1 00:00:00,090 --> 00:00:02,430 The following content is provided under a Creative 2 00:00:02,430 --> 00:00:03,820 Commons license. 3 00:00:03,820 --> 00:00:06,030 Your support will help MIT OpenCourseWare 4 00:00:06,030 --> 00:00:10,120 continue to offer high-quality educational resources for free. 5 00:00:10,120 --> 00:00:12,690 To make a donation, or to view additional materials 6 00:00:12,690 --> 00:00:16,620 from hundreds of MIT courses, visit MIT OpenCourseWare 7 00:00:16,620 --> 00:00:17,550 at ocw.mit.edu. 8 00:00:22,420 --> 00:00:24,830 GEORGE BARBASTATHIS: Hi, everyone. 9 00:00:24,830 --> 00:00:31,940 OK, Yeah, so let me tell you my vision of what SMA is 10 00:00:31,940 --> 00:00:34,290 and what we're supposed to do. 11 00:00:34,290 --> 00:00:36,540 Oh, before I do that, let me do one more introduction. 12 00:00:36,540 --> 00:00:39,940 This is Professor Colin Sheppard sitting on the other side. 13 00:00:39,940 --> 00:00:43,470 So he's the instructor on the Singapore side. 14 00:00:43,470 --> 00:00:46,430 So basically, the four of us are the team of instructors-- 15 00:00:46,430 --> 00:00:51,470 Professor Shepherd, Se Baek, Pepe, and myself. 16 00:00:51,470 --> 00:00:55,420 And the class is not quite an SMA class. 17 00:00:55,420 --> 00:00:58,790 It is not quite part of the Singapore-MIT Alliance. 18 00:00:58,790 --> 00:01:00,290 It is part of something else called 19 00:01:00,290 --> 00:01:04,819 Singapore-MIT Alliance for Research and Technology, SMART. 20 00:01:04,819 --> 00:01:09,830 And there is a very complicated description of what SMART is 21 00:01:09,830 --> 00:01:11,570 and why we're teaching the class. 22 00:01:11,570 --> 00:01:14,360 But the bottom line is that this is more or less 23 00:01:14,360 --> 00:01:17,900 the same class of optics that has been taught 24 00:01:17,900 --> 00:01:19,590 at MIT for the last 10 years. 25 00:01:19,590 --> 00:01:22,010 It's actually an improved version of the class. 26 00:01:22,010 --> 00:01:23,930 And it is being broadcast to Singapore 27 00:01:23,930 --> 00:01:26,510 at a very inconvenient time for everybody involved, 28 00:01:26,510 --> 00:01:28,500 both in Singapore and for us. 29 00:01:28,500 --> 00:01:31,610 So I think it is fair. 30 00:01:31,610 --> 00:01:35,900 And so this is a summary, a little bit of what I just 31 00:01:35,900 --> 00:01:37,780 said about the instructors. 32 00:01:37,780 --> 00:01:39,310 We also have the two assistants. 33 00:01:39,310 --> 00:01:41,900 Primarily, you'll be dealing with Kate, 34 00:01:41,900 --> 00:01:43,440 those of you who are here. 35 00:01:43,440 --> 00:01:45,080 She's my assistant at MIT. 36 00:01:45,080 --> 00:01:47,390 And for those of you in Singapore, 37 00:01:47,390 --> 00:01:49,610 if you need sometimes to turn in assignments, 38 00:01:49,610 --> 00:01:52,240 or desperately get hold of me, or whatever, 39 00:01:52,240 --> 00:01:53,430 [? Deana ?] is your contact. 40 00:01:53,430 --> 00:01:55,940 She's in block S16. 41 00:01:59,290 --> 00:02:02,660 But anyway, Singapore uses English 42 00:02:02,660 --> 00:02:04,520 as an official language, but as you 43 00:02:04,520 --> 00:02:06,050 will notice throughout the class, 44 00:02:06,050 --> 00:02:07,110 there's some differences. 45 00:02:07,110 --> 00:02:09,235 For example, in Singapore, we don't say "building." 46 00:02:09,235 --> 00:02:10,340 We say "block." 47 00:02:10,340 --> 00:02:12,950 So there's also some other subtle differences 48 00:02:12,950 --> 00:02:15,700 in Singapore English. 49 00:02:15,700 --> 00:02:20,440 OK, we will seldom give any handouts in the class. 50 00:02:20,440 --> 00:02:22,280 Everything you need is in the website. 51 00:02:22,280 --> 00:02:24,960 I have listed there link over here. 52 00:02:24,960 --> 00:02:27,820 And when you log in there, you will hit two, three things, 53 00:02:27,820 --> 00:02:28,320 actually. 54 00:02:28,320 --> 00:02:31,720 You'll see the syllabus has been posted, 55 00:02:31,720 --> 00:02:34,180 a set of policies has been posted, 56 00:02:34,180 --> 00:02:37,020 which says some obvious things like don't copy, 57 00:02:37,020 --> 00:02:39,490 don't cheat on exams, and stuff like that. 58 00:02:39,490 --> 00:02:44,372 And also, the first lecture has also been posted. 59 00:02:44,372 --> 00:02:46,830 And I will tell you a little bit about how we deal with the 60 00:02:46,830 --> 00:02:49,240 posted lectures and so on. 61 00:02:49,240 --> 00:02:52,380 And these are some administrative details here 62 00:02:52,380 --> 00:02:55,860 that I'm not sure if I want to spend any time on those. 63 00:02:55,860 --> 00:02:57,713 For those of you who are Course 2, 64 00:02:57,713 --> 00:02:59,130 if you're undergraduate, graduate, 65 00:02:59,130 --> 00:03:01,910 it meets your restricted elective requirement. 66 00:03:01,910 --> 00:03:03,480 If you're graduate, it prepares you 67 00:03:03,480 --> 00:03:08,570 for one of the qualifying exams offered in the department. 68 00:03:08,570 --> 00:03:15,270 And a little bit about what the class covers. 69 00:03:15,270 --> 00:03:16,770 So the class is very introductory 70 00:03:16,770 --> 00:03:22,990 about light phenomena and how we design optical systems. 71 00:03:22,990 --> 00:03:26,610 And so this is a bunch of pictures 72 00:03:26,610 --> 00:03:28,405 I stole from various websites. 73 00:03:28,405 --> 00:03:29,220 It shows a rainbow. 74 00:03:29,220 --> 00:03:32,880 It shows the galaxy that we can capture 75 00:03:32,880 --> 00:03:35,070 with advanced telescopes. 76 00:03:35,070 --> 00:03:38,992 It shows-- do I have a pointer? 77 00:03:38,992 --> 00:03:42,370 I'd better just use this for now. 78 00:03:42,370 --> 00:03:43,680 Well, I guess I cannot use. 79 00:03:43,680 --> 00:03:46,380 Anyway, so it shows a cell over here 80 00:03:46,380 --> 00:03:48,822 captured with a microscope-- 81 00:03:48,822 --> 00:03:50,655 which, I believe, is a confocal microscopes. 82 00:03:50,655 --> 00:03:53,590 So it is Professor Sheppard's expertise. 83 00:03:53,590 --> 00:03:57,990 And this is the picture of the esophagus of a person captured 84 00:03:57,990 --> 00:03:58,900 with an endoscopy. 85 00:03:58,900 --> 00:04:03,660 So they basically lower the fiber bundle inside, 86 00:04:03,660 --> 00:04:06,120 down someone's throat. 87 00:04:06,120 --> 00:04:09,060 And using a technique called optical coherence tomography-- 88 00:04:09,060 --> 00:04:11,310 it is an optical imaging technique-- 89 00:04:11,310 --> 00:04:15,020 they capture the esophagus. 90 00:04:15,020 --> 00:04:18,329 And so finally, what you see here 91 00:04:18,329 --> 00:04:20,250 is, of course, an optical disk, if you're not 92 00:04:20,250 --> 00:04:21,510 familiar with those. 93 00:04:21,510 --> 00:04:24,530 And over here I believe that's a holographic setup. 94 00:04:24,530 --> 00:04:27,360 It is a diffusion screen, and this 95 00:04:27,360 --> 00:04:32,010 is supposed to be a setup for a three-dimensional display. 96 00:04:32,010 --> 00:04:34,320 When you look at it, it creates the illusion 97 00:04:34,320 --> 00:04:37,410 of a three-dimensional projection. 98 00:04:37,410 --> 00:04:39,510 So if we had this, for example, in Singapore, 99 00:04:39,510 --> 00:04:41,130 then I would, in principle, appear 100 00:04:41,130 --> 00:04:42,660 as if I'm standing over there. 101 00:04:42,660 --> 00:04:45,770 This, of course, is still at the science fiction stage, 102 00:04:45,770 --> 00:04:48,340 but a lot of people are working on it. 103 00:04:48,340 --> 00:04:51,990 And in fact, nowadays, some companies, 104 00:04:51,990 --> 00:04:53,850 they offer a three dimensional television 105 00:04:53,850 --> 00:04:57,282 sets that you can buy for a small additional amount. 106 00:04:57,282 --> 00:04:58,740 I think it's a few hundred dollars. 107 00:04:58,740 --> 00:05:01,710 Samsung offers a 3D TV set. 108 00:05:01,710 --> 00:05:05,370 Anyway, so the point of this slide 109 00:05:05,370 --> 00:05:09,240 is that there's many applications of optics that 110 00:05:09,240 --> 00:05:11,430 are interesting in engineering. 111 00:05:11,430 --> 00:05:14,520 And, of course, light phenomena are 112 00:05:14,520 --> 00:05:16,630 interesting in their own right. 113 00:05:16,630 --> 00:05:22,475 So the class will try to balance curiosity-based, 114 00:05:22,475 --> 00:05:23,850 more of a science approach, where 115 00:05:23,850 --> 00:05:27,060 we learn basic facts about how light behaves, 116 00:05:27,060 --> 00:05:29,790 how it propagates, how it interacts with matter, 117 00:05:29,790 --> 00:05:32,270 and we'll balance those with engineering applications that 118 00:05:32,270 --> 00:05:36,760 are, presumably, of interest to many of you. 119 00:05:36,760 --> 00:05:39,730 And for issues that have to do with the expertise of both 120 00:05:39,730 --> 00:05:43,090 of us, both of the instructors, we 121 00:05:43,090 --> 00:05:46,400 will concentrate most of the applications on imaging. 122 00:05:46,400 --> 00:05:49,150 So we'll be dealing a lot with things like microscopes 123 00:05:49,150 --> 00:05:51,260 and telescopes primarily. 124 00:05:51,260 --> 00:05:56,500 These the major imaging instruments. 125 00:05:56,500 --> 00:05:58,630 But we'll also cover some other things for fun. 126 00:05:58,630 --> 00:06:01,060 For example, we'll talk about the human eye. 127 00:06:01,060 --> 00:06:05,510 We'll describe its structure, its biology, how it works-- 128 00:06:05,510 --> 00:06:07,510 not in great detail, because this is, after all, 129 00:06:07,510 --> 00:06:09,220 not a biology class. 130 00:06:09,220 --> 00:06:11,590 But just for fun, because of the human eye 131 00:06:11,590 --> 00:06:15,130 turns out to have some very interesting optics inside it. 132 00:06:15,130 --> 00:06:17,380 And also, we'll discuss very briefly 133 00:06:17,380 --> 00:06:20,830 the eyes of insects, which, as you can see from the picture 134 00:06:20,830 --> 00:06:23,740 and you may already know, they're very 135 00:06:23,740 --> 00:06:25,870 different than the human eye. 136 00:06:25,870 --> 00:06:28,820 And we'll discuss a little bit why they're different 137 00:06:28,820 --> 00:06:31,490 and how each one of them operates. 138 00:06:31,490 --> 00:06:33,970 And finally, some other optical imaging systems that 139 00:06:33,970 --> 00:06:35,770 look very surprising. 140 00:06:35,770 --> 00:06:38,770 This picture over here is an instrument 141 00:06:38,770 --> 00:06:41,920 called the Very Large Array telescope, or VLA. 142 00:06:41,920 --> 00:06:46,410 It is located in Socorro, New Mexico, here in the States. 143 00:06:46,410 --> 00:06:50,470 And it is composed of 27 antennas. 144 00:06:50,470 --> 00:06:53,350 Each one of these little white things is an antenna. 145 00:06:53,350 --> 00:06:58,280 It's about 27 meters tall, and the diameter of the instrument, 146 00:06:58,280 --> 00:07:01,930 this branch over here, is approximately-- 147 00:07:01,930 --> 00:07:02,740 well, it varies. 148 00:07:02,740 --> 00:07:05,080 I don't know what it was when this picture was taken. 149 00:07:05,080 --> 00:07:07,520 But it can between 3 miles-- 150 00:07:07,520 --> 00:07:11,080 the diameter that is the size of Cambridge, Massachusetts-- 151 00:07:11,080 --> 00:07:15,040 and 15 miles-- that is the size of Washington, DC. 152 00:07:15,040 --> 00:07:16,210 So that is an instrument. 153 00:07:16,210 --> 00:07:18,085 An optical instrument, if you can believe it, 154 00:07:18,085 --> 00:07:21,580 has the size of an entire state in the US. 155 00:07:21,580 --> 00:07:25,450 And it is used to observe very remote galaxies 156 00:07:25,450 --> 00:07:27,310 with high resolution. 157 00:07:27,310 --> 00:07:29,650 So it falls a little bit outside the scope of the class, 158 00:07:29,650 --> 00:07:34,690 because it uses it uses statistical optics, which 159 00:07:34,690 --> 00:07:37,390 we don't cover over here, but we may mention it 160 00:07:37,390 --> 00:07:40,720 in passing a little bit later. 161 00:07:40,720 --> 00:07:44,320 So this is, of course, among other things 162 00:07:44,320 --> 00:07:46,780 that you may have seen. 163 00:07:46,780 --> 00:07:48,730 But actually, it cannot be done. 164 00:07:48,730 --> 00:07:49,930 This is Luke Skywalker. 165 00:07:49,930 --> 00:07:52,180 I'm old enough to have been around when 166 00:07:52,180 --> 00:07:54,700 this movie came out, Star Wars. 167 00:07:54,700 --> 00:07:57,940 And I just want to point out that a lightsaber can actually 168 00:07:57,940 --> 00:07:59,020 not be made. 169 00:07:59,020 --> 00:08:00,530 It is one of these impossible things 170 00:08:00,530 --> 00:08:03,390 that you can see in science fiction, 171 00:08:03,390 --> 00:08:05,920 but it violates some physical principles. 172 00:08:05,920 --> 00:08:08,470 So unfortunately, it cannot be made, but anyway, 173 00:08:08,470 --> 00:08:13,050 it is still fun to think about. 174 00:08:13,050 --> 00:08:16,460 OK, so I think I covered the class objectives. 175 00:08:16,460 --> 00:08:20,740 And we have to balance here physical intuition 176 00:08:20,740 --> 00:08:27,080 with engineering understanding and design. 177 00:08:27,080 --> 00:08:31,300 So we'll cover the fundamentals in pretty good detail, 178 00:08:31,300 --> 00:08:33,100 and we'll also cover some applications 179 00:08:33,100 --> 00:08:35,710 in pretty good detail to the degree that we can 180 00:08:35,710 --> 00:08:38,620 within the scope of a semester. 181 00:08:38,620 --> 00:08:42,100 So we'll try to be to be very careful about that, 182 00:08:42,100 --> 00:08:43,348 how we balance the two. 183 00:08:43,348 --> 00:08:44,890 Sometimes the two can compete, right? 184 00:08:44,890 --> 00:08:47,140 So we'll try to balance the competition between basics 185 00:08:47,140 --> 00:08:49,870 and application. 186 00:08:49,870 --> 00:08:54,190 And also, we'll cover some applications. 187 00:08:54,190 --> 00:08:56,170 And I mentioned, primarily, we'll 188 00:08:56,170 --> 00:09:01,540 deal with microscopy and, also, some topics such as telescopes. 189 00:09:01,540 --> 00:09:03,820 There are some other topics that I will not really 190 00:09:03,820 --> 00:09:07,030 cover in class, like optical data storage. 191 00:09:07,030 --> 00:09:10,060 But as I will mention in a second, 192 00:09:10,060 --> 00:09:14,380 there is class projects that are like mini research projects 193 00:09:14,380 --> 00:09:16,850 that you will do later in the semester. 194 00:09:16,850 --> 00:09:18,640 So you're welcome to pick topics out 195 00:09:18,640 --> 00:09:21,480 of those if you are interested. 196 00:09:21,480 --> 00:09:24,810 Some basics about the sort of prerequisites. 197 00:09:24,810 --> 00:09:28,890 This is the basic math and physics that you need. 198 00:09:28,890 --> 00:09:32,640 I think most of you have covered these topics in your-- 199 00:09:32,640 --> 00:09:35,310 at least on the MIT side, you covered those in places 200 00:09:35,310 --> 00:09:40,470 like 18.03, and 2.004, and 8.02. 