, I have twice the logarithm 452 00:29:10 --> 00:29:20 of x, plus a constant. 453 00:29:20 --> 00:29:27 So let's see what happens to this example. 454 00:29:27 --> 00:29:30 This is an implicit equation, and of course we have the 455 00:29:30 --> 00:29:32 problems of the plus or minus signs, which I'm not going 456 00:29:32 --> 00:29:38 to worry about until later. 457 00:29:38 --> 00:29:40 So let's exponentiate and see what happens. 458 00:29:40 --> 00:29:47 We get e ^ ln y = e ^ 2 ln x + c. 459 00:29:47 --> 00:29:51 So, again, this is y on the left-hand side. 460 00:29:51 --> 00:29:54 And on the right-hand side, if you think about it for a 461 00:29:54 --> 00:29:58 second, it's (e ^ ln x)^2. 462 00:29:59 --> 00:30:00 Which is x^2. 463 00:30:00 --> 00:30:02 So this is x ^2, and then there's an e^ c. 464 00:30:02 --> 00:30:06 So that's another one of these A factors here. 465 00:30:06 --> 00:30:13 A = e^ c. 466 00:30:13 --> 00:30:20 So the answer is, well, I'll draw the picture. 467 00:30:20 --> 00:30:22 And I'm going to cheat as I did before. 468 00:30:22 --> 00:30:24 We skipped the case y negative. 469 00:30:24 --> 00:30:30 We really only did the case y positive, so far. 470 00:30:30 --> 00:30:32 But if you think about it for a second, and we'll check it in 471 00:30:32 --> 00:30:36 a second, you're going to get all of these parabolas here. 472 00:30:36 --> 00:30:40 So the solution is this family of functions. 473 00:30:40 --> 00:30:44 And they can be bending down. 474 00:30:44 --> 00:30:45 As well as up. 475 00:30:45 --> 00:30:48 So these are the solutions to this equation. 476 00:30:48 --> 00:30:50 Every single one of these curves has the property that if 477 00:30:50 --> 00:30:53 you pick a point on it, the tangent line has twice the 478 00:30:53 --> 00:30:58 slope of the ray to the origin. 479 00:30:58 --> 00:31:01 And the formula, if you like, of the general solution is y 480 00:31:01 --> 00:31:08 = ax^2, a is any constant. 481 00:31:08 --> 00:31:09 Question? 482 00:31:09 --> 00:31:21 STUDENT: [INAUDIBLE] 483 00:31:21 --> 00:31:22 PROFESSOR: Yeah. 484 00:31:22 --> 00:31:29 So again - so first of all, so there are two 485 00:31:29 --> 00:31:30 approaches to this. 486 00:31:30 --> 00:31:32 One is to check it, and make sure that it's right. 487 00:31:32 --> 00:31:35 When a formula works for some family of values, sometimes 488 00:31:35 --> 00:31:36 it works for others. 489 00:31:36 --> 00:31:39 But another one is to realize that these things will 490 00:31:39 --> 00:31:40 usually work out this way. 491 00:31:40 --> 00:31:45 Because in this argument here, I allow the absolute value. 492 00:31:45 --> 00:31:47 And that would have been a perfectly legal 493 00:31:47 --> 00:31:47 thing for me to do. 494 00:31:47 --> 00:31:51 I could have put in absolute values here. 495 00:31:51 --> 00:31:55 In which case, I would've gotten that the absolute value 496 00:31:55 --> 00:31:56 of this was equal to that. 497 00:31:56 --> 00:32:02 And now you see I've covered the plus and minus cases. 498 00:32:02 --> 00:32:03 So it's that same idea. 499 00:32:03 --> 00:32:11 This implies that y = either + A x^2 or - Ax^, depending 500 00:32:11 --> 00:32:14 on which sign you pick. 501 00:32:14 --> 00:32:21 So that allows me for the curves above and curves below. 502 00:32:21 --> 00:32:24 Because it's really true that the antiderivative 503 00:32:24 --> 00:32:26 here is the function. 504 00:32:26 --> 00:32:28 It's defined for y negative. 505 00:32:28 --> 00:32:33 So let's just double-check. 506 00:32:33 --> 00:32:39 In this case, what's happening, we have y = ax^2 and we want to 507 00:32:39 --> 00:32:44 compute dy / dx to make sure that it satisfies the equation 508 00:32:44 --> 00:32:46 that I started out with. 509 00:32:46 --> 00:32:50 And what I see here is that this is 2ax. 510 00:32:50 --> 00:32:53 And now I'm going to write this in a suggestive way. 511 00:32:53 --> 00:33:00 I'm going to write it as 2ax^2 / x. 512 00:33:00 --> 00:33:06 And, sure enough, this is 2y / x. 513 00:33:06 --> 00:33:14 It does not matter whether a, it works for a positive, 514 00:33:14 --> 00:33:17 a negative, a = 0. 