1 00:00:00,300 --> 00:00:01,185 Holograms. 2 00:00:01,185 --> 00:00:07,680 [SOUND]. 3 00:00:07,680 --> 00:00:10,010 They tell me that if you take a total little bit of a 4 00:00:10,010 --> 00:00:15,100 hologram and you look through it, you can still see the whole picture. 5 00:00:15,100 --> 00:00:17,110 The same is sort of true of analytic functions. 6 00:00:17,110 --> 00:00:19,270 All right? Let's think about sine. 7 00:00:19,270 --> 00:00:23,910 So here, I've got the graph of a function, y equals f of x. 8 00:00:23,910 --> 00:00:27,990 And in this case, the function that I'm graphing is just sine. 9 00:00:27,990 --> 00:00:29,930 I'm going to think about this graph a little bit 10 00:00:29,930 --> 00:00:33,030 and just focus on this region right around the origin. 11 00:00:33,030 --> 00:00:37,170 All right, imagine, if you will, that I've taken. 12 00:00:37,170 --> 00:00:40,120 Away all of the graph and I'm just looking 13 00:00:40,120 --> 00:00:43,660 at just this little tiny piece right around the origin. 14 00:00:43,660 --> 00:00:48,350 What can I figure out about sine just by looking right around the origin. 15 00:00:48,350 --> 00:00:49,920 Well, if I look around the origin, I can 16 00:00:49,920 --> 00:00:51,850 figure out the value of sine at the origin. 17 00:00:51,850 --> 00:00:53,590 If I'm just looking the origin I can 18 00:00:53,590 --> 00:00:56,380 figure out the derivative of sine at the origin. 19 00:00:56,380 --> 00:00:58,110 I can figure out the second derivative sine at 20 00:00:58,110 --> 00:00:58,640 the origin. 21 00:00:58,640 --> 00:01:00,600 I can figure out the third derivative of sine. 22 00:01:00,600 --> 00:01:03,290 Just by looking at this little tiny piece of the graph. 23 00:01:03,290 --> 00:01:05,890 I can figure out all of the derivatives of sine, just 24 00:01:05,890 --> 00:01:08,620 by looking at this little tiny piece of the graph of sine. 25 00:01:08,620 --> 00:01:13,430 And if I can calculate all the derivatives of sine, that means that just by looking 26 00:01:13,430 --> 00:01:19,230 at that piece, I can write down the Taylor series for sine at 0. 27 00:01:19,230 --> 00:01:21,040 And we've already seen that the Taylor 28 00:01:21,040 --> 00:01:24,710 series for sine converges to sine everywhere. 29 00:01:24,710 --> 00:01:25,810 That's exactly right. 30 00:01:25,810 --> 00:01:31,940 We've seen that sine of x is equal to its Taylor series for all values of x. 31 00:01:31,940 --> 00:01:34,740 And what that means is that just this little tiny piece of 32 00:01:34,740 --> 00:01:40,490 sine, just around the origin, manages to encode the entire story about sine. 33 00:01:40,490 --> 00:01:43,300 All of the values of sine can be recovered just 34 00:01:43,300 --> 00:01:46,150 by knowing a little tiny piece of sine around the origin. 35 00:01:46,150 --> 00:01:49,720 Because that's enough to calculate all the derivatives at 0 which 36 00:01:49,720 --> 00:01:53,870 is enough to recover the Taylor series, which recovers the entire function. 37 00:01:53,870 --> 00:01:57,510 Contrast that with something involving absolute value. 38 00:01:57,510 --> 00:02:01,370 Well, here's the graph. Of a function, so y=f(x). 39 00:02:01,370 --> 00:02:07,521 But in this case, the function is f(x)=|x-1|-1. 40 00:02:07,521 --> 00:02:11,600 Now, what happens if I zoom in on the origin? 41 00:02:11,600 --> 00:02:14,830 Well, this little piece of the graph just around the origin is enough to 42 00:02:14,830 --> 00:02:17,040 calculate some facts about f, right? 43 00:02:17,040 --> 00:02:19,450 What can I calculate just by looking right around the origin? 44 00:02:19,450 --> 00:02:23,716 Well I can calculate the value of this function is 0 when I plug in 45 00:02:23,716 --> 00:02:29,040 0, I can calculate that the derivative of this function is negative 1 at 0. 46 00:02:29,040 --> 00:02:32,550 And I can calculate that all of the higher derivatives, all of the 47 00:02:32,550 --> 00:02:36,580 second, third, fourth and so on derivatives at 0 are equal to 0. 48 00:02:36,580 --> 00:02:40,230 So yeah, this thing looks like a straight line around here and 49 00:02:40,230 --> 00:02:43,140 that infinitesimal information at the point 0. 50 00:02:43,140 --> 00:02:45,890 Just the derivatives at the point 0 are enough to 51 00:02:45,890 --> 00:02:51,590 recover the function around 0 on a whole interval around 0. 52 00:02:51,590 --> 00:02:53,376 Now of course, I might have been tricked into 53 00:02:53,376 --> 00:02:56,970 thinking that the entire function just looked like this, right. 54 00:02:56,970 --> 00:02:59,610 I can't tell that there's this point where the function 55 00:02:59,610 --> 00:03:02,740 fails to be differentiable, just when I'm looking over here. 56 00:03:02,740 --> 00:03:05,380 But nevertheless, just this infinitesimal information 57 00:03:05,380 --> 00:03:08,660 at a point, is still enough to recover some information 58 00:03:08,660 --> 00:03:12,390 about the function in a whole interval, around that point. 59 00:03:12,390 --> 00:03:15,240 Real analytic functions are really quite surprising. 60 00:03:15,240 --> 00:03:17,550 Infinitesimal information, just at a point, is 61 00:03:17,550 --> 00:03:19,640 giving you information at a whole interval. 62 00:03:20,800 --> 00:03:23,310 Sine, cosine, and e to the x are even better. 63 00:03:23,310 --> 00:03:28,050 In that case, the Taylor series converges to those functions everywhere. 64 00:03:28,050 --> 00:03:30,800 Which means infinitesimal information at a single 65 00:03:30,800 --> 00:03:34,410 point, on say the graph of sine, alright, a single point on the graph 66 00:03:34,410 --> 00:03:37,660 of cosine, or at a single point on the graph of e to the x. 67 00:03:37,660 --> 00:03:42,830 That information is telling you everything about the entire function. 68 00:03:42,830 --> 00:03:45,830 Yeah en, en, entire is actually the word that, that's used. 69 00:03:45,830 --> 00:03:51,660 Entire describes functions like sin where just the infinitesimal information at a 70 00:03:51,660 --> 00:03:56,700 point is enough to recover a power series with an infinite radius of convergence. 71 00:03:56,700 --> 00:04:00,170 Converges everywhere to the entire function. 72 00:04:00,170 --> 00:04:02,040 So, it's really like a hologram. 73 00:04:02,040 --> 00:04:02,270 Alright? 74 00:04:02,270 --> 00:04:05,674 Just a little tiny bit of a hologram records everything 75 00:04:05,674 --> 00:04:08,335 in the scene and so too would say sine of x. 76 00:04:08,335 --> 00:04:08,443 Alright? 77 00:04:08,443 --> 00:04:13,736 Just a little tiny piece of sine reveals everything about the function. 78 00:04:13,736 --> 00:04:22,891 [SOUND] 79 00:04:22,891 --> 00:04:24,440 [BLANK_AUDIO]