201 00:09:40,470 --> 00:09:44,258 So I assume that all of you who are undergraduates 202 00:09:44,258 --> 00:09:45,300 have taken those classes. 203 00:09:49,170 --> 00:09:52,370 And there is it two textbooks. 204 00:09:52,370 --> 00:09:54,790 So the class is a little bit expensive, sorry about that. 205 00:09:54,790 --> 00:09:58,170 There's two textbooks, [? Hecht ?] and Goodman. 206 00:09:58,170 --> 00:10:01,290 We'll be using, throughout the first half 207 00:10:01,290 --> 00:10:03,840 of the semester, mostly [? Hecht, ?] 208 00:10:03,840 --> 00:10:06,540 and then, throughout the second half, mostly Goodman. 209 00:10:06,540 --> 00:10:10,170 But the textbooks-- we did not really 210 00:10:10,170 --> 00:10:12,330 cover the sequence of the textbooks. 211 00:10:12,330 --> 00:10:15,810 You should use them primarily as a reference. 212 00:10:15,810 --> 00:10:18,370 All of this stuff is posted, by the way, on the website. 213 00:10:18,370 --> 00:10:23,300 So you don't need to write down the book names. 214 00:10:23,300 --> 00:10:26,570 But anyway, so the textbooks are reference. 215 00:10:26,570 --> 00:10:29,870 Your primary sources are the notes and what you do in class. 216 00:10:29,870 --> 00:10:31,880 And then you can go back and read them. 217 00:10:31,880 --> 00:10:34,550 And there some other texts that are 218 00:10:34,550 --> 00:10:37,590 useful if you have access to them through the library, 219 00:10:37,590 --> 00:10:38,728 and so on. 220 00:10:38,728 --> 00:10:40,145 Some other administrative details. 221 00:10:43,310 --> 00:10:45,830 This is the grade distribution for the undergraduate class, 222 00:10:45,830 --> 00:10:47,620 2.71-- 223 00:10:47,620 --> 00:10:50,740 30 homeworks, 30 quizzes, 40 final. 224 00:10:50,740 --> 00:10:52,360 We have eight homeworks. 225 00:10:56,700 --> 00:10:58,860 And the homeworks are due-- 226 00:10:58,860 --> 00:11:03,540 actually, they are due nine days after they're posted. 227 00:11:03,540 --> 00:11:05,970 So you have plenty of time to work on them. 228 00:11:05,970 --> 00:11:08,250 And also, Pepe will strategically 229 00:11:08,250 --> 00:11:12,780 schedule his office hours so that you can ask questions 230 00:11:12,780 --> 00:11:14,430 before the homework. 231 00:11:14,430 --> 00:11:19,600 And we'll see how to do the office hours for the Singapore 232 00:11:19,600 --> 00:11:20,100 students. 233 00:11:20,100 --> 00:11:23,800 We'll work something out when I get there. 234 00:11:23,800 --> 00:11:27,510 Anyway, the first homework is not due until February 18, 235 00:11:27,510 --> 00:11:31,410 so there's no need to panic about that yet. 236 00:11:31,410 --> 00:11:35,940 And the homeworks will also be posted on their website. 237 00:11:35,940 --> 00:11:38,610 And the 7.10 is very similar, but the 7.10, 238 00:11:38,610 --> 00:11:41,230 the graduate version, also has a project. 239 00:11:41,230 --> 00:11:44,430 So the project also counts for a significant portion 240 00:11:44,430 --> 00:11:45,095 of the grade. 241 00:11:45,095 --> 00:11:46,470 And I think I already mentioned-- 242 00:11:46,470 --> 00:11:48,678 this is like a mini research project where you either 243 00:11:48,678 --> 00:11:53,760 give a short lecture on a hot topic in current optics 244 00:11:53,760 --> 00:11:59,190 research, or you pick your own topic, 245 00:11:59,190 --> 00:12:03,150 and you do a little bit of calculation 246 00:12:03,150 --> 00:12:08,040 or some simple thinking. 247 00:12:08,040 --> 00:12:10,750 It's supposed to be a class topic. 248 00:12:10,750 --> 00:12:13,020 It's not a [INAUDIBLE] or anything, but like a mini 249 00:12:13,020 --> 00:12:14,410 research topic. 250 00:12:14,410 --> 00:12:16,950 In fact, there are a couple of people already asking me 251 00:12:16,950 --> 00:12:20,830 if they can do something related to their current research. 252 00:12:20,830 --> 00:12:23,310 And that's perfectly fine, but you have to sell it, 253 00:12:23,310 --> 00:12:25,890 because this is a team project, right? 254 00:12:25,890 --> 00:12:28,410 So if you want to do something related to you research, 255 00:12:28,410 --> 00:12:31,100 you need to recruit two, three, four, 256 00:12:31,100 --> 00:12:33,810 other colleagues from the class and form a team around it. 257 00:12:33,810 --> 00:12:34,560 So it's up to you. 258 00:12:34,560 --> 00:12:38,160 And I certainly encourage, actually, 259 00:12:38,160 --> 00:12:42,070 research-related projects in the class. 260 00:12:42,070 --> 00:12:43,860 So this is only for 710. 261 00:12:43,860 --> 00:12:47,190 If you are enrolled in 701 and would like to be involved 262 00:12:47,190 --> 00:12:52,530 in this, you are welcome to do it, but to be fair, 263 00:12:52,530 --> 00:12:54,060 you cannot get credit. 264 00:12:54,060 --> 00:12:55,890 However, you can be undergraduate 265 00:12:55,890 --> 00:12:59,380 and enroll in the graduate version of the class. 266 00:12:59,380 --> 00:13:01,680 So for example, if you are planning 267 00:13:01,680 --> 00:13:04,440 to stay on at MIT for graduate school, 268 00:13:04,440 --> 00:13:06,660 that's not a bad idea, because the class is H-level, 269 00:13:06,660 --> 00:13:10,470 so it will already count you towards some of your credits 270 00:13:10,470 --> 00:13:11,280 later. 271 00:13:11,280 --> 00:13:14,225 So anyway, that's something that we can discuss separately, 272 00:13:14,225 --> 00:13:16,610 if you like. 273 00:13:16,610 --> 00:13:19,538 And finally, the ugly side, we do have quizzes, and exams, 274 00:13:19,538 --> 00:13:20,330 and all this stuff. 275 00:13:20,330 --> 00:13:21,350 I hate them myself. 276 00:13:21,350 --> 00:13:22,790 I hated them when I was a student. 277 00:13:22,790 --> 00:13:24,710 But it's a little bit like the dentist, right? 278 00:13:24,710 --> 00:13:27,920 In You hate it, but you have to do it. 279 00:13:27,920 --> 00:13:32,030 So this is the distribution of the quizzes and the final. 280 00:13:34,610 --> 00:13:37,790 One important thing I would like to emphasize, which is, 281 00:13:37,790 --> 00:13:41,120 I always deliver a small sermon when I start a class, 282 00:13:41,120 --> 00:13:44,720 and that has to do with asking the question. 283 00:13:44,720 --> 00:13:48,590 I really think that you get the most benefit not from listening 284 00:13:48,590 --> 00:13:52,610 to me while I lecture, especially at 7:00 AM, 285 00:13:52,610 --> 00:13:55,507 you know, when, including me, you're all sleepy. 286 00:13:55,507 --> 00:13:57,132 And I will be sleepy in Singapore, too, 287 00:13:57,132 --> 00:13:58,460 because it's going to be late. 288 00:13:58,460 --> 00:14:00,710 Anyway, so you don't get the most benefit out of that. 289 00:14:00,710 --> 00:14:03,470 You don't get the most benefit by reading your book alone 290 00:14:03,470 --> 00:14:07,010 at home in your bed and so on. 291 00:14:07,010 --> 00:14:08,840 The most benefit you get is actually 292 00:14:08,840 --> 00:14:12,800 from participating in discussions in the classroom-- 293 00:14:12,800 --> 00:14:19,310 with your peers, with the instructors, everybody. 294 00:14:19,310 --> 00:14:23,330 So I would like to encourage you to not hesitate for any reason 295 00:14:23,330 --> 00:14:24,700 whatsoever. 296 00:14:24,700 --> 00:14:26,540 If there's something that bothers you, 297 00:14:26,540 --> 00:14:29,060 some question, something you're not understanding, 298 00:14:29,060 --> 00:14:34,280 something you're uncertain, or whatever, please do ask. 299 00:14:34,280 --> 00:14:39,050 There's no reason to be shy. 300 00:14:39,050 --> 00:14:45,017 Very often people-- myself included-- 301 00:14:45,017 --> 00:14:47,100 if you're in a big audience, you may be reluctant. 302 00:14:47,100 --> 00:14:51,090 Because you say well, gee, what if my question is not good, 303 00:14:51,090 --> 00:14:53,460 or what if I embarrass myself? 304 00:14:53,460 --> 00:14:55,620 So there is no such thing, OK? 305 00:14:55,620 --> 00:14:58,710 If a question pops up in your mind, 306 00:14:58,710 --> 00:15:01,890 the probability is very high that someone else in the class 307 00:15:01,890 --> 00:15:03,880 has the exact same question. 308 00:15:03,880 --> 00:15:06,960 And this person is equally shy as you 309 00:15:06,960 --> 00:15:08,700 are to ask that question. 310 00:15:08,700 --> 00:15:10,350 So you do yourself a favor, and you 311 00:15:10,350 --> 00:15:12,780 do many of your other classmates a favor, 312 00:15:12,780 --> 00:15:16,620 if you just interrupt me and ask a question so please do that. 313 00:15:16,620 --> 00:15:21,090 And also, on my side, I will treat all questions equally, 314 00:15:21,090 --> 00:15:24,450 and I will do my best to answer every possible question. 315 00:15:24,450 --> 00:15:26,460 Sometimes I might not answer a question 316 00:15:26,460 --> 00:15:27,910 if I don't know the answer myself. 317 00:15:27,910 --> 00:15:29,640 This happens very often in my classes 318 00:15:29,640 --> 00:15:31,530 and, I think, in everybody's classes. 319 00:15:31,530 --> 00:15:34,012 Always, someone can come up with a question 320 00:15:34,012 --> 00:15:35,220 that I don't know the answer. 321 00:15:35,220 --> 00:15:38,280 If that happens I'll tell you, sorry, I'll get back to you 322 00:15:38,280 --> 00:15:40,530 in the next lecture, right? 323 00:15:40,530 --> 00:15:44,640 Anyway I think, it will take a few lectures. 324 00:15:44,640 --> 00:15:48,110 Usually, in my classes, it takes a few lectures for the students 325 00:15:48,110 --> 00:15:49,618 to overcome the threshold. 326 00:15:49,618 --> 00:15:51,660 But I think it becomes very productive, actually, 327 00:15:51,660 --> 00:15:54,670 when you engage in discussions in the class. 328 00:15:54,670 --> 00:15:57,660 And yeah, don't worry about falling behind 329 00:15:57,660 --> 00:15:59,160 on the syllabus or anything. 330 00:15:59,160 --> 00:16:01,980 It is much more important that we learn well what 331 00:16:01,980 --> 00:16:05,320 we do learn than that we cover a lot of material 332 00:16:05,320 --> 00:16:08,100 and, in the end, nothing has been left in your minds. 333 00:16:08,100 --> 00:16:10,320 So one of the benefit of discussions, especially 334 00:16:10,320 --> 00:16:12,940 arguments, if we get into an argument about something, 335 00:16:12,940 --> 00:16:15,180 then everybody will remember, right? 336 00:16:15,180 --> 00:16:18,210 Because it's kind of fun to watch people argue a topic. 337 00:16:18,210 --> 00:16:22,950 So yeah, by all means, please interrupt and ask. 338 00:16:22,950 --> 00:16:26,040 And we don't have recitations, but as you noticed, 339 00:16:26,040 --> 00:16:28,800 the class has a slightly unusual schedule. 340 00:16:28,800 --> 00:16:30,840 You have a two-hour lecture on Wednesday 341 00:16:30,840 --> 00:16:32,910 and one hour on Monday. 342 00:16:32,910 --> 00:16:36,510 So we'll structure the syllabus so that most of the material 343 00:16:36,510 --> 00:16:41,190 is covered on Wednesday and most of the examples, and practice, 344 00:16:41,190 --> 00:16:44,460 and so on, they happen on Mondays. 345 00:16:44,460 --> 00:16:47,790 So this is how we deal with the recitation issue. 346 00:16:47,790 --> 00:16:50,250 And, of course, there's also the office hours. 347 00:16:50,250 --> 00:17:00,050 And-- oh, yeah, and sometimes, we 348 00:17:00,050 --> 00:17:02,930 cover some mathematical topics that some of you 349 00:17:02,930 --> 00:17:07,790 may have forgotten or may not be very up to speed with, 350 00:17:07,790 --> 00:17:09,770 especially Fourier transforms. 351 00:17:09,770 --> 00:17:15,310 So when the time comes, we might do a special lecture 352 00:17:15,310 --> 00:17:17,790 in the evening, MIT time. 353 00:17:17,790 --> 00:17:19,700 And if we need to do that in Singapore, 354 00:17:19,700 --> 00:17:22,210 we'll do it, actually, individually with me, 355 00:17:22,210 --> 00:17:24,290 sort of in my office or something like that. 356 00:17:24,290 --> 00:17:25,790 Those of you at MIT, you'll probably 357 00:17:25,790 --> 00:17:30,680 do it with Se Baek or Pepe, come back one evening after 7:00 PM, 358 00:17:30,680 --> 00:17:35,578 so we obey Institute policies, and do a math review. 359 00:17:35,578 --> 00:17:37,620 So this may happen once or twice in the semester, 360 00:17:37,620 --> 00:17:39,980 especially when it comes to Fourier transforms. 361 00:17:39,980 --> 00:17:43,700 Because my experience. 362 00:17:43,700 --> 00:17:46,100 You need the logistics of Fourier 363 00:17:46,100 --> 00:17:49,010 transforms in order to follow a significant fraction 364 00:17:49,010 --> 00:17:50,190 of the class. 365 00:17:50,190 --> 00:17:55,750 So if you are not really up to speed with your basic Fourier 366 00:17:55,750 --> 00:18:01,480 from wherever you learned things 18.03 or 2.671, and so on, 367 00:18:01,480 --> 00:18:02,550 we'll do that for you. 368 00:18:05,200 --> 00:18:11,150 OK, this is a list of topics that we'll cover in the class. 369 00:18:11,150 --> 00:18:12,970 You can browse them in the website. 370 00:18:12,970 --> 00:18:15,590 I will not go through each topic now, 371 00:18:15,590 --> 00:18:18,640 because I don't want to give it away. 372 00:18:18,640 --> 00:18:22,060 I want to leave an element of surprise. 373 00:18:22,060 --> 00:18:25,270 But basically, the class is divided into geometrical optics 374 00:18:25,270 --> 00:18:27,250 and wave optics. 375 00:18:27,250 --> 00:18:32,570 And we'll start with geometrical optics for about four weeks, 376 00:18:32,570 --> 00:18:35,270 and then we'll move to wave optics. 377 00:18:35,270 --> 00:18:38,050 So the difference, it really has to do with approximations 378 00:18:38,050 --> 00:18:42,703 of when we deal with light phenomena, 379 00:18:42,703 --> 00:18:44,120 it's actually very complicated how 380 00:18:44,120 --> 00:18:47,000 light interacts with matter, and how it propagates, and so. 381 00:18:47,000 --> 00:18:49,640 It is really a horrendous problem. 382 00:18:49,640 --> 00:18:51,950 But over the years-- over the centuries, 383 00:18:51,950 --> 00:18:55,030 actually-- people have come up with different approximations 384 00:18:55,030 --> 00:18:56,800 of progressive accuracy. 385 00:18:56,800 --> 00:18:59,330 So geometrical optics is the simplest approximation 386 00:18:59,330 --> 00:19:03,170 that gives you very simple formulas, very simple math, 387 00:19:03,170 --> 00:19:07,280 and actually describes light quite well up to a point. 388 00:19:07,280 --> 00:19:09,710 So we'll do that first, and then we'll 389 00:19:09,710 --> 00:19:13,160 graduate to wave optics, which is a little bit more 390 00:19:13,160 --> 00:19:15,800 involved mathematically, but it also 391 00:19:15,800 --> 00:19:21,380 gives better approximations about the propagation of light. 