515 00:33:17 --> 00:33:24 It's OK. 516 00:33:24 --> 00:33:29 Again, we didn't pick up by this method the a = 0 case. 517 00:33:29 --> 00:33:35 And that's not surprising because we divided by y. 518 00:33:35 --> 00:33:39 There's another thing to watch out about, about this example. 519 00:33:39 --> 00:33:41 So there's another warning. 520 00:33:41 --> 00:33:44 Which I have to give you. 521 00:33:44 --> 00:33:48 And this is a subtlety which you definitely won't get to in 522 00:33:48 --> 00:33:52 any detail until you get to a higher level ordinary 523 00:33:52 --> 00:33:54 differential equations course, but I do want to warn 524 00:33:54 --> 00:33:56 you about it right now. 525 00:33:56 --> 00:34:06 Which is that if you look at the equation, you need to 526 00:34:06 --> 00:34:14 watch out that it's undefined at x = 0. 527 00:34:14 --> 00:34:15 It's undefined at x = 0. 528 00:34:15 --> 00:34:20 We also divided by x, and x is also a problem. 529 00:34:20 --> 00:34:24 Now, that actually has an important consequence. 530 00:34:24 --> 00:34:27 Which is that, strangely, knowing the value here and 531 00:34:27 --> 00:34:31 knowing the rate of change doesn't specify this function. 532 00:34:31 --> 00:34:33 This is bad. 533 00:34:33 --> 00:34:36 And it violates one of our pieces of intuition. 534 00:34:36 --> 00:34:38 And what's going wrong is that the rate of change 535 00:34:38 --> 00:34:40 was not specified. 536 00:34:40 --> 00:34:43 It's undefined at x = 0. 537 00:34:43 --> 00:34:46 So there's a problem here, and in fact if you think carefully 538 00:34:46 --> 00:34:49 about what this function is doing, it could come in on 539 00:34:49 --> 00:34:56 one branch and leave on a completely different branch. 540 00:34:56 --> 00:35:01 It doesn't really have to obey any rule across x = 0. 541 00:35:01 --> 00:35:03 So you should really be thinking of these things as 542 00:35:03 --> 00:35:05 rays emanating from the origin. 543 00:35:05 --> 00:35:10 The origin was a special point in the whole geometric problem. 544 00:35:10 --> 00:35:15 Rather than as being complete parabolas. 545 00:35:15 --> 00:35:16 But that's a very subtle point. 546 00:35:16 --> 00:35:23 I don't expect you to be able to say anything about it. 547 00:35:23 --> 00:35:26 But I just want to warn you that it really is true that 548 00:35:26 --> 00:35:33 when x = 0 there's a problem for this differential equation. 549 00:35:33 --> 00:35:46 So now, let me say our next problem. 550 00:35:46 --> 00:35:47 Next example. 551 00:35:47 --> 00:35:52 Just another geometry question. 552 00:35:52 --> 00:36:01 So here's Example 4. 553 00:36:01 --> 00:36:04 I'm just going to use the example that we've already got. 554 00:36:04 --> 00:36:09 Because there's only so much time left here. 555 00:36:09 --> 00:36:23 The fourth example is to take the curves perpendicular 556 00:36:23 --> 00:36:31 to the parabolas. 557 00:36:31 --> 00:36:33 This is another geometry problem. 558 00:36:33 --> 00:36:35 And by specifying that the the curves are perpendicular to 559 00:36:35 --> 00:36:44 these parabolas, I'm telling you what their slope is. 560 00:36:44 --> 00:36:47 So let's think about that. 561 00:36:47 --> 00:36:48 What's the new equation? 562 00:36:48 --> 00:36:56 The new diff. eq. is the following. 563 00:36:56 --> 00:37:01 It's that the slope is equal to the negative reciprocal of the 564 00:37:01 --> 00:37:05 slope of the tangent line. 565 00:37:05 --> 00:37:14 Of tangent to the parabola. 566 00:37:14 --> 00:37:16 So that's the equation. 567 00:37:16 --> 00:37:19 That's actually fairly easy to write down, because 568 00:37:19 --> 00:37:26 it's - 1 / 2(y / x). 569 00:37:26 --> 00:37:32 That's the slope of the parabola. 