392 00:19:21,380 --> 00:19:24,750 And then, finally, in the very last few-- 393 00:19:24,750 --> 00:19:27,590 probably in the last lecture, and only if we have time-- 394 00:19:27,590 --> 00:19:31,070 we'll cover a topic called sub-wavelength optics, which is 395 00:19:31,070 --> 00:19:32,510 an even better approximation. 396 00:19:32,510 --> 00:19:37,790 But that is actually pretty much impossible to do analytically. 397 00:19:37,790 --> 00:19:39,890 So one has to go onto a computer and do 398 00:19:39,890 --> 00:19:44,090 numerical solution of a nasty set of coupled differential 399 00:19:44,090 --> 00:19:45,000 equations. 400 00:19:45,000 --> 00:19:48,230 So we'll do that not in the computational way, 401 00:19:48,230 --> 00:19:50,840 but we'll cover some of the related phenomena 402 00:19:50,840 --> 00:19:54,170 and what this approximation gives. 403 00:19:54,170 --> 00:19:57,650 But roughly, anyway, the class is structured according 404 00:19:57,650 --> 00:20:01,490 to these approximations. 405 00:20:01,490 --> 00:20:03,020 Any questions so far? 406 00:20:14,700 --> 00:20:17,910 And if think of a question, you can also interrupt me, right? 407 00:20:17,910 --> 00:20:18,998 You're always welcome. 408 00:20:18,998 --> 00:20:20,040 Well, and one more thing. 409 00:20:20,040 --> 00:20:22,560 Yes, I'll tell you the one more thing, perhaps, later. 410 00:20:26,810 --> 00:20:29,798 Let me start with a little bit of history. 411 00:20:29,798 --> 00:20:31,840 This, of course, is not the subject of the class, 412 00:20:31,840 --> 00:20:33,790 but it's kind of fun to do. 413 00:20:33,790 --> 00:20:37,320 I used to start my classes with a joke that not everybody got. 414 00:20:37,320 --> 00:20:40,090 I used to start by saying that optics 415 00:20:40,090 --> 00:20:41,800 is the most ancient science. 416 00:20:41,800 --> 00:20:43,240 Not the most ancient profession-- 417 00:20:43,240 --> 00:20:44,480 that's something else-- 418 00:20:44,480 --> 00:20:45,820 but is the most ancient science. 419 00:20:48,830 --> 00:20:52,420 And I think the reason is because humans 420 00:20:52,420 --> 00:20:55,330 are very visual animals. 421 00:20:55,330 --> 00:21:00,160 Our vision, for those of us who are lucky enough to have it, 422 00:21:00,160 --> 00:21:03,460 our vision is one of them most dominant census. 423 00:21:03,460 --> 00:21:07,240 So people got interested in phenomena involving light 424 00:21:07,240 --> 00:21:11,440 relatively early on in the early ages. 425 00:21:11,440 --> 00:21:13,870 And this probably happened across civilizations-- 426 00:21:13,870 --> 00:21:19,340 Chinese, Egyptian, Western Greek, and so on. 427 00:21:19,340 --> 00:21:22,960 But as it happens, the Greeks were the only ones to publish. 428 00:21:22,960 --> 00:21:25,510 They were open about what they were discovering. 429 00:21:25,510 --> 00:21:28,060 The Egyptians and the Chinese, the priests 430 00:21:28,060 --> 00:21:30,690 kept everything under control. 431 00:21:30,690 --> 00:21:32,440 So we don't know much about what they did. 432 00:21:32,440 --> 00:21:35,560 But from what we've discovered, archaeologists 433 00:21:35,560 --> 00:21:38,710 have discovered in ancient tombs and so on, they also 434 00:21:38,710 --> 00:21:39,940 knew quite a bit about light. 435 00:21:43,630 --> 00:21:46,300 Of course, the Greeks made the major mistake-- 436 00:21:46,300 --> 00:21:49,570 so Greek science was very interesting 437 00:21:49,570 --> 00:21:52,730 because it was the flip side of modern science. 438 00:21:52,730 --> 00:22:01,570 The Greeks had the attitude that you can understand nature 439 00:22:01,570 --> 00:22:03,970 just by thinking. 440 00:22:03,970 --> 00:22:07,950 So the Greeks actually discouraged experiment. 441 00:22:07,950 --> 00:22:12,450 Strangely enough, this tradition has followed the Greek psyche, 442 00:22:12,450 --> 00:22:13,950 because if you look at the faculty 443 00:22:13,950 --> 00:22:16,110 in the mechanical engineering department, 444 00:22:16,110 --> 00:22:21,030 there's a lot of Greeks, or professors of Greek origin, 445 00:22:21,030 --> 00:22:22,870 and lots of them are theoreticians. 446 00:22:22,870 --> 00:22:25,590 Anyway, I'm just joking. 447 00:22:25,590 --> 00:22:27,480 But anyway, the ancient Greeks, they 448 00:22:27,480 --> 00:22:30,110 have this attitude that you don't need to do experiment. 449 00:22:30,110 --> 00:22:32,070 In fact, you must not do experiment. 450 00:22:32,070 --> 00:22:36,790 You have to understand everything by thought. 451 00:22:36,790 --> 00:22:39,383 So because of that, they came up with some strange ideas. 452 00:22:39,383 --> 00:22:41,050 So for example, the Greeks, they thought 453 00:22:41,050 --> 00:22:46,210 that when you look at something, your eyes emit some substance, 454 00:22:46,210 --> 00:22:49,090 which they called simulacra. 455 00:22:49,090 --> 00:22:54,940 And this absence is their thought of what light is. 456 00:22:54,940 --> 00:22:57,610 So I look at you, I transmit a substance. 457 00:22:57,610 --> 00:23:00,610 The substance comes back to me, and that's how I see you. 458 00:23:00,610 --> 00:23:02,930 Which is, of course, a very bizarre, bizarre way 459 00:23:02,930 --> 00:23:03,430 of thinking. 460 00:23:03,430 --> 00:23:05,500 But anyway, that's what they thought. 461 00:23:05,500 --> 00:23:11,050 And it was the Arabs, much later in the 10th century or so, 462 00:23:11,050 --> 00:23:13,917 who read the Greek script. 463 00:23:13,917 --> 00:23:16,250 And they said, well, that doesn't make any sense at all. 464 00:23:16,250 --> 00:23:17,625 So the Arabs, for the first time, 465 00:23:17,625 --> 00:23:19,840 thought, well, it must be the other way around. 466 00:23:19,840 --> 00:23:23,620 There must be light sources, like the sun, or a fire, or-- 467 00:23:23,620 --> 00:23:24,900 that's about it at the time. 468 00:23:24,900 --> 00:23:28,090 They didn't have light bulbs yet. 469 00:23:28,090 --> 00:23:32,590 So it must be that they emit something that is called light, 470 00:23:32,590 --> 00:23:34,156 and that's how we see. 471 00:23:34,156 --> 00:23:36,920 So it took us about 1,000 years, I guess, 472 00:23:36,920 --> 00:23:40,520 to resolve that question. 473 00:23:40,520 --> 00:23:44,100 And also, the Arabs did a lot of the very first basic work 474 00:23:44,100 --> 00:23:44,600 in optics. 475 00:23:44,600 --> 00:23:47,810 For example, Snell's Law, the law of refraction 476 00:23:47,810 --> 00:23:50,030 that I will cover in a little bit, 477 00:23:50,030 --> 00:23:53,740 the Arabs discovered it first. 478 00:23:53,740 --> 00:23:59,470 And then, much later, another 400 years later, 479 00:23:59,470 --> 00:24:03,010 Descartes, he did two things. 480 00:24:03,010 --> 00:24:06,110 He put the basic foundations of science-- 481 00:24:06,110 --> 00:24:11,300 Descartes, you may know this, Descartes 482 00:24:11,300 --> 00:24:14,000 was the first philosopher, I should say, 483 00:24:14,000 --> 00:24:16,890 who flipped the Greek point of view. 484 00:24:16,890 --> 00:24:19,160 And he said that it's actually the other way around. 485 00:24:19,160 --> 00:24:22,070 Science must follow experiment. 486 00:24:22,070 --> 00:24:24,800 Instead of just thinking about nature and explaining it, 487 00:24:24,800 --> 00:24:26,570 he said that it's the other way around-- 488 00:24:26,570 --> 00:24:29,000 science must be driven by observation. 489 00:24:29,000 --> 00:24:32,060 So we observe something, we create experimental conditions 490 00:24:32,060 --> 00:24:36,080 to test it, and then we come up with a theory 491 00:24:36,080 --> 00:24:39,050 that tries to explain the observation-- not the other way 492 00:24:39,050 --> 00:24:39,750 around. 493 00:24:39,750 --> 00:24:46,067 And of course, modern science still follows that principle. 494 00:24:46,067 --> 00:24:47,150 At least hopefully, right? 495 00:24:47,150 --> 00:24:49,910 Because there have been occasions 496 00:24:49,910 --> 00:24:51,560 of cheating and so on. 497 00:24:51,560 --> 00:24:54,170 You probably see those in newspapers. 498 00:24:54,170 --> 00:24:56,060 I think there was a guy who invented, 499 00:24:56,060 --> 00:24:58,930 who sort of created data at HP Labs. 500 00:24:58,930 --> 00:25:01,180 Was it HP Labs? 501 00:25:01,180 --> 00:25:03,730 Anyway, so there are some people who violated principle. 502 00:25:03,730 --> 00:25:07,500 But hopefully, 99.9999% of us will actually 503 00:25:07,500 --> 00:25:08,500 follow Descartes, right? 504 00:25:08,500 --> 00:25:12,820 We make an observation, we report it faithfully, 505 00:25:12,820 --> 00:25:15,440 and then we try to explain it to the best we can 506 00:25:15,440 --> 00:25:17,020 and in the simplest way that we can. 507 00:25:17,020 --> 00:25:21,290 That's the scientific method. 508 00:25:21,290 --> 00:25:23,650 But also, Descartes, as it turns out, worked on optics. 509 00:25:23,650 --> 00:25:27,370 And he also derived Snell's Law in his own way. 510 00:25:27,370 --> 00:25:30,550 And there's something called the Descartes Sphere, which 511 00:25:30,550 --> 00:25:32,650 was invented independently by the Arabs 512 00:25:32,650 --> 00:25:35,260 in the 11th century or 12th, I forget-- 513 00:25:35,260 --> 00:25:41,050 Ninth, actually-- and then Descartes 514 00:25:41,050 --> 00:25:46,710 reinvented it about 400 or 500 years later. 515 00:25:46,710 --> 00:25:49,635 Then, the next major advance in optics came from Newton-- 516 00:25:52,530 --> 00:25:54,720 actually, Newton and Huygens, who tried to explain 517 00:25:54,720 --> 00:25:56,790 light in two different ways. 518 00:25:56,790 --> 00:25:58,650 Newton was of the opinion that light 519 00:25:58,650 --> 00:26:02,970 is a bunch of particles that travel in air. 520 00:26:02,970 --> 00:26:07,890 And he tried to explain various phenomena like refraction 521 00:26:07,890 --> 00:26:11,790 from a prism, and so on, based on this idea. 522 00:26:11,790 --> 00:26:13,830 Huygens thought that light is a wave very 523 00:26:13,830 --> 00:26:15,380 similar to water waves. 524 00:26:15,380 --> 00:26:16,690 They did not know about-- 525 00:26:16,690 --> 00:26:21,042 I believe Newton also postulated that sound is a wave. 526 00:26:21,042 --> 00:26:22,500 But for some reason, Newton thought 527 00:26:22,500 --> 00:26:24,550 that light is not a wave. 528 00:26:24,550 --> 00:26:25,950 In fact, the two of them fought. 529 00:26:25,950 --> 00:26:30,780 I don't know if the fought over it, but they disagreed over it. 530 00:26:30,780 --> 00:26:33,960 But I guess because Newton was more famous-- 531 00:26:33,960 --> 00:26:39,090 he was a professor, a Lucasian professor at Cambridge-- 532 00:26:39,090 --> 00:26:43,060 so Newton's view actually prevailed 533 00:26:43,060 --> 00:26:46,470 for several years, prevailed. 534 00:26:46,470 --> 00:26:49,080 And the particle theory of light was 535 00:26:49,080 --> 00:26:52,590 dominant until about a century later 536 00:26:52,590 --> 00:26:55,410 when people experimentally-- 537 00:26:55,410 --> 00:26:57,540 again, here comes the scientific method-- 538 00:26:57,540 --> 00:27:01,620 people experimentally observed phenomena like interference 539 00:27:01,620 --> 00:27:06,900 that would only be described if light were a wave. 540 00:27:06,900 --> 00:27:09,240 So the particle theory got a big hit then, 541 00:27:09,240 --> 00:27:13,290 because it could not explain diffraction, interference, 542 00:27:13,290 --> 00:27:14,370 and so on, and so forth. 543 00:27:14,370 --> 00:27:17,760 But yet, people were observing them in the laboratory. 544 00:27:17,760 --> 00:27:20,620 Of course, now, after one more century, people 545 00:27:20,620 --> 00:27:22,230 discovered that, guess what? 546 00:27:22,230 --> 00:27:23,790 Both theories are correct. 547 00:27:23,790 --> 00:27:26,520 With quantum mechanics, light can be thought of as 548 00:27:26,520 --> 00:27:29,490 both as particle and as a wave. 549 00:27:29,490 --> 00:27:32,640 And in fact, Einstein and some other scientists-- 550 00:27:32,640 --> 00:27:34,480 Schrodinger, Planck, and so on-- 551 00:27:34,480 --> 00:27:39,520 they reconciled the two points of view. 552 00:27:39,520 --> 00:27:41,940 Not perfectly-- there still some puzzling aspects 553 00:27:41,940 --> 00:27:44,770 of the quantum theory of light. 554 00:27:44,770 --> 00:27:46,330 But I think nowadays, most people 555 00:27:46,330 --> 00:27:48,010 are comfortable with the idea that you 556 00:27:48,010 --> 00:27:51,940 can use both approaches to describe light phenomena. 557 00:27:51,940 --> 00:27:54,340 You simply select the ones that best 558 00:27:54,340 --> 00:27:57,670 suits your approximations and your conditions 559 00:27:57,670 --> 00:27:58,970 at any given moment. 560 00:27:58,970 --> 00:28:01,420 So for example, if a particle approach 561 00:28:01,420 --> 00:28:04,730 is sufficient to describe the phenomenon, then you use it. 562 00:28:04,730 --> 00:28:07,570 And of course, there's also, typically-- or, not typically, 563 00:28:07,570 --> 00:28:09,730 always-- 564 00:28:09,730 --> 00:28:10,660 let me restate. 565 00:28:10,660 --> 00:28:15,100 There had better be an equivalent wave description 566 00:28:15,100 --> 00:28:17,620 of whatever phenomenon you're describing, 567 00:28:17,620 --> 00:28:19,320 but it may be more complicated, right? 568 00:28:19,320 --> 00:28:21,980 So in that case, you use particle theory. 569 00:28:21,980 --> 00:28:22,980 Or the other way around. 570 00:28:22,980 --> 00:28:26,410 If it is easier to describe something as a wave, 571 00:28:26,410 --> 00:28:30,513 you opt for the wave description. 572 00:28:30,513 --> 00:28:32,930 So of course, in this class, we don't cover quantum optics 573 00:28:32,930 --> 00:28:33,430 at all. 574 00:28:33,430 --> 00:28:36,050 Professor Shapiro in the electrical engineering 575 00:28:36,050 --> 00:28:39,110 department offers a class in quantum optics. 576 00:28:39,110 --> 00:28:41,630 And I suppose that there is also a quantum optics 577 00:28:41,630 --> 00:28:45,080 glass for those of you who are interested. 578 00:28:45,080 --> 00:28:46,250 It's a very elegant topic. 579 00:28:49,050 --> 00:28:54,260 So the other major advance in optics 580 00:28:54,260 --> 00:28:58,700 came in the middle of the last century, 581 00:28:58,700 --> 00:29:04,160 when the laser was invented and the technique 582 00:29:04,160 --> 00:29:07,780 called holography called holographic was invented. 583 00:29:07,780 --> 00:29:11,420 Not because holography is somehow dominant in practice. 584 00:29:11,420 --> 00:29:14,345 I mean, you see holograms typically in museums. 585 00:29:14,345 --> 00:29:15,640 It's no big deal. 586 00:29:15,640 --> 00:29:18,530 But holography turned out to be a very interesting 587 00:29:18,530 --> 00:29:21,800 mathematical way of looking at optics. 588 00:29:21,800 --> 00:29:23,510 Now, that really had a major impact 589 00:29:23,510 --> 00:29:28,520 in the subsequent development of optical science. 