570 00:37:32 --> 00:37:36 2y / x. 571 00:37:36 --> 00:37:38 So let's rewrite that. 572 00:37:38 --> 00:37:52 Now, this is the x goes in the numerator, so it's - x / 2y. 573 00:37:52 --> 00:37:57 And now I want to solve this one. 574 00:37:57 --> 00:38:01 Well, again, there's only one technique. 575 00:38:01 --> 00:38:10 Which is we're going to separate variables. 576 00:38:10 --> 00:38:12 And we separate the differentials here, so 577 00:38:12 --> 00:38:18 we get 2y dy = - x dx. 578 00:38:18 --> 00:38:20 That's just looking at the equation that I have, which is 579 00:38:20 --> 00:38:26 right over here. dy / dx = - x / 2y, and cross-multiplying 580 00:38:26 --> 00:38:30 to get this. 581 00:38:30 --> 00:38:33 And now I can take the antiderivative. 582 00:38:33 --> 00:38:33 This is y^2. 583 00:38:35 --> 00:38:40 And the antiderivative over here is - x^2 / 2 + c. 584 00:38:40 --> 00:38:44 585 00:38:44 --> 00:38:57 And so, the solutions are x^2 / 2 + y^2 = some c. 586 00:38:57 --> 00:39:02 Some constant c. 587 00:39:02 --> 00:39:06 Now, this time, things don't work the same. 588 00:39:06 --> 00:39:09 And you can't expect them always to work the same. 589 00:39:09 --> 00:39:11 I claimed that this must be true. 590 00:39:11 --> 00:39:16 But unfortunately I cannot insist that every c will work. 591 00:39:16 --> 00:39:19 As you can see here, only the positive numbers 592 00:39:19 --> 00:39:24 c can work here. 593 00:39:24 --> 00:39:28 So the picture is that something slightly 594 00:39:28 --> 00:39:29 different happened here. 595 00:39:29 --> 00:39:31 And you have to live with this. 596 00:39:31 --> 00:39:33 Is that sometimes not all the constants will work. 597 00:39:33 --> 00:39:36 Because there's more to the problem than just 598 00:39:36 --> 00:39:37 the antidifferentiation. 599 00:39:37 --> 00:39:40 And here there are fewer answers rather 600 00:39:40 --> 00:39:40 than more answers. 601 00:39:40 --> 00:39:43 In the other case we had to add in some answers, here 602 00:39:43 --> 00:39:45 we have to take them away. 603 00:39:45 --> 00:39:46 Some of them don't make any sense. 604 00:39:46 --> 00:39:49 And the only ones we can get are the ones which are of this 605 00:39:49 --> 00:39:54 form, where this is, say, some radius squared. 606 00:39:54 --> 00:39:55 Well maybe I shouldn't call it a radius. 607 00:39:55 --> 00:39:56 I'll just call it a parameter, a^2. 608 00:39:58 --> 00:40:05 And these are of course ellipses. 609 00:40:05 --> 00:40:11 And you can see that the ellipses, the length here is 610 00:40:11 --> 00:40:16 the square root of 2a and the semi-axis, vertical 611 00:40:16 --> 00:40:18 semi-axis, is a. 612 00:40:18 --> 00:40:20 So this is the kind of ellipse that we've got. 613 00:40:20 --> 00:40:24 And I draw it on the previous diagram, I think it's 614 00:40:24 --> 00:40:28 somewhat suggestive here. 615 00:40:28 --> 00:40:30 There, ellipses are kind of eggs. 616 00:40:30 --> 00:40:32 They're a little bit longer than they are high. 617 00:40:32 --> 00:40:37 And they go like this. 618 00:40:37 --> 00:40:41 And if I drew them pretty much right, they should 619 00:40:41 --> 00:40:43 be making right angles. 620 00:40:43 --> 00:40:49 At all of these places. 621 00:40:49 --> 00:40:53 OK, last little bit here. 622 00:40:53 --> 00:40:57 Again, you've got to be very careful with these solutions. 623 00:40:57 --> 00:41:06 And so there's a warning here too. 624 00:41:06 --> 00:41:10 So let's take a look at, this is the implicit solution 625 00:41:10 --> 00:41:10 to the equation. 626 00:41:10 --> 00:41:13 And this is the one that tells us what the shape is. 627 00:41:13 --> 00:41:16 But we can also have the explicit solution. 628 00:41:16 --> 00:41:20 And if I solve for the explicit solution, it's either y = + 629 00:41:20 --> 00:41:27 square root of a^2 - x^2 / 2, or y = - square root 630 00:41:27 --> 00:41:32 of a^2 - x^2 / 2. 631 00:41:32 --> 00:41:39 These are the explicit solutions. 632 00:41:39 --> 00:41:41 And now, we notice something that we should have 633 00:41:41 --> 00:41:43 noticed before. 634 00:41:43 --> 00:41:50 Which is that an ellipse is not a function. 