590 00:29:28,520 --> 00:29:30,800 So for this reason, both of these inventions 591 00:29:30,800 --> 00:29:33,260 led to Nobel prizes. 592 00:29:33,260 --> 00:29:37,320 They were very major advances in the field of light. 593 00:29:37,320 --> 00:29:43,150 And especially after the invention of the laser, 594 00:29:43,150 --> 00:29:45,460 optical science had a huge impact 595 00:29:45,460 --> 00:29:46,630 on everyday applications. 596 00:29:46,630 --> 00:29:48,070 If you think about devices you use 597 00:29:48,070 --> 00:29:52,750 in your everyday life, every time you pick up a telephone 598 00:29:52,750 --> 00:29:56,262 or you use the internet, there's typically-- especially 599 00:29:56,262 --> 00:29:58,720 if you use it long-distance-- there's some optics involved. 600 00:29:58,720 --> 00:30:03,040 Because the signals propagate through optical fibers, 601 00:30:03,040 --> 00:30:08,530 at least in part of the telecommunications network. 602 00:30:08,530 --> 00:30:10,950 If you're unlucky enough to have surgery, 603 00:30:10,950 --> 00:30:14,560 there's many kinds of laser surgery. 604 00:30:14,560 --> 00:30:17,470 Lots of clinical medical diagnosis 605 00:30:17,470 --> 00:30:19,840 is done using high-end microscopes, 606 00:30:19,840 --> 00:30:22,840 including confocal microscopes, optical coherence tomographers, 607 00:30:22,840 --> 00:30:23,920 and so on, and so forth. 608 00:30:23,920 --> 00:30:26,700 These are all commercial instruments. 609 00:30:26,700 --> 00:30:28,620 There's applications in industry-- 610 00:30:28,620 --> 00:30:32,820 for example, laser cutting, laser welding, laser metrology 611 00:30:32,820 --> 00:30:39,990 that is used in high-end precision engineering 612 00:30:39,990 --> 00:30:41,010 applications. 613 00:30:41,010 --> 00:30:44,040 And of course, finally, every time you pick up a computer, 614 00:30:44,040 --> 00:30:47,520 the chips that are all made using optical lithography, 615 00:30:47,520 --> 00:30:52,590 which is a really highly sophisticated form of optical 616 00:30:52,590 --> 00:30:53,580 imagine. 617 00:30:53,580 --> 00:30:57,000 And I use the term "optical" here in a very general way. 618 00:30:57,000 --> 00:30:58,440 Most of it is really optical. 619 00:30:58,440 --> 00:30:59,670 We use light. 620 00:30:59,670 --> 00:31:02,430 In some really extreme, high-end applications, 621 00:31:02,430 --> 00:31:04,290 they use electron lithography. 622 00:31:04,290 --> 00:31:08,940 But still electrons, behave like light when it comes to this, 623 00:31:08,940 --> 00:31:10,500 to this scale. 624 00:31:10,500 --> 00:31:14,740 So basically, the same equations that we use to describe light, 625 00:31:14,740 --> 00:31:19,050 they use them to describe imaging by electrons. 626 00:31:19,050 --> 00:31:26,930 So that is really a huge, huge, huge domain of application. 627 00:31:26,930 --> 00:31:30,450 It still remains a very active scientific field. 628 00:31:30,450 --> 00:31:32,340 So if you look at the list of Nobel Prizes-- 629 00:31:32,340 --> 00:31:36,080 this is a very incomplete list that I compiled from the Nobel 630 00:31:36,080 --> 00:31:37,970 website-- 631 00:31:37,970 --> 00:31:42,320 even that latest Nobel Prize that was awarded-- 632 00:31:42,320 --> 00:31:45,740 in chemistry, actually; it was in the field of optics-- 633 00:31:45,740 --> 00:31:49,010 these fellows, they invented something, 634 00:31:49,010 --> 00:31:53,675 green fluorescent protein, which is-- 635 00:31:53,675 --> 00:31:55,880 I may embarrass myself now, because I don't 636 00:31:55,880 --> 00:31:57,200 understand the biology of it, 637 00:31:57,200 --> 00:32:00,020 But my very simple understanding is 638 00:32:00,020 --> 00:32:03,920 that they can genetically program this protein 639 00:32:03,920 --> 00:32:07,020 to get into some animals' DNA. 640 00:32:07,020 --> 00:32:10,430 So they basically create animals that have this protein embedded 641 00:32:10,430 --> 00:32:13,340 in their genes, and then these proteins 642 00:32:13,340 --> 00:32:18,655 can also be designed to turn itself on or off depending 643 00:32:18,655 --> 00:32:19,780 on happens with the animal. 644 00:32:19,780 --> 00:32:22,610 For example, if the animal is exposed to a disease, 645 00:32:22,610 --> 00:32:25,550 or if it is exposed to a certain chemical agent, 646 00:32:25,550 --> 00:32:28,100 or anyway, whatever is of interest 647 00:32:28,100 --> 00:32:31,790 to the particular biological experiment, 648 00:32:31,790 --> 00:32:35,330 it sounds kind of funny, but the animal becomes fluorescent. 649 00:32:35,330 --> 00:32:38,330 Or more interestingly, certain parts 650 00:32:38,330 --> 00:32:40,110 of the tissue of the animal-- for example, 651 00:32:40,110 --> 00:32:44,510 the liver, or some tissue of interest-- becomes fluorescent. 652 00:32:44,510 --> 00:32:48,230 So then you can pump the animal with a laser beam, 653 00:32:48,230 --> 00:32:50,660 you can measure the fluorescence that is coming out 654 00:32:50,660 --> 00:32:52,670 of the animal's tissue, and then you 655 00:32:52,670 --> 00:32:55,940 can derive conclusions about what happened to the animal. 656 00:32:55,940 --> 00:33:00,830 So this is a fantastic way of studying genetics, studying 657 00:33:00,830 --> 00:33:05,960 diseases, studying a number of different and very important 658 00:33:05,960 --> 00:33:07,400 biological phenomena. 659 00:33:07,400 --> 00:33:08,780 So for that reason, these fellows 660 00:33:08,780 --> 00:33:11,810 were awarded the Nobel Prize. 661 00:33:11,810 --> 00:33:14,600 And actually, many people, including myself-- 662 00:33:14,600 --> 00:33:19,210 at least not yet, but I'm sure in Colin's lab, already, 663 00:33:19,210 --> 00:33:24,860 we'll use animals that are genetically 664 00:33:24,860 --> 00:33:25,940 modified with this-- 665 00:33:25,940 --> 00:33:28,700 It's called GFC, green fluorescent protein-- 666 00:33:28,700 --> 00:33:30,980 to study various biological phenomena. 667 00:33:30,980 --> 00:33:34,550 Now it is a very commonly used technique in microscopy. 668 00:33:34,550 --> 00:33:38,780 So this was the most recent optics-related Nobel Prize. 669 00:33:38,780 --> 00:33:41,810 There's a bunch of others. 670 00:33:41,810 --> 00:33:43,825 My favorite is actually-- 671 00:33:43,825 --> 00:33:44,900 where is it? 672 00:33:44,900 --> 00:33:46,430 This one. 673 00:33:46,430 --> 00:33:51,010 In 1997, this was a given for optical traps. 674 00:33:51,010 --> 00:33:52,640 So an optical trap is actually a way 675 00:33:52,640 --> 00:33:54,860 to move particles by using light. 676 00:33:54,860 --> 00:33:58,370 It's a very surprising thing, because none 677 00:33:58,370 --> 00:34:02,210 of us in everyday life will experience mechanical force 678 00:34:02,210 --> 00:34:03,680 from a light beam. 679 00:34:03,680 --> 00:34:05,027 But in actuality, there is one. 680 00:34:05,027 --> 00:34:06,860 If you are sitting in the back of the light, 681 00:34:06,860 --> 00:34:08,090 you are feeling the force. 682 00:34:08,090 --> 00:34:09,100 This once is very weak. 683 00:34:09,100 --> 00:34:11,370 It's in the range of femtonewtons, typically-- 684 00:34:11,370 --> 00:34:14,550 a really tiny, tiny force. 685 00:34:14,550 --> 00:34:18,020 But we're also very big, so the force is not enough to move us. 686 00:34:18,020 --> 00:34:20,300 But if you're really tiny-- like a cell, for example-- 687 00:34:20,300 --> 00:34:22,730 the force, especially if you design the optical right 688 00:34:22,730 --> 00:34:24,860 with a very highly focused beam, you 689 00:34:24,860 --> 00:34:26,860 can boost that force to the range 690 00:34:26,860 --> 00:34:28,770 of, perhaps, a few piconewtons. 691 00:34:28,770 --> 00:34:31,010 Not really that's a very high force, but anyway, 692 00:34:31,010 --> 00:34:32,989 in that order of magnitude, it can 693 00:34:32,989 --> 00:34:35,690 be enough to actually move a particle. 694 00:34:35,690 --> 00:34:41,520 So you can make, you can apply mechanical forces using light. 695 00:34:41,520 --> 00:34:44,719 So this was another Nobel Prize. 696 00:34:44,719 --> 00:34:48,110 So anyway, the reason I'm bringing this up 697 00:34:48,110 --> 00:34:50,270 is because this is a very exciting field. 698 00:34:50,270 --> 00:34:52,469 At least-- well, I'm partial, because I work on it, 699 00:34:52,469 --> 00:34:54,380 but it's a very exciting field. 700 00:34:54,380 --> 00:34:58,970 People come up with clever, crazy inventions all the time. 701 00:34:58,970 --> 00:35:02,810 And many, many of these inventions have-- 702 00:35:02,810 --> 00:35:05,570 usually, they have a very high impact. 703 00:35:05,570 --> 00:35:11,450 And so it is interesting to see both sides of the coin, 704 00:35:11,450 --> 00:35:13,730 both the science side of the coin 705 00:35:13,730 --> 00:35:16,820 that is purely curiosity-driven, and very often 706 00:35:16,820 --> 00:35:19,190 people in government question it, 707 00:35:19,190 --> 00:35:21,410 because they say, well, why are you guys doing 708 00:35:21,410 --> 00:35:22,940 all this crazy stuff? 709 00:35:22,940 --> 00:35:25,100 Who cares about optical forces? 710 00:35:25,100 --> 00:35:26,900 But of course, these people are so excited, 711 00:35:26,900 --> 00:35:31,310 because history shows that most of the time, 712 00:35:31,310 --> 00:35:33,650 these curiosity-driven discoveries, 713 00:35:33,650 --> 00:35:37,040 they end up having a huge impact in everyday life. 714 00:35:37,040 --> 00:35:44,540 Some crazy persons-- they were French, American, 715 00:35:44,540 --> 00:35:46,010 and Chinese-American, right? 716 00:35:46,010 --> 00:35:48,680 Three crazy persons thought about focusing 717 00:35:48,680 --> 00:35:50,180 light to move particles. 718 00:35:50,180 --> 00:35:53,030 Then, all of a sudden, this is used in biological research 719 00:35:53,030 --> 00:35:55,940 to try to understand diseases like malaria. 720 00:35:55,940 --> 00:35:58,470 I don't know if any of Professor Subra Suresh's students 721 00:35:58,470 --> 00:36:03,410 are here, but one of my colleagues, Subra Suresh, 722 00:36:03,410 --> 00:36:05,840 studied malaria using this technique that 723 00:36:05,840 --> 00:36:09,530 won the Nobel Prize in 1997. 724 00:36:09,530 --> 00:36:13,350 So it is our duty as engineers, or scientists, 725 00:36:13,350 --> 00:36:15,650 or whatever the case may be to emphasize 726 00:36:15,650 --> 00:36:17,750 to the people in government and politics 727 00:36:17,750 --> 00:36:21,450 that yes, there is value in fundamental science 728 00:36:21,450 --> 00:36:23,550 when they bash it and they say that, 729 00:36:23,550 --> 00:36:27,820 what, you guys are playing in laboratories, and so on. 730 00:36:27,820 --> 00:36:30,380 OK, so I went onto my tirade. 731 00:36:30,380 --> 00:36:34,288 And any questions? 732 00:36:38,212 --> 00:36:39,170 AUDIENCE: I've got one. 733 00:36:39,170 --> 00:36:40,212 GEORGE BARBASTATHIS: Yes. 734 00:36:40,212 --> 00:36:42,200 AUDIENCE: So I think I'm on. 735 00:36:42,200 --> 00:36:45,015 GEORGE BARBASTATHIS: Yes, can you hear him? 736 00:36:45,015 --> 00:36:45,560 OK. 737 00:36:45,560 --> 00:36:47,185 AUDIENCE: It says that you can describe 738 00:36:47,185 --> 00:36:50,640 how an electron beam images in a similar way as optics. 739 00:36:50,640 --> 00:36:52,500 But electrons interact with matter. 740 00:36:52,500 --> 00:36:54,428 So how does light interact with matter? 741 00:36:54,428 --> 00:36:55,470 GEORGE BARBASTATHIS: Yes. 742 00:36:55,470 --> 00:36:56,490 So we will cover that. 743 00:36:56,490 --> 00:36:59,880 Of course, they interact in very different ways, right? 744 00:36:59,880 --> 00:37:03,920 The fundamental difference is that electrons are fermions, 745 00:37:03,920 --> 00:37:09,400 so they cannot really be in the same state. 746 00:37:09,400 --> 00:37:15,090 Photons are bosons, so they can actually be in the same state. 747 00:37:15,090 --> 00:37:17,360 So what I really should have said-- and thank you 748 00:37:17,360 --> 00:37:20,600 for pointing it out-- is that in free space, 749 00:37:20,600 --> 00:37:22,340 they're described by the same equations. 750 00:37:22,340 --> 00:37:24,380 Of course, when they get inside matter, 751 00:37:24,380 --> 00:37:27,062 their behavior is quite different. 752 00:37:27,062 --> 00:37:28,520 But again, for example, if you look 753 00:37:28,520 --> 00:37:31,220 at the electrons that go ballistically through matter, 754 00:37:31,220 --> 00:37:34,880 they experience an effect that is very similar to refraction. 755 00:37:34,880 --> 00:37:36,350 So you can describe-- 756 00:37:36,350 --> 00:37:38,550 you still see Snell's Law, and so on. 757 00:37:38,550 --> 00:37:40,720 But of course, you see these additional phenomena, 758 00:37:40,720 --> 00:37:44,930 like all the electrons, which you don't see in light beams. 759 00:37:44,930 --> 00:37:46,100 So you're absolutely right. 760 00:37:46,100 --> 00:37:50,480 There's some significant differences 761 00:37:50,480 --> 00:37:51,950 which are very important. 762 00:37:51,950 --> 00:37:56,260 But there's also some very, very dominant 763 00:37:56,260 --> 00:37:57,970 and prominent commonalities. 764 00:37:57,970 --> 00:38:00,100 The same goes for light and sound. 765 00:38:00,100 --> 00:38:06,585 And our department recently merged with ocean engineering. 766 00:38:06,585 --> 00:38:07,960 And in ocean engineering, there's 767 00:38:07,960 --> 00:38:10,270 a lot of professors who do acoustics. 768 00:38:10,270 --> 00:38:12,620 So as a result, I started sitting in-- 769 00:38:12,620 --> 00:38:14,110 at the beginning, out of curiosity, 770 00:38:14,110 --> 00:38:16,360 I started sitting in a couple of the acoustic classes. 771 00:38:16,360 --> 00:38:21,580 And also, this year, I sat in the doctoral exam in acoustics. 772 00:38:21,580 --> 00:38:23,730 And I was surprised to see the same terms-- 773 00:38:23,730 --> 00:38:28,420 diffraction, refraction, Snell's law, waveguiding, 774 00:38:28,420 --> 00:38:31,000 all of these things, they happen in acoustics as well. 775 00:38:31,000 --> 00:38:33,220 So you could say the same thing about sound. 776 00:38:33,220 --> 00:38:36,130 To some approximation, sound effects 777 00:38:36,130 --> 00:38:40,120 are identical to optics, identical to light diffraction. 778 00:38:40,120 --> 00:38:43,120 But there's also cases of interaction between sound 779 00:38:43,120 --> 00:38:46,120 and matter that is radically different than interaction 780 00:38:46,120 --> 00:38:47,710 between light and matter. 781 00:38:47,710 --> 00:38:50,535 For example, I think it is impossible for sound 782 00:38:50,535 --> 00:38:52,000 to ionize matter. 783 00:38:52,000 --> 00:38:53,650 Light can ionize matter. 784 00:38:53,650 --> 00:38:57,460 I think sound has to be pretty darn strong to ionize, right? 785 00:38:57,460 --> 00:39:02,230 So there are significant differences, but also some very 786 00:39:02,230 --> 00:39:03,690 convenient commonalities. 787 00:39:03,690 --> 00:39:06,800 So all of a sudden, by studying one field, all of a sudden, 788 00:39:06,800 --> 00:39:09,100 you discover that you can understand quite a bit 789 00:39:09,100 --> 00:39:10,608 about a different field. 790 00:39:10,608 --> 00:39:11,650 So that's kind of useful. 791 00:39:14,480 --> 00:39:15,765 Any other questions? 792 00:39:22,900 --> 00:39:27,960 Let's start by saying a few things about what is light. 793 00:39:27,960 --> 00:39:30,260 So light is actually a form of energy. 794 00:39:30,260 --> 00:39:34,235 Really that's the simplest-- that's the only correct way 795 00:39:34,235 --> 00:39:35,450 to describe it. 796 00:39:35,450 --> 00:39:37,820 It is a form of energy that is transmitted 797 00:39:37,820 --> 00:39:40,160 as an electromagnetic wave. 798 00:39:40,160 --> 00:39:43,170 That's a quite correct description. 799 00:39:43,170 --> 00:39:46,490 But as I said before, you can think of it either as particles 800 00:39:46,490 --> 00:39:48,360 or as waves. 801 00:39:48,360 --> 00:39:53,220 So the particles are officially called photons. 802 00:39:53,220 --> 00:39:58,940 And what is a photon is actually not an easy thing to describe. 803 00:39:58,940 --> 00:40:01,070 Various scientists over the centuries 804 00:40:01,070 --> 00:40:03,860 fought over the definition of a photon. 805 00:40:03,860 --> 00:40:05,930 And we certainly don't want to go into quantum 806 00:40:05,930 --> 00:40:07,880 optics in this class. 807 00:40:07,880 --> 00:40:11,150 So we'll think of photons in a very simple-minded way, 808 00:40:11,150 --> 00:40:14,120 as bullets that carry energy-- 809 00:40:14,120 --> 00:40:20,630 a very small amount of energy, as we'll see in a second-- 810 00:40:20,630 --> 00:40:25,020 and they follow certain trajectories. 811 00:40:25,020 --> 00:40:27,860 So the trajectories we'll call rays. 812 00:40:27,860 --> 00:40:32,250 And I will describe these rays a little bit later. 813 00:40:32,250 --> 00:40:36,380 Now, the photon, one thing that the photons do have in common 814 00:40:36,380 --> 00:40:37,340 is their speed. 815 00:40:37,340 --> 00:40:40,310 It is, of course, the speed of light, which, in a vacuum, 816 00:40:40,310 --> 00:40:46,080 is the familiar 3 times 10 to the 8 meters per second. 817 00:40:46,080 --> 00:40:48,060 How much energy they carry? 818 00:40:48,060 --> 00:40:53,230 Well, the amount of energy is given by Planck's constant, 819 00:40:53,230 --> 00:41:00,360 which is a very small amount of 6.6 10 to the minus 34 joules 820 00:41:00,360 --> 00:41:03,920 times second, and then multiplied by a frequency. 821 00:41:03,920 --> 00:41:06,490 OK, so the frequency is, of course, hertz. 822 00:41:06,490 --> 00:41:07,710 So the units work out. 823 00:41:07,710 --> 00:41:12,570 The product over there is energy. 824 00:41:12,570 --> 00:41:13,680 What is the frequency? 825 00:41:13,680 --> 00:41:15,380 Where does it come about? 826 00:41:15,380 --> 00:41:18,900 Well, to really justify the presence of a frequency there, 827 00:41:18,900 --> 00:41:20,130 I have to see it. 828 00:41:20,130 --> 00:41:22,500 I have to go, actually, to the other way 829 00:41:22,500 --> 00:41:26,430 of describing light, which is as an electromagnetic wave. 830 00:41:26,430 --> 00:41:31,200 And of course, the name "wave" implies some sort 831 00:41:31,200 --> 00:41:34,120 of oscillatory motion. 832 00:41:34,120 --> 00:41:36,420 So the horizontal axis here is the direction 833 00:41:36,420 --> 00:41:38,050 of the propagation of the light. 834 00:41:38,050 --> 00:41:41,550 So the light is propagating from the left to the right. 835 00:41:41,550 --> 00:41:43,140 What is the vertical axis? 836 00:41:43,140 --> 00:41:46,050 The vertical axis is an electric field, actually. 837 00:41:46,050 --> 00:41:48,870 It is the same spot that you have in a capacitor where 838 00:41:48,870 --> 00:41:50,460 you charge it. 839 00:41:50,460 --> 00:41:53,020 So it is convenient to describe it as an electric field. 840 00:41:53,020 --> 00:41:55,920 You can also describe it is a magnetic field-- 841 00:41:55,920 --> 00:42:00,690 the same stuff that you see when you have a refrigerator magnet. 842 00:42:00,690 --> 00:42:03,980 You can put either quantity over here in the vertical axis 843 00:42:03,980 --> 00:42:07,470 because there are a couple of electromagnetic fields by, 844 00:42:07,470 --> 00:42:10,500 as the name suggests, it is a coupled oscillation 845 00:42:10,500 --> 00:42:12,973 of electric and magnetic fields. 846 00:42:12,973 --> 00:42:14,640 For now, let's stick to electric fields. 847 00:42:14,640 --> 00:42:18,030 In this class, I will say very little about magnetic fields. 848 00:42:18,030 --> 00:42:22,110 When I describe light as a wave, I will by default 849 00:42:22,110 --> 00:42:24,960 refer to an electric field, OK? 850 00:42:24,960 --> 00:42:29,270 So light is an electric field that oscillates 851 00:42:29,270 --> 00:42:31,370 as a function of position. 852 00:42:31,370 --> 00:42:34,870 And of course, a wave is not static. 853 00:42:34,870 --> 00:42:38,590 You, all of you, have seen waves in the Singapore 854 00:42:38,590 --> 00:42:40,930 Harbor, the Singapore River. 855 00:42:40,930 --> 00:42:43,510 You cannot see waves on the Charles right now because it is 856 00:42:43,510 --> 00:42:44,570 frozen. 857 00:42:44,570 --> 00:42:46,630 But during more normal times, you 858 00:42:46,630 --> 00:42:47,910 can see waves on the Charles. 859 00:42:47,910 --> 00:42:52,660 So you know a wave implies both a spatial structure-- 860 00:42:52,660 --> 00:42:54,430 if you look at the picture of a wave, 861 00:42:54,430 --> 00:42:58,690 you see oscillatory in the picture-- 862 00:42:58,690 --> 00:43:01,510 but also time, because a wave travels in time. 863 00:43:01,510 --> 00:43:05,570 So in the context here, the time valuable-- 864 00:43:05,570 --> 00:43:07,540 well, OK, I'll [INAUDIBLE] that back. 865 00:43:07,540 --> 00:43:09,880 But after some time lapse, the wave 866 00:43:09,880 --> 00:43:13,270 will actually move a little bit further, OK? 867 00:43:13,270 --> 00:43:17,080 So this is the sense of the wave propagation. 868 00:43:17,080 --> 00:43:21,140 So since you have an oscillatory quantity here, 869 00:43:21,140 --> 00:43:23,920 the period is called the wavelength-- 870 00:43:23,920 --> 00:43:25,900 the period in the space domain. 871 00:43:25,900 --> 00:43:30,820 So the distance between two peaks of the electric field 872 00:43:30,820 --> 00:43:33,520 oscillator there would define it as a wavelength. 873 00:43:33,520 --> 00:43:38,260 And it is related to the frequency, this quantity that 874 00:43:38,260 --> 00:43:41,470 enters in the particle description of light uses 875 00:43:41,470 --> 00:43:43,030 this equation here. 876 00:43:43,030 --> 00:43:45,040 The speed of light equals the product 877 00:43:45,040 --> 00:43:48,765 of the wavelength times the frequency. 878 00:43:48,765 --> 00:43:50,150 So we'll do the calculation here. 879 00:43:57,625 --> 00:43:59,000 Well, before we go calculation, I 880 00:43:59,000 --> 00:44:02,740 need to say something about what is-- 881 00:44:02,740 --> 00:44:04,990 I think I did something I was not supposed to do here. 882 00:44:04,990 --> 00:44:09,760 But anyway, the blackboard went up by itself. 883 00:44:09,760 --> 00:44:14,460 But this classroom is highly automated. 884 00:44:14,460 --> 00:44:19,850 So I guess there's some things that cannot be done. 885 00:44:19,850 --> 00:44:24,340 OK, so what are the typical wavelengths? 886 00:44:24,340 --> 00:44:28,820 So the electromagnetic spectrum actually spans all wavelengths 887 00:44:28,820 --> 00:44:33,580 from sort of infinitely long, or kilometers long, 888 00:44:33,580 --> 00:44:38,270 to very, very short, down to nanometers. 889 00:44:38,270 --> 00:44:42,560 The visible light, the light that we see with our own eyes, 890 00:44:42,560 --> 00:44:48,860 is in this range over here between approximately 891 00:44:48,860 --> 00:44:58,523 650 nanometers or so and 450 nanometers or so. 892 00:44:58,523 --> 00:44:59,440 So what's a nanometer? 893 00:44:59,440 --> 00:45:02,750 It's 10 to the minus 9 meters. 894 00:45:02,750 --> 00:45:04,620 So let's pick a convenient number here. 895 00:45:04,620 --> 00:45:06,475 Let's say lambda equals-- 896 00:45:09,160 --> 00:45:10,640 how about I do this here? 897 00:45:21,200 --> 00:45:24,400 OK, this is the wavelength. 898 00:45:24,400 --> 00:45:27,265 So our other question is c equals lambda nu. 899 00:45:27,265 --> 00:45:35,580 So it means that nu equals 3 times 10 to the 8 over five 900 00:45:35,580 --> 00:45:38,220 times 10 to the minus 7. 901 00:45:38,220 --> 00:45:45,530 So this is something of the order of 6 times 10 to the 14-- 902 00:45:45,530 --> 00:45:46,470 what? 903 00:45:46,470 --> 00:45:47,570 Hertz, right? 904 00:45:47,570 --> 00:45:51,050 It's a temporal frequency. 905 00:45:51,050 --> 00:45:53,390 So this oscillation that I showed 906 00:45:53,390 --> 00:45:57,230 before, it's a very high-frequency oscillation. 907 00:45:57,230 --> 00:45:59,420 is in there in the order of 10 to the 14 908 00:45:59,420 --> 00:46:03,600 had now we don't listen to the radio anymore 909 00:46:03,600 --> 00:46:10,870 we listen to you know podcasts or our satellite and so on. 910 00:46:10,870 --> 00:46:15,970 So we're not very familiar with radio frequencies. 911 00:46:15,970 --> 00:46:17,950 But I'm old enough to remember when you tuned 912 00:46:17,950 --> 00:46:22,150 your radio to 104.3 Megahertz. 913 00:46:22,150 --> 00:46:26,390 That happens to be Boston's WBCN station. 914 00:46:26,390 --> 00:46:31,290 So OK, Boston's WBCN station emits at 100 megahertz. 915 00:46:31,290 --> 00:46:33,380 It is actually the same stuff-- 916 00:46:33,380 --> 00:46:36,590 I'm going to force the machine to do what I want it to do, 917 00:46:36,590 --> 00:46:38,960 so I'm going to keep this down. 918 00:46:38,960 --> 00:46:42,320 OK, so let's say nu equals 100 megahertz. 919 00:46:45,470 --> 00:46:50,570 That is 10 to the 8, correct? 920 00:46:50,570 --> 00:46:56,240 So therefore, the wavelength now is what? 921 00:46:56,240 --> 00:46:58,700 c over the frequency so it is 3 times 922 00:46:58,700 --> 00:47:08,040 10 to the 8 meters per second over 10 to the 8 hertz. 923 00:47:08,040 --> 00:47:11,350 So this is now 3 meters. 924 00:47:11,350 --> 00:47:12,650 So it is still the same stuff. 925 00:47:12,650 --> 00:47:16,310 It is still light, if you wish, but of a much, much longer 926 00:47:16,310 --> 00:47:18,770 wavelength at the radio frequencies. 927 00:47:18,770 --> 00:47:23,120 So you can see that electromagnetic waves can span 928 00:47:23,120 --> 00:47:25,850 a very broad range of scales. 929 00:47:25,850 --> 00:47:28,940 In this class, the wavelengths of interest 930 00:47:28,940 --> 00:47:31,610 are in this range between the dashed lines 931 00:47:31,610 --> 00:47:34,370 and the infrared, which nominally 932 00:47:34,370 --> 00:47:38,390 ends at about 10 micrometers, and the ultraviolet, 933 00:47:38,390 --> 00:47:43,470 which nominally ends at about 30 nanometers. 934 00:47:43,470 --> 00:47:45,080 Where do the names come from? 935 00:47:45,080 --> 00:47:48,680 "Infra," in Latin, means "below"-- 936 00:47:48,680 --> 00:47:50,000 below red. 937 00:47:50,000 --> 00:47:53,160 So therefore, the term "infra" refers to what, the frequency 938 00:47:53,160 --> 00:47:54,258 or the wavelength? 939 00:47:59,520 --> 00:48:00,830 The frequency, right? 940 00:48:00,830 --> 00:48:04,770 Infrared has longer wavelengths than visible, 941 00:48:04,770 --> 00:48:08,490 and therefore it has smaller frequencies. 942 00:48:08,490 --> 00:48:12,170 So it is below the red in frequency. 943 00:48:12,170 --> 00:48:15,400 "Ultra," of course, means higher, also in Latin, 944 00:48:15,400 --> 00:48:19,770 so "ultraviolet" means higher frequencies than violet light. 945 00:48:19,770 --> 00:48:22,980 Not "violent" light, but "violet" light. 946 00:48:22,980 --> 00:48:27,740 OK, and the major difference, if you 947 00:48:27,740 --> 00:48:30,620 look at light propagation in free space 948 00:48:30,620 --> 00:48:33,890 it doesn't really matter which wavelength you are considering. 949 00:48:33,890 --> 00:48:35,720 But of course, the interaction with matter 950 00:48:35,720 --> 00:48:38,900 is radically different as you change wavelengths. 951 00:48:38,900 --> 00:48:42,500 So it is similar to the question you asked about electrons. 952 00:48:42,500 --> 00:48:45,680 It is also true for microwaves, or even 953 00:48:45,680 --> 00:48:47,920 for electromagnetic waves themselves. 954 00:48:47,920 --> 00:48:51,410 The way visible light interacts with matter 955 00:48:51,410 --> 00:48:55,730 is very different than microwaves and RF waves, 956 00:48:55,730 --> 00:48:57,970 and it is also very different than X-rays. 957 00:48:57,970 --> 00:49:00,920 So X-rays are actually the next highest 958 00:49:00,920 --> 00:49:06,350 in frequency after ultraviolet, and even higher in frequency 959 00:49:06,350 --> 00:49:07,460 are gamma rays. 960 00:49:07,460 --> 00:49:10,010 And I guess we stop there. 961 00:49:10,010 --> 00:49:11,680 But actually, we don't stop. 962 00:49:11,680 --> 00:49:13,970 The frequency can go, in principle, all the way 963 00:49:13,970 --> 00:49:14,570 to infinity. 964 00:49:14,570 --> 00:49:19,070 But the gamma rays is the highest that we can observe. 965 00:49:19,070 --> 00:49:21,140 Now, I promised to do a calculation 966 00:49:21,140 --> 00:49:25,850 of the energy-- how much energy is carried by a photon. 967 00:49:25,850 --> 00:49:29,920 So remember the formula, equals h nu, 968 00:49:29,920 --> 00:49:35,060 where h is 6.6 times 10 to the-- remember how much it was, 969 00:49:35,060 --> 00:49:36,880 the exponent? 970 00:49:36,880 --> 00:49:37,600 34, right? 971 00:49:42,800 --> 00:49:48,350 So let's pick one here-- let's say this one-- which is visible 972 00:49:48,350 --> 00:49:49,610 wavelength. 973 00:49:49,610 --> 00:49:56,500 So it is six times 10 to the 14 times inverse second. 974 00:49:56,500 --> 00:49:58,460 OK, so these conveniently cancel. 975 00:49:58,460 --> 00:50:01,670 And 6 times 6 is-- 976 00:50:01,670 --> 00:50:04,990 let's call it 10 for convenience. 977 00:50:04,990 --> 00:50:08,030 So it is 10, and this is 14, of course. 978 00:50:08,030 --> 00:50:10,840 So this is 10 to the minus 20 joules. 979 00:50:10,840 --> 00:50:13,220 OK, my arithmetic is, obviously, wrong. 980 00:50:13,220 --> 00:50:18,710 OK, what is the pedagogical message here? 981 00:50:18,710 --> 00:50:21,470 That when we do order of magnitude calculations-- 982 00:50:21,470 --> 00:50:25,498 6.6 times 6.6 times equals 10, let's-- 983 00:50:25,498 --> 00:50:26,540 actually, I got it wrong. 