635 00:41:50 --> 00:41:55 It's only the top half, if you like, that's giving you a 636 00:41:55 --> 00:41:56 solution to this equation. 637 00:41:56 --> 00:41:58 Or maybe the bottom half that's giving it the 638 00:41:58 --> 00:42:00 solution to the equation. 639 00:42:00 --> 00:42:07 So the one over here, this one is the top halves. 640 00:42:07 --> 00:42:15 And this one over here is the bottom halves. 641 00:42:15 --> 00:42:18 And there's something else that's interesting. 642 00:42:18 --> 00:42:31 Which is that we have a problem at y = 0. y = 0 is where 643 00:42:31 --> 00:42:32 x = square root of 2a. 644 00:42:33 --> 00:42:35 That's when we get to this end here. 645 00:42:35 --> 00:42:37 And what happens is the solution comes 646 00:42:37 --> 00:42:38 around and it stops. 647 00:42:38 --> 00:42:44 It has a vertical slope. 648 00:42:44 --> 00:42:48 Vertical slope. 649 00:42:48 --> 00:42:56 And the solution stops. 650 00:42:56 --> 00:43:00 But really, that's not so unreasonable. 651 00:43:00 --> 00:43:01 After all, look at the formula. 652 00:43:01 --> 00:43:03 There was a y in the denominator here. 653 00:43:03 --> 00:43:08 When y = 0, the slope should be infinite. 654 00:43:08 --> 00:43:12 And so this equation is just giving us what it 655 00:43:12 --> 00:43:15 geometrically and intuitively should be giving us. 656 00:43:15 --> 00:43:22 At that stage. 657 00:43:22 --> 00:43:25 So that is the introduction to ordinary 658 00:43:25 --> 00:43:26 differential equations. 659 00:43:26 --> 00:43:30 Again, there's only one technique which is - we're not 660 00:43:30 --> 00:43:33 done yet, we have a whole four minutes left and we're 661 00:43:33 --> 00:43:34 going to review. 662 00:43:34 --> 00:43:39 Now, so fortunately, this review is very short. 663 00:43:39 --> 00:43:43 Fortunately for you, I handed out to you exactly what you're 664 00:43:43 --> 00:43:44 going to be covering on the test. 665 00:43:44 --> 00:43:48 And it's what's printed here but there's a whole two 666 00:43:48 --> 00:43:51 pages of discussion. 667 00:43:51 --> 00:43:59 And I want to give you very, very clear-cut 668 00:43:59 --> 00:44:00 instructions here. 669 00:44:00 --> 00:44:04 This is usually the hardest test of this course. 670 00:44:04 --> 00:44:07 People usually do terribly on it. 671 00:44:07 --> 00:44:13 And I'm going to try to stop that by making it 672 00:44:13 --> 00:44:14 a little bit easier. 673 00:44:14 --> 00:44:17 And now here's what we're going to do. 674 00:44:17 --> 00:44:21 I'm telling you exactly what type of problems are 675 00:44:21 --> 00:44:22 going to be on the test. 676 00:44:22 --> 00:44:23 These are these six. 677 00:44:23 --> 00:44:25 It's also written on your sheet, your handout. 678 00:44:25 --> 00:44:29 It's also just what was asked on last year's test. 679 00:44:29 --> 00:44:31 You should go and you should look at last year's test 680 00:44:31 --> 00:44:33 and see what types of problems they are. 681 00:44:33 --> 00:44:36 I really, really, am going to ask the same questions, or 682 00:44:36 --> 00:44:38 the same type of questions. 683 00:44:38 --> 00:44:41 Not the same questions. 684 00:44:41 --> 00:44:44 So that's what's going to happen on the test. 685 00:44:44 --> 00:44:49 And let me just tell you, say one thing, which is the 686 00:44:49 --> 00:44:51 main theme of the class. 687 00:44:51 --> 00:44:52 And I will open up. 688 00:44:52 --> 00:44:54 We'll have time for one question after that. 689 00:44:54 --> 00:44:58 The main theme of this unit is simply the following. 690 00:44:58 --> 00:45:06 That information about derivative and sometimes maybe 691 00:45:06 --> 00:45:17 the second derivative, tells us information about f itself. 692 00:45:17 --> 00:45:19 And that's just what were doing here with ordinary 693 00:45:19 --> 00:45:20 differential equations. 694 00:45:20 --> 00:45:22 And that was what we were doing way at the beginning when 695 00:45:22 --> 00:45:24 we did approximations. 696 00:45:24 --> 00:45:24