984 00:50:26,540 --> 00:50:27,945 I should have put "100." 985 00:50:27,945 --> 00:50:30,640 So minus 19. 986 00:50:30,640 --> 00:50:34,460 OK, so just the order of magnitude, right? 987 00:50:34,460 --> 00:50:37,330 I'm not looking for the exact answer here. 988 00:50:37,330 --> 00:50:39,060 Actually, it's very interesting. 989 00:50:39,060 --> 00:50:41,450 I did my graduate in Greece. 990 00:50:41,450 --> 00:50:43,500 And over there, the professors were very careful. 991 00:50:43,500 --> 00:50:47,160 So here, they would have written 39.6, or whatever 992 00:50:47,160 --> 00:50:48,928 it is-- the actual number. 993 00:50:48,928 --> 00:50:50,720 Then, I went to graduate school at Caltech. 994 00:50:50,720 --> 00:50:54,970 And I took my first class in quantum electronics 995 00:50:54,970 --> 00:50:57,020 by a fellow called Amnom Yariv, who 996 00:50:57,020 --> 00:50:59,300 is pretty well-known in the field of lasers. 997 00:50:59,300 --> 00:51:00,710 So we walked into classes, and he 998 00:51:00,710 --> 00:51:03,220 started doing things like that-- that pi equals 3, 999 00:51:03,220 --> 00:51:05,710 pi squared equals 10. 1000 00:51:05,710 --> 00:51:06,960 And at first, I was horrified. 1001 00:51:06,960 --> 00:51:10,230 But then I realized he had a point-- that very often, it 1002 00:51:10,230 --> 00:51:13,470 is pointless to do exact calculations if you're 1003 00:51:13,470 --> 00:51:15,420 looking for an order of magnitude result. 1004 00:51:15,420 --> 00:51:18,082 For example, is the bullet going to crash into a wall, 1005 00:51:18,082 --> 00:51:19,290 or is it going to go through? 1006 00:51:19,290 --> 00:51:20,820 Is it going to go back, or what? 1007 00:51:20,820 --> 00:51:22,612 For that, you don't need the exact numbers. 1008 00:51:22,612 --> 00:51:27,193 Of course, exact numbers are valuable in some other cases. 1009 00:51:27,193 --> 00:51:28,610 It's kind of an interesting skill, 1010 00:51:28,610 --> 00:51:31,370 to know when to do an half-calculation 1011 00:51:31,370 --> 00:51:34,190 and when to do an exact calculation, and what 1012 00:51:34,190 --> 00:51:36,710 level of accuracy you need, depending 1013 00:51:36,710 --> 00:51:39,153 on the resources that you have, the time that you have, 1014 00:51:39,153 --> 00:51:41,320 the nature of the answer you're looking for, and on, 1015 00:51:41,320 --> 00:51:43,560 and so forth. 1016 00:51:43,560 --> 00:51:47,680 OK, so for our purposes here for now, 6 times 6 equals 100. 1017 00:51:47,680 --> 00:51:49,470 So we'll get a very small energy, right? 1018 00:51:49,470 --> 00:51:52,790 It's 10 to the minus 19 joules. 1019 00:51:52,790 --> 00:51:57,710 If you go to higher frequencies, in the range of X-rays, 1020 00:51:57,710 --> 00:52:02,390 the energy would go up by a factor of maybe a couple 1021 00:52:02,390 --> 00:52:04,163 of orders of magnitude. 1022 00:52:04,163 --> 00:52:06,080 So in these kinds of frequencies, of energies, 1023 00:52:06,080 --> 00:52:09,230 if you go up to 10 to the minus 16 joules or so, 1024 00:52:09,230 --> 00:52:12,110 it becomes comparable with the ionizing radiation. 1025 00:52:12,110 --> 00:52:16,850 So you see now why light frequency is very important 1026 00:52:16,850 --> 00:52:19,210 when it comes to interaction with matter. 1027 00:52:19,210 --> 00:52:21,710 Because visible light, the photon, 1028 00:52:21,710 --> 00:52:25,190 each photon that impinges on an atom in a material 1029 00:52:25,190 --> 00:52:27,380 has a relatively low energy. 1030 00:52:27,380 --> 00:52:29,180 It can do something to the material-- 1031 00:52:29,180 --> 00:52:30,530 we'll talk about it later-- 1032 00:52:30,530 --> 00:52:31,850 but it cannot ionize it. 1033 00:52:31,850 --> 00:52:33,500 If you increase the frequency, you 1034 00:52:33,500 --> 00:52:36,080 increase the energy of the photon, and all of a sudden, 1035 00:52:36,080 --> 00:52:39,860 you can get ionizing effects. 1036 00:52:39,860 --> 00:52:42,140 So these sort of calculations give you 1037 00:52:42,140 --> 00:52:44,490 an idea of what's going on. 1038 00:52:48,560 --> 00:52:52,610 And of course, if you conclude the energy carried 1039 00:52:52,610 --> 00:52:57,620 by a microwave photon, it will be several orders of magnitude 1040 00:52:57,620 --> 00:52:58,120 lower-- 1041 00:52:58,120 --> 00:53:01,580 I think something like five or six orders of magnitude 1042 00:53:01,580 --> 00:53:04,220 smaller. 1043 00:53:04,220 --> 00:53:06,510 OK, any questions about that? 1044 00:53:06,510 --> 00:53:07,680 About photons or-- 1045 00:53:14,250 --> 00:53:17,392 Let me say a few things about wave propagation. 1046 00:53:17,392 --> 00:53:19,850 At the beginning of the class, we'll do geometrical optics. 1047 00:53:19,850 --> 00:53:22,610 But I want to say a few things about waves 1048 00:53:22,610 --> 00:53:26,432 that we need before geometrical optics begins to make sense. 1049 00:53:26,432 --> 00:53:27,890 So the first things that we learned 1050 00:53:27,890 --> 00:53:29,540 is wavelength and frequency, right? 1051 00:53:29,540 --> 00:53:34,140 These two things are important even in geometrical optics. 1052 00:53:34,140 --> 00:53:36,490 The wavelength is a very important concept. 1053 00:53:36,490 --> 00:53:39,840 The thing I want to talk about is, a little bit, to show you 1054 00:53:39,840 --> 00:53:42,520 what the wave looks like. 1055 00:53:42,520 --> 00:53:44,760 So this is very simple, one-dimensional wave. 1056 00:53:44,760 --> 00:53:47,350 And what I've done is I have plotted it 1057 00:53:47,350 --> 00:53:49,150 at different snapshots in time. 1058 00:53:49,150 --> 00:53:54,150 So the horizontal axis, again, is the propagation distance 1059 00:53:54,150 --> 00:54:00,360 that the wave is propagating, and the vertical axis is-- 1060 00:54:00,360 --> 00:54:03,410 well, this part of the small axis is time, 1061 00:54:03,410 --> 00:54:06,750 and then I have captured different snapshots. 1062 00:54:06,750 --> 00:54:08,950 So as you can see, there's a sense of motion here. 1063 00:54:08,950 --> 00:54:12,600 If you latch on a peak of the wave, 1064 00:54:12,600 --> 00:54:15,270 you will see that at different instances, 1065 00:54:15,270 --> 00:54:18,600 the peak is moving from the left to the right. 1066 00:54:18,600 --> 00:54:20,350 And of course, the symbol uppercase 1067 00:54:20,350 --> 00:54:22,180 T here is the frequency. 1068 00:54:22,180 --> 00:54:24,300 I think it was defined in an earlier slide. 1069 00:54:24,300 --> 00:54:26,650 It is simply the inverse-- 1070 00:54:26,650 --> 00:54:29,370 I'm sorry, that is the period, the temporal period, 1071 00:54:29,370 --> 00:54:33,820 the inverse of the temporal frequency. 1072 00:54:33,820 --> 00:54:37,960 And of course, after one full time 1073 00:54:37,960 --> 00:54:40,700 period, the wave replicates itself. 1074 00:54:40,700 --> 00:54:43,630 So if you look carefully at this wave from over here, 1075 00:54:43,630 --> 00:54:46,300 it is identical to the wavefront at t equals 0 1076 00:54:46,300 --> 00:54:50,680 that I'm not tall enough to reach. 1077 00:54:50,680 --> 00:54:52,690 So you can pick arbitrarily. 1078 00:54:52,690 --> 00:54:57,080 You can pick any point in the wave. 1079 00:54:57,080 --> 00:54:58,690 I happened to pick a peak. 1080 00:54:58,690 --> 00:55:02,200 OK, I happened to pick a peak, and I tracked that peak 1081 00:55:02,200 --> 00:55:03,730 as the wave propagates. 1082 00:55:03,730 --> 00:55:06,970 I could equally well have picked a point over here 1083 00:55:06,970 --> 00:55:07,960 and tracked it. 1084 00:55:07,960 --> 00:55:11,330 It would also have propagated the same way. 1085 00:55:11,330 --> 00:55:17,120 And so this concept of a point in the wave, if you wish, 1086 00:55:17,120 --> 00:55:21,230 or more generally a surface of a wave 1087 00:55:21,230 --> 00:55:26,760 that propagates with a wave as a function of time 1088 00:55:26,760 --> 00:55:29,030 is called a wavefront. 1089 00:55:29,030 --> 00:55:32,630 And the term is very suggestive. 1090 00:55:32,630 --> 00:55:33,920 It implies motion. 1091 00:55:33,920 --> 00:55:35,673 It's like a battlefront. 1092 00:55:35,673 --> 00:55:36,590 What is a battlefront? 1093 00:55:36,590 --> 00:55:39,650 It's the people who are unlucky enough to have 1094 00:55:39,650 --> 00:55:42,590 been picked to be at the frontline of the battle. 1095 00:55:42,590 --> 00:55:47,780 So if you've seen all these old, horrible movies about battles 1096 00:55:47,780 --> 00:55:49,640 in the Middle Ages, you see all these guys 1097 00:55:49,640 --> 00:55:51,795 with their shields going ahead. 1098 00:55:51,795 --> 00:55:54,020 And that's a battlefront, moving. 1099 00:55:54,020 --> 00:55:56,150 So a wavefront is a similar concept. 1100 00:55:56,150 --> 00:56:01,040 You have a front that is moving as the energy of the wave 1101 00:56:01,040 --> 00:56:04,060 is propagating. 1102 00:56:04,060 --> 00:56:06,060 So it's perhaps not a very interesting wavefront 1103 00:56:06,060 --> 00:56:08,250 because it is one-dimensional, right? 1104 00:56:08,250 --> 00:56:11,610 The wave is propagating along a sort of linear axis. 1105 00:56:11,610 --> 00:56:15,780 In a second, I will show you more interesting wavefronts 1106 00:56:15,780 --> 00:56:19,753 that are of relevance in this class. 1107 00:56:19,753 --> 00:56:21,420 The other thing I want to point out here 1108 00:56:21,420 --> 00:56:24,660 is, again, I want to bring up the concept of the wavelength. 1109 00:56:24,660 --> 00:56:26,730 And we defined the wavelength already 1110 00:56:26,730 --> 00:56:29,070 as the distance between two peaks. 1111 00:56:29,070 --> 00:56:31,200 So if you look at two peaks over here, 1112 00:56:31,200 --> 00:56:34,080 the distance is, by definition, of a wavelength. 1113 00:56:34,080 --> 00:56:37,140 But also, the wavelength, it has a different meaning. 1114 00:56:37,140 --> 00:56:39,540 If you look at it from the point of view of propagation 1115 00:56:39,540 --> 00:56:42,150 of the wave, it is also the distance 1116 00:56:42,150 --> 00:56:45,240 that the wave propagated in-- 1117 00:56:45,240 --> 00:56:46,020 how long? 1118 00:56:46,020 --> 00:56:48,660 Well, one period, right? 1119 00:56:48,660 --> 00:56:50,400 And in fact, this is where the equation c 1120 00:56:50,400 --> 00:56:52,140 equals lambda nu comes from. 1121 00:56:58,780 --> 00:57:00,830 I'll let you do that as a homework. 1122 00:57:00,830 --> 00:57:04,720 But if you think about it, if you treat the wave 1123 00:57:04,720 --> 00:57:11,030 as a particle that took 3 seconds to move 1124 00:57:11,030 --> 00:57:15,520 lambda units of distance, then its velocity c 1125 00:57:15,520 --> 00:57:18,520 must obey this equation over here. 1126 00:57:18,520 --> 00:57:21,310 It's a one-line derivation kind of thing. 1127 00:57:21,310 --> 00:57:22,910 I'll let you do it as a homework. 1128 00:57:22,910 --> 00:57:25,630 And also, I want to emphasize that this equation 1129 00:57:25,630 --> 00:57:30,340 that we called the spatial relation in the previous slide, 1130 00:57:30,340 --> 00:57:33,460 it is only true if light propagates in free space 1131 00:57:33,460 --> 00:57:35,110 or in uniform media. 1132 00:57:35,110 --> 00:57:39,268 If you put light, for example, in a confined space, 1133 00:57:39,268 --> 00:57:41,560 this equation changes, and it becomes a little bit more 1134 00:57:41,560 --> 00:57:43,360 complicated. 1135 00:57:43,360 --> 00:57:46,600 But in this class, we don't deal with this phenomenon. 1136 00:57:46,600 --> 00:57:49,690 If you want to learn about more complicated dispersion 1137 00:57:49,690 --> 00:57:52,930 relations, you will have to take Professor Fujimoto's class 1138 00:57:52,930 --> 00:57:55,600 in electrical engineering. 1139 00:57:55,600 --> 00:57:57,780 I might mention something like this in passing, 1140 00:57:57,780 --> 00:57:59,520 but not in great detail. 1141 00:57:59,520 --> 00:58:01,080 For this, we will be happy enough 1142 00:58:01,080 --> 00:58:05,950 to take this as a dispersion equation of the light. 1143 00:58:05,950 --> 00:58:07,950 But again, I want to alert you that there's also 1144 00:58:07,950 --> 00:58:12,900 other dispersion relations that may occur. 1145 00:58:12,900 --> 00:58:15,970 OK, the other thing that I will not spend too much time here, 1146 00:58:15,970 --> 00:58:20,880 but it will come up later with great force and great detail 1147 00:58:20,880 --> 00:58:23,600 is the concept of phase delay. 1148 00:58:23,600 --> 00:58:28,190 So you probably remember this from your trigonometry class. 1149 00:58:28,190 --> 00:58:30,500 If you have a periodic phenomenon 1150 00:58:30,500 --> 00:58:34,430 or a periodic function, you can pick an arbitrary point in time 1151 00:58:34,430 --> 00:58:36,200 and call it your reference. 1152 00:58:36,200 --> 00:58:38,390 And then, as the phenomenon evolves, 1153 00:58:38,390 --> 00:58:43,890 you can refer to this initial point as if with a phase delay. 1154 00:58:43,890 --> 00:58:46,760 So the phase delay is relative to 2pi, 1155 00:58:46,760 --> 00:58:49,310 which measures one full cycle. 1156 00:58:49,310 --> 00:58:54,590 So then you can interpret these snapshots over here 1157 00:58:54,590 --> 00:58:58,850 as phase-delayed versions of the original wave. 1158 00:58:58,850 --> 00:59:04,580 So for example, between 0 and 1/8 of a period, 1159 00:59:04,580 --> 00:59:08,660 your phase delay equals pi over 4, because 2pi over 8 1160 00:59:08,660 --> 00:59:10,460 equals pi over 4. 1161 00:59:10,460 --> 00:59:13,190 So this is a concept that will come up again, as I said, 1162 00:59:13,190 --> 00:59:14,550 in great detail. 1163 00:59:14,550 --> 00:59:19,620 I just wanted you to be a little bit aware of it right now. 1164 00:59:19,620 --> 00:59:23,280 What I really wanted to emphasize over here 1165 00:59:23,280 --> 00:59:26,380 is that light does not usually propagate along 1166 00:59:26,380 --> 00:59:30,150 an exact one line, as I showed in a previous line, 1167 00:59:30,150 --> 00:59:31,770 but it propagates in 3D space. 1168 00:59:31,770 --> 00:59:33,040 So it can expand. 1169 00:59:33,040 --> 00:59:34,040 It can contract. 1170 00:59:34,040 --> 00:59:36,450 It can do weird things, right? 1171 00:59:36,450 --> 00:59:38,340 So to do that, we need a slightly more 1172 00:59:38,340 --> 00:59:39,360 elaborate description. 1173 00:59:39,360 --> 00:59:43,017 So this is an attempt to plot 3D space. 1174 00:59:43,017 --> 00:59:45,100 And if you think about the wavefront in this case, 1175 00:59:45,100 --> 00:59:48,390 it is a surface that moves from left 1176 00:59:48,390 --> 00:59:51,240 to right as a function of time. 1177 00:59:51,240 --> 00:59:54,292 So as the wavefront propagates, the surface is moving. 1178 00:59:54,292 --> 00:59:56,000 By the way, this is a fictitious surface. 1179 00:59:56,000 --> 00:59:59,220 I'm not thinking of a physical surface or anything. 1180 00:59:59,220 --> 01:00:03,680 But if you think about the energy that the light carries, 1181 01:00:03,680 --> 01:00:07,430 the energy is actually moving as the wave propagates. 1182 01:00:07,430 --> 01:00:09,410 This is how you can connect the two. 1183 01:00:09,410 --> 01:00:11,200 If you go out to the Charles-- 1184 01:00:11,200 --> 01:00:13,970 OK, you have to wait until April when it unfreezes-- 1185 01:00:13,970 --> 01:00:16,990 but if you look at the waves on the water-- 1186 01:00:16,990 --> 01:00:19,490 of course, you can do it at home on your bucket or something 1187 01:00:19,490 --> 01:00:20,130 like that-- 1188 01:00:20,130 --> 01:00:22,630 but if you look at the waves, there's also a physical sense, 1189 01:00:22,630 --> 01:00:24,770 because the water wave, there's a crest. 1190 01:00:24,770 --> 01:00:26,420 So there wavefront of the water wave 1191 01:00:26,420 --> 01:00:30,687 is the crest that moves as the wave propagates. 1192 01:00:33,320 --> 01:00:37,800 So these surfaces, the weapons, they can have different shapes. 1193 01:00:37,800 --> 01:00:40,490 They cannot have arbitrary shapes because they're governed 1194 01:00:40,490 --> 01:00:43,880 by the laws of light propagation. 1195 01:00:43,880 --> 01:00:48,860 But certain allowable shapes turn out to be very simple, 1196 01:00:48,860 --> 01:00:50,930 and we will be dealing with them a lot. 1197 01:00:50,930 --> 01:00:53,480 So the simplest is a planar wavefront 1198 01:00:53,480 --> 01:00:56,960 that, as the name implies, is a plane. 1199 01:00:56,960 --> 01:01:00,260 And the next simple is a spherical wavefront, 1200 01:01:00,260 --> 01:01:03,450 which, again, as the name implies, is a sphere. 1201 01:01:03,450 --> 01:01:08,330 So you can think those as our two major wavefronts 1202 01:01:08,330 --> 01:01:10,770 that we'll be dealing with throughout the class-- 1203 01:01:10,770 --> 01:01:12,830 the planar wavefront and the spherical. 1204 01:01:12,830 --> 01:01:14,980 And we'll-- yes. 1205 01:01:14,980 --> 01:01:17,530 AUDIENCE: So in the last slide, you showed the electric field 1206 01:01:17,530 --> 01:01:18,760 as being the y-axis. 1207 01:01:18,760 --> 01:01:21,070 But here, it's space, not field. 1208 01:01:24,030 --> 01:01:26,790 GEORGE BARBASTATHIS: Yes, so that is correct, and thank you. 1209 01:01:26,790 --> 01:01:28,620 And I should relabel the slide. 1210 01:01:28,620 --> 01:01:34,380 Here, the two axes, they correspond to x and y, 1211 01:01:34,380 --> 01:01:36,370 the space coordinates, yeah. 1212 01:01:36,370 --> 01:01:40,200 And the electric field is not found here because I cannot 1213 01:01:40,200 --> 01:01:42,100 plot a fourth dimension. 1214 01:01:42,100 --> 01:01:45,750 So what is happening here is the electric field is maximum at t 1215 01:01:45,750 --> 01:01:47,230 equal to 0. 1216 01:01:47,230 --> 01:01:51,690 So at t equals 0, the electric field is maximum on this plane. 1217 01:01:51,690 --> 01:01:54,630 If you wait 1/8 of a period, the field 1218 01:01:54,630 --> 01:01:56,220 will be maximum at this plane. 1219 01:01:56,220 --> 01:01:58,620 If you wait another 1/8 of a period, 1220 01:01:58,620 --> 01:02:00,540 the field is maximum on this plane. 1221 01:02:00,540 --> 01:02:03,090 So the wavefront, in this case, is the maximum 1222 01:02:03,090 --> 01:02:04,290 of the electric field-- 1223 01:02:04,290 --> 01:02:06,480 the crest, if you wish, of the electric field-- 1224 01:02:06,480 --> 01:02:08,740 as it propagates through space. 1225 01:02:08,740 --> 01:02:10,790 And the same is here. 1226 01:02:10,790 --> 01:02:14,990 Again, these surfaces mean that the field is maximum 1227 01:02:14,990 --> 01:02:17,160 on the surface at t equals 0. 1228 01:02:17,160 --> 01:02:19,340 And then, 1/8 of a period later, the field 1229 01:02:19,340 --> 01:02:22,660 is maximum on the surface, and so on, and so forth. 1230 01:02:22,660 --> 01:02:23,260 Thanks, yeah. 1231 01:02:23,260 --> 01:02:28,020 So that's a very important clarification. 1232 01:02:28,020 --> 01:02:31,400 Now, what do you think should happen to the energy 1233 01:02:31,400 --> 01:02:34,370 density in the two cases? 1234 01:02:34,370 --> 01:02:36,170 Suppose I have a fixed amount of energy 1235 01:02:36,170 --> 01:02:40,438 that is entered in on the left. 1236 01:02:40,438 --> 01:02:41,730 Are they different in some way? 1237 01:02:41,730 --> 01:02:43,387 Yeah. 1238 01:02:43,387 --> 01:02:45,543 AUDIENCE: [INAUDIBLE] 1239 01:02:45,543 --> 01:02:46,960 GEORGE BARBASTATHIS: That's right. 1240 01:02:46,960 --> 01:02:50,280 Can I can ask you to push the button and repeat that? 1241 01:02:50,280 --> 01:02:52,290 Yeah. 1242 01:02:52,290 --> 01:02:55,170 AUDIENCE: The plane wave's energy is constant, 1243 01:02:55,170 --> 01:02:58,050 energy density is constant, and the spherical wave's energy 1244 01:02:58,050 --> 01:02:59,582 density is smaller. 1245 01:02:59,582 --> 01:03:00,790 GEORGE BARBASTATHIS: Correct. 1246 01:03:00,790 --> 01:03:01,720 AUDIENCE: As it expands. 1247 01:03:01,720 --> 01:03:03,137 GEORGE BARBASTATHIS: Correct, yes, 1248 01:03:03,137 --> 01:03:04,990 because energy has to be concerned. 1249 01:03:04,990 --> 01:03:10,410 So in this case, the wavefront is invariant, 1250 01:03:10,410 --> 01:03:12,360 so the energy must remain constant. 1251 01:03:12,360 --> 01:03:14,520 In this case, the wavefront is expanding, 1252 01:03:14,520 --> 01:03:19,270 so the energy density will decrease as you go away. 1253 01:03:19,270 --> 01:03:21,360 We will make this more precise later. 1254 01:03:21,360 --> 01:03:23,590 We'll define what we mean by energy density. 1255 01:03:23,590 --> 01:03:25,710 In fact, it is called intensity. 1256 01:03:25,710 --> 01:03:28,420 So we'll define that. 1257 01:03:28,420 --> 01:03:30,390 So basically if you measure the energy 1258 01:03:30,390 --> 01:03:34,500 in watts per area, watts per centimeter square, 1259 01:03:34,500 --> 01:03:36,630 in this case, it has to decrease in order 1260 01:03:36,630 --> 01:03:38,640 to make sure that the energy you started 1261 01:03:38,640 --> 01:03:44,190 with at the center of the sphere is preserved throughout. 1262 01:03:44,190 --> 01:03:46,800 The next concept I would like to define is the ray. 1263 01:03:46,800 --> 01:03:49,140 And the reason we introduced wavefronts 1264 01:03:49,140 --> 01:03:53,550 is primarily because I wanted to define relatively precisely, 1265 01:03:53,550 --> 01:03:56,550 now, what I mean by a ray. 1266 01:03:56,550 --> 01:04:00,470 For the next 4 weeks, we will be talking about rays exclusively, 1267 01:04:00,470 --> 01:04:02,070 OK? 1268 01:04:02,070 --> 01:04:05,160 So a ray is basically a normal to the wavefront. 1269 01:04:05,160 --> 01:04:08,670 That is the correct, accurate definition of a ray. 1270 01:04:08,670 --> 01:04:11,820 You take this surfaces, you plug the normals, 1271 01:04:11,820 --> 01:04:13,807 and these lines are the rays. 1272 01:04:13,807 --> 01:04:15,390 So in this case, the rays are parallel 1273 01:04:15,390 --> 01:04:18,360 because all the surfaces are parallel planes. 1274 01:04:18,360 --> 01:04:20,910 In this case, the rays form a fan, 1275 01:04:20,910 --> 01:04:23,680 like a divergent fan, that attaches 1276 01:04:23,680 --> 01:04:27,270 at each point on the spheres. 1277 01:04:27,270 --> 01:04:31,280 The fan components are normal to the surfaces. 1278 01:04:31,280 --> 01:04:34,230 And you can also think of them as trajectories 1279 01:04:34,230 --> 01:04:39,846 over which the particles of light propagate. 1280 01:04:39,846 --> 01:04:41,590 It is not, perhaps, very accurate 1281 01:04:41,590 --> 01:04:44,200 to think of the particles as photons in this case. 1282 01:04:44,200 --> 01:04:47,740 So think of them as some sort of fictitious light bullets that 1283 01:04:47,740 --> 01:04:52,370 propagate down the ray trajectories. 1284 01:04:52,370 --> 01:04:54,020 And the rays have several properties, 1285 01:04:54,020 --> 01:04:57,050 which I will ratify later in the class. 1286 01:04:57,050 --> 01:04:59,800 The rays have to be continuous in piecewise differential. 1287 01:04:59,800 --> 01:05:01,480 A ray cannot jump, for example. 1288 01:05:01,480 --> 01:05:04,430 You cannot have a ray that looks like this. 1289 01:05:12,910 --> 01:05:14,836 That cannot happen-- forbidden. 1290 01:05:18,724 --> 01:05:26,440 A ray can have a continuous but, perhaps, not differentiable 1291 01:05:26,440 --> 01:05:27,410 band like this. 1292 01:05:27,410 --> 01:05:28,700 So that's allowed. 1293 01:05:28,700 --> 01:05:31,150 And it can also have a smooth, continuous path. 1294 01:05:31,150 --> 01:05:33,190 That's also allowed. 1295 01:05:33,190 --> 01:05:35,970 OK, that is, obviously, why it is forbidden. 1296 01:05:35,970 --> 01:05:39,190 It is kind of strange to imagine the photon disappearing 1297 01:05:39,190 --> 01:05:40,650 and appearing again someplace else. 1298 01:05:44,260 --> 01:05:48,290 The others we will see later in action. 1299 01:05:48,290 --> 01:05:53,670 And from our experience, rays are straight lines. 1300 01:05:53,670 --> 01:05:55,910 And why do we say that, from our experience? 1301 01:05:55,910 --> 01:05:58,200 Where have you seen rays in everyday life? 1302 01:06:01,320 --> 01:06:02,820 Button. 1303 01:06:02,820 --> 01:06:03,532 AUDIENCE: Lasers. 1304 01:06:03,532 --> 01:06:04,990 GEORGE BARBASTATHIS: Lasers is one. 1305 01:06:04,990 --> 01:06:08,460 But usually, if you have the beam coming out of a laser, 1306 01:06:08,460 --> 01:06:12,260 it looks kind of like a straight line. 1307 01:06:12,260 --> 01:06:15,800 Another example, perhaps, from even more everyday life. 1308 01:06:15,800 --> 01:06:16,730 AUDIENCE: Shadows. 1309 01:06:16,730 --> 01:06:18,522 GEORGE BARBASTATHIS: Shadows, that's right. 1310 01:06:18,522 --> 01:06:20,240 If you look at shadows, the light 1311 01:06:20,240 --> 01:06:24,070 appears to come out straight out of the shadows. 1312 01:06:24,070 --> 01:06:26,105 So it's a little bit strange that I drew a ray 1313 01:06:26,105 --> 01:06:28,340 as a curved trajectory. 1314 01:06:28,340 --> 01:06:31,250 We will see a bit later, maybe even today if we don't run out 1315 01:06:31,250 --> 01:06:36,590 of time, that light rays can actually follow curved paths 1316 01:06:36,590 --> 01:06:38,390 under certain conditions. 1317 01:06:38,390 --> 01:06:41,810 But what is for sure, that in free space or uniform space 1318 01:06:41,810 --> 01:06:42,940 like air-- 1319 01:06:42,940 --> 01:06:44,990 we observe shadows in air. 1320 01:06:44,990 --> 01:06:51,810 So air is pretty much uniform, and for that reason, 1321 01:06:51,810 --> 01:06:53,950 rays propagate in straight lines. 1322 01:06:53,950 --> 01:06:56,550 By the way, you don't have to go too far to see examples 1323 01:06:56,550 --> 01:06:59,280 of curved ray propagation. 1324 01:06:59,280 --> 01:07:01,470 The best example is flicker. 1325 01:07:01,470 --> 01:07:04,680 If you go up in the mountains at night 1326 01:07:04,680 --> 01:07:06,753 and you look down at the city beneath-- 1327 01:07:06,753 --> 01:07:08,420 I don't think you can do that in Boston. 1328 01:07:08,420 --> 01:07:10,210 We don't have any mountains high enough. 1329 01:07:10,210 --> 01:07:13,140 But in Los Angeles, for example, it's very pronounced. 1330 01:07:13,140 --> 01:07:16,020 If you go to the Hollywood Hills and look down, you see flicker. 1331 01:07:16,020 --> 01:07:18,380 The lights in the city, they are not steady. 1332 01:07:18,380 --> 01:07:20,940 They kind of flicker. 1333 01:07:20,940 --> 01:07:25,010 So the result of that is because the atmosphere, 1334 01:07:25,010 --> 01:07:26,770 it is not an exactly uniform medium. 1335 01:07:26,770 --> 01:07:31,250 You have temperature changes, air currents, and so on. 1336 01:07:31,250 --> 01:07:35,080 And because of that, the rays between the city lights 1337 01:07:35,080 --> 01:07:38,590 and your eye, the rays follow a sort of curved path. 1338 01:07:38,590 --> 01:07:40,800 Very slightly curved, but because they propagate 1339 01:07:40,800 --> 01:07:43,600 a long distance, it is enough to result in this flicker 1340 01:07:43,600 --> 01:07:45,340 phenomenon. 1341 01:07:45,340 --> 01:07:47,270 OK, so from that-- 1342 01:07:47,270 --> 01:07:50,060 it is not quite obvious as in the shadow-- 1343 01:07:50,060 --> 01:07:54,010 but from that, we have kind of experienced, all of us, 1344 01:07:54,010 --> 01:07:57,125 that the rays might actually not propagate along 1345 01:07:57,125 --> 01:07:58,170 a straight path. 1346 01:07:58,170 --> 01:08:00,020 And in a second, I will define when 1347 01:08:00,020 --> 01:08:02,450 that happens-- when a ray can propagate 1348 01:08:02,450 --> 01:08:06,650 in a curved trajectory. 1349 01:08:06,650 --> 01:08:11,770 Before I do that, I already implied that the reason 1350 01:08:11,770 --> 01:08:14,420 rays might do strange things, like deviate 1351 01:08:14,420 --> 01:08:16,109 from the straight and narrow-- 1352 01:08:16,109 --> 01:08:18,710 I'm sorry, might deviate from the straight path-- 1353 01:08:18,710 --> 01:08:21,950 is because of interaction with matter, right? 1354 01:08:21,950 --> 01:08:26,120 It is the non-uniformity in air, in my earlier example, 1355 01:08:26,120 --> 01:08:29,670 that caused the rays to bend. 1356 01:08:29,670 --> 01:08:33,930 So then, the next topic is a very simple description 1357 01:08:33,930 --> 01:08:36,240 of how light interacts with matter. 1358 01:08:36,240 --> 01:08:38,180 And for now, I will say it is a fairy 1359 01:08:38,180 --> 01:08:41,550 tale, because we don't know enough electromagnetics yet. 1360 01:08:41,550 --> 01:08:44,670 I will come back to this topic after we define light 1361 01:08:44,670 --> 01:08:47,010 as an electromagnetic wave. 1362 01:08:47,010 --> 01:08:50,490 I will come back to this topic and tell you more rigorously 1363 01:08:50,490 --> 01:08:52,610 how light interacts with matter. 1364 01:08:52,610 --> 01:08:54,420 For now, very briefly, I will tell you 1365 01:08:54,420 --> 01:08:58,430 that there is three types of interaction 1366 01:08:58,430 --> 01:09:00,410 that we'll discuss in this class-- 1367 01:09:00,410 --> 01:09:03,470 absorption, refraction, and scattering. 1368 01:09:03,470 --> 01:09:06,050 So today, I will define absorption and refraction 1369 01:09:06,050 --> 01:09:10,600 in very simple phenomenological terms. 1370 01:09:10,600 --> 01:09:13,939 Anybody knows what it means, "phenomenological"? 1371 01:09:13,939 --> 01:09:16,729 I am Greek, so I have a benefit of the language. 1372 01:09:22,410 --> 01:09:25,529 "Phenomenological" means based on observation. 1373 01:09:25,529 --> 01:09:28,649 It means we define this phenomenon 1374 01:09:28,649 --> 01:09:30,569 based on what we observe, but we don't 1375 01:09:30,569 --> 01:09:34,470 try to dig any deeper into the basic principles 1376 01:09:34,470 --> 01:09:36,149 behind this phenomenon. 1377 01:09:36,149 --> 01:09:38,290 You will see in a second what I mean. 1378 01:09:38,290 --> 01:09:41,779 Very well, we'll define absorption and refraction. 1379 01:09:41,779 --> 01:09:43,849 And what I want to emphasize, also, 1380 01:09:43,849 --> 01:09:46,430 is that this is not the only three types of interactions. 1381 01:09:46,430 --> 01:09:49,183 Light can do a lot of other things. 1382 01:09:49,183 --> 01:09:50,600 There's fluorescence, that you are 1383 01:09:50,600 --> 01:09:53,660 familiar if you go to nightclubs where they use ultraviolet, 1384 01:09:53,660 --> 01:09:54,260 right? 1385 01:09:54,260 --> 01:09:55,700 People look kind of funny. 1386 01:09:55,700 --> 01:09:58,220 That is fluorescence. 1387 01:09:58,220 --> 01:10:01,420 There is non-linear phenomena. 1388 01:10:01,420 --> 01:10:03,290 There's ionization that can happen. 1389 01:10:03,290 --> 01:10:05,360 So a lot of different things that can happen, 1390 01:10:05,360 --> 01:10:07,290 but I will not cover them in this class. 1391 01:10:07,290 --> 01:10:10,610 So as I say, they're outside the scope of our interest here. 1392 01:10:15,110 --> 01:10:18,140 Going on with this, let me define absorption first. 1393 01:10:18,140 --> 01:10:23,010 So from experience, we know that anything 1394 01:10:23,010 --> 01:10:26,700 that travels through a medium suffers losses. 1395 01:10:26,700 --> 01:10:28,140 Many of your mechanical engineers, 1396 01:10:28,140 --> 01:10:33,210 you know that if you have a mechanical disturbance 1397 01:10:33,210 --> 01:10:37,140 like sound propagating down the medium, at the exit, 1398 01:10:37,140 --> 01:10:39,543 you see less of the energy that you put in. 1399 01:10:39,543 --> 01:10:41,085 Some of you are electrical engineers. 1400 01:10:41,085 --> 01:10:44,310 You know that if you run current through a device, 1401 01:10:44,310 --> 01:10:46,230 typically, at the exit of the device, 1402 01:10:46,230 --> 01:10:49,990 you see less current or less electrical energy. 1403 01:10:49,990 --> 01:10:52,630 Typically, you see a voltage drop than the energy 1404 01:10:52,630 --> 01:10:54,260 that you put in. 1405 01:10:54,260 --> 01:10:57,270 So why does this happen? 1406 01:10:57,270 --> 01:10:58,670 Well, because of-- 1407 01:10:58,670 --> 01:10:59,170 Why? 1408 01:10:59,170 --> 01:10:59,962 Why does it happen? 1409 01:11:07,930 --> 01:11:08,430 Yes. 1410 01:11:13,300 --> 01:11:14,761 [LAUGHS] 1411 01:11:14,761 --> 01:11:16,222 AUDIENCE: [INAUDIBLE]. 1412 01:11:16,222 --> 01:11:17,650 GEORGE BARBASTATHIS: That's right. 1413 01:11:17,650 --> 01:11:19,770 It is conversion of energy to heat, right? 1414 01:11:19,770 --> 01:11:22,450 And that generally is undesirable unless-- 1415 01:11:22,450 --> 01:11:24,900 anyway, we seldom heat ourselves with-- well, 1416 01:11:24,900 --> 01:11:26,810 unless it's the sunlight on a day like this, 1417 01:11:26,810 --> 01:11:29,080 we appreciate the heating. 1418 01:11:29,080 --> 01:11:32,980 But in Singapore, generally, we don't appreciate the heating, 1419 01:11:32,980 --> 01:11:36,160 because the sunlight is too intense, typically, 1420 01:11:36,160 --> 01:11:38,702 to tolerate. 1421 01:11:38,702 --> 01:11:40,160 But yeah, the fact of the matter is 1422 01:11:40,160 --> 01:11:44,090 that there is ohmic losses, or dissipation, 1423 01:11:44,090 --> 01:11:48,680 like you very correctly said, that cause a decrease in power. 1424 01:11:48,680 --> 01:11:54,500 So the phenomenological law that describes this effect 1425 01:11:54,500 --> 01:11:58,430 is exponential in the length of propagation in matter. 1426 01:11:58,430 --> 01:12:00,800 So by "phenomenological," what I mean 1427 01:12:00,800 --> 01:12:03,370 is that I throw this equation at you, 1428 01:12:03,370 --> 01:12:05,870 but I haven't told you why, OK? 1429 01:12:05,870 --> 01:12:07,010 I will tell you why later. 1430 01:12:07,010 --> 01:12:09,710 When we do electromagnetics, I will justify 1431 01:12:09,710 --> 01:12:11,570 why this law comes about. 1432 01:12:11,570 --> 01:12:13,700 And strangely enough, it is called Beer's Law. 1433 01:12:13,700 --> 01:12:15,050 No, it's not pronounced "beer." 1434 01:12:15,050 --> 01:12:16,400 It's pronounced "bear." 1435 01:12:16,400 --> 01:12:17,470 This fellow was German. 1436 01:12:17,470 --> 01:12:22,050 But anyway-- and light does get absorbed by beer, actually. 1437 01:12:22,050 --> 01:12:25,680 And strangely enough, I did see a paper at a conference 1438 01:12:25,680 --> 01:12:29,070 once where someone was measuring the optical properties of beer. 1439 01:12:29,070 --> 01:12:31,340 And I'm not kidding, actually. 1440 01:12:31,340 --> 01:12:33,960 They had their project funded by I don't know whom, 1441 01:12:33,960 --> 01:12:37,998 to shoot laser beams through big containers of beer. 1442 01:12:37,998 --> 01:12:40,290 And then I don't know exactly what they were measuring, 1443 01:12:40,290 --> 01:12:42,720 but I thought it was a very cleverly conceived project. 1444 01:12:42,720 --> 01:12:45,180 Because after you finish the experiment, what do you do? 1445 01:12:45,180 --> 01:12:46,660 You drink the beer, right? 1446 01:12:46,660 --> 01:12:47,160 OK. 1447 01:12:50,360 --> 01:12:55,490 So I said that the output energy decays exponentially 1448 01:12:55,490 --> 01:12:57,620 as a function of the length of the medium. 1449 01:12:57,620 --> 01:12:59,570 The coefficient that goes in the exponent 1450 01:12:59,570 --> 01:13:02,090 is, again, very highly dependent on the material 1451 01:13:02,090 --> 01:13:03,590 that the light propagates. 1452 01:13:03,590 --> 01:13:06,380 Conductors-- like metals-- they tend 1453 01:13:06,380 --> 01:13:07,800 to have very high dissipation. 1454 01:13:07,800 --> 01:13:11,390 If you might propagate a few microns inside the metal, 1455 01:13:11,390 --> 01:13:12,770 the light is all lost. 1456 01:13:12,770 --> 01:13:14,810 It is all converted to heat. 1457 01:13:14,810 --> 01:13:17,732 So on the other hand, the electrics like glass, 1458 01:13:17,732 --> 01:13:19,190 they can have very low dissipation. 1459 01:13:19,190 --> 01:13:23,780 In fact, some materials, they use some special glasses 1460 01:13:23,780 --> 01:13:27,860 in optical fibers that they usually transmit light 1461 01:13:27,860 --> 01:13:29,552 over very long distances. 1462 01:13:29,552 --> 01:13:31,010 In these occasions, the dissipation 1463 01:13:31,010 --> 01:13:34,860 is in the order of a fraction of a dB per kilometer. 1464 01:13:34,860 --> 01:13:37,460 So it is I don't know how many orders of magnitude there, 1465 01:13:37,460 --> 01:13:41,540 around eight or nine orders of magnitude in the dissipation 1466 01:13:41,540 --> 01:13:42,890 coefficient. 1467 01:13:42,890 --> 01:13:45,020 And again, that depends on the way 1468 01:13:45,020 --> 01:13:46,760 light interacts with matter. 1469 01:13:46,760 --> 01:13:49,480 I will say a little bit more about that later. 1470 01:13:49,480 --> 01:13:53,645 But for now, again, take me to my word. 1471 01:13:53,645 --> 01:13:55,520 Never take anybody to their word, by the way. 1472 01:13:55,520 --> 01:13:58,705 But I think for reasons of organizing 1473 01:13:58,705 --> 01:14:00,080 the presentation of the material, 1474 01:14:00,080 --> 01:14:05,090 sometimes I will ask you to take my word for granted. 1475 01:14:05,090 --> 01:14:07,190 And usually, when I ask you to do that, 1476 01:14:07,190 --> 01:14:11,140 I will come back and justify myself perhaps a few lectures 1477 01:14:11,140 --> 01:14:13,600 later, or something like that. 1478 01:14:13,600 --> 01:14:16,960 OK, and the other thing I want to emphasize 1479 01:14:16,960 --> 01:14:20,740 is that dissipation or absorption depends strongly 1480 01:14:20,740 --> 01:14:21,910 on the wavelength. 1481 01:14:21,910 --> 01:14:24,490 And that, again, goes back to what we were saying before. 1482 01:14:24,490 --> 01:14:27,430 Different wavelengths carry different energy, 1483 01:14:27,430 --> 01:14:29,110 and different energies of the photons, 1484 01:14:29,110 --> 01:14:31,530 they will interact with the matter in different ways. 1485 01:14:31,530 --> 01:14:33,280 They might [INAUDIBLE] due to oscillation. 1486 01:14:33,280 --> 01:14:36,850 They might set it into dipole polarization. 1487 01:14:36,850 --> 01:14:40,620 They might set matter, they might ionize it-- whatever. 1488 01:14:40,620 --> 01:14:43,490 So depending on who happens, you get different behavior. 1489 01:14:43,490 --> 01:14:46,790 So this is the atmosphere. 1490 01:14:46,790 --> 01:14:49,140 The percent of transmission-- not exactly the alpha 1491 01:14:49,140 --> 01:14:54,210 coefficient, but a transmission, percent transmission throughout 1492 01:14:54,210 --> 01:14:55,380 a nominal length-- 1493 01:14:55,380 --> 01:15:01,030 I believe it is in the order of over a few meters-- 1494 01:15:01,030 --> 01:15:03,020 as a function of wavelength. 1495 01:15:03,020 --> 01:15:04,900 So we can see that it varies quite a bit 1496 01:15:04,900 --> 01:15:07,180 even within the visible range. 1497 01:15:07,180 --> 01:15:09,850 The atmosphere is not completely transparent. 1498 01:15:09,850 --> 01:15:12,340 It is a little bit less transparent 1499 01:15:12,340 --> 01:15:17,185 at blue wavelengths. 1500 01:15:17,185 --> 01:15:20,830 It becomes, then, almost transparent 1501 01:15:20,830 --> 01:15:22,530 at the longer wavelengths. 1502 01:15:22,530 --> 01:15:26,025 And then-- this is infrared now-- 1503 01:15:26,025 --> 01:15:27,400 in the infrared, you see you have 1504 01:15:27,400 --> 01:15:30,735 some very strong absorption. 1505 01:15:30,735 --> 01:15:32,360 The transmission coefficient goes down. 1506 01:15:32,360 --> 01:15:34,030 That means strong absorption here. 1507 01:15:34,030 --> 01:15:36,680 That actually has to do with molecular resonances. 1508 01:15:36,680 --> 01:15:40,270 And you can think of molecules as little mass spring damper 1509 01:15:40,270 --> 01:15:41,200 systems. 1510 01:15:41,200 --> 01:15:42,790 And the photon comes in and kicks them 1511 01:15:42,790 --> 01:15:44,868 so it sets them into oscillation. 1512 01:15:44,868 --> 01:15:46,660 When that happens, the energy of the photon 1513 01:15:46,660 --> 01:15:50,080 gets transformed resonantly into the molecule, 1514 01:15:50,080 --> 01:15:51,530 and then you get loss. 1515 01:15:51,530 --> 01:15:54,760 So in this case, it is a little bit more complicated 1516 01:15:54,760 --> 01:15:57,940 than heating, than simple heating. 1517 01:15:57,940 --> 01:15:59,680 But the net effect is still the same. 1518 01:15:59,680 --> 01:16:02,715 You still get heating from the motion of these molecules. 1519 01:16:02,715 --> 01:16:04,090 But anyway, that's the reason why 1520 01:16:04,090 --> 01:16:08,140 you get these strong absorption maxima over here. 1521 01:16:11,800 --> 01:16:15,190 What I really wanted to get to today so that we 1522 01:16:15,190 --> 01:16:17,110 can progress with geometrical optics 1523 01:16:17,110 --> 01:16:20,870 is the phenomenon of refraction. 1524 01:16:20,870 --> 01:16:23,880 So refraction, is-- is refers to, actually, 1525 01:16:23,880 --> 01:16:25,440 a rather strange thing that, again, I 1526 01:16:25,440 --> 01:16:28,470 will ask you to take for granted until we talk 1527 01:16:28,470 --> 01:16:30,910 in detail about polarization. 1528 01:16:30,910 --> 01:16:34,200 And that is the fact that the speed of light 1529 01:16:34,200 --> 01:16:37,500 changes when light enters the material. 1530 01:16:37,500 --> 01:16:40,110 In this case, we're talking primarily about dielectrics, 1531 01:16:40,110 --> 01:16:41,957 but it's also true for metals. 1532 01:16:41,957 --> 01:16:44,290 But of course, in metals, the light doesn't go very far. 1533 01:16:44,290 --> 01:16:47,830 So OK, the speed changes, but it doesn't go very far. 1534 01:16:47,830 --> 01:16:51,180 In dielectrics, the light can go quite far, 1535 01:16:51,180 --> 01:16:52,690 but its speed is different. 1536 01:16:52,690 --> 01:16:57,210 And again, phenomenologically-- without describing the physical 1537 01:16:57,210 --> 01:16:59,710 origins of why-- 1538 01:16:59,710 --> 01:17:02,260 the speed is, of course, reduced, 1539 01:17:02,260 --> 01:17:04,150 and it's used by a constant that is 1540 01:17:04,150 --> 01:17:07,540 known as index of refraction, or refractive index. 1541 01:17:07,540 --> 01:17:13,900 And most books use the symbol n to denote it. 1542 01:17:13,900 --> 01:17:17,650 And the value of n can value a lot. 1543 01:17:17,650 --> 01:17:21,400 In a vacuum, n equals exactly 1. 1544 01:17:21,400 --> 01:17:24,870 So the speed of light in vacuum equals exactly c. 1545 01:17:24,870 --> 01:17:28,600 In air, it is close to 1, within two significant digits. 1546 01:17:28,600 --> 01:17:32,260 It's maybe 1.005 or something like that. 1547 01:17:32,260 --> 01:17:34,790 And it depends also on the temperature, the pressure, 1548 01:17:34,790 --> 01:17:38,700 a number of different properties over the air, 1549 01:17:38,700 --> 01:17:41,970 as we'll see again later. 1550 01:17:41,970 --> 01:17:44,220 And then, typical dielectrics that we see 1551 01:17:44,220 --> 01:17:45,750 are water, of course. 1552 01:17:45,750 --> 01:17:48,840 So then, why is it the water interesting? 1553 01:17:48,840 --> 01:17:51,120 Well, because-- well, water. 1554 01:17:51,120 --> 01:17:54,110 But also because our bodies are composed mostly of water. 1555 01:17:54,110 --> 01:17:57,900 Our tissue is approximately 70% or 75% water. 1556 01:17:57,900 --> 01:18:00,720 So light index of refraction in a body 1557 01:18:00,720 --> 01:18:04,050 is also equal to the same quantity, 1.3. 1558 01:18:04,050 --> 01:18:07,140 Actually, this would be 1.33, if you really 1559 01:18:07,140 --> 01:18:08,750 want to be more accurate. 1560 01:18:08,750 --> 01:18:11,640 And glass-- so glass is used in pretty much 1561 01:18:11,640 --> 01:18:14,880 every optical instrument for visible wavelengths. 1562 01:18:14,880 --> 01:18:16,470 So in glass, the index of refraction 1563 01:18:16,470 --> 01:18:21,390 is approximately 1.5. 1564 01:18:21,390 --> 01:18:24,810 OK what does this mean now, the speed of light changes? 1565 01:18:24,810 --> 01:18:28,490 Another way to say it is that the wavelength of the light 1566 01:18:28,490 --> 01:18:29,320 changes. 1567 01:18:29,320 --> 01:18:32,750 And this is actually a more proper way 1568 01:18:32,750 --> 01:18:35,030 to think of the phenomenon. 1569 01:18:35,030 --> 01:18:37,310 When we'll do electromagnetics, we'll 1570 01:18:37,310 --> 01:18:40,850 see that the change in speed is actually 1571 01:18:40,850 --> 01:18:44,050 derived from that observation. 1572 01:18:44,050 --> 01:18:49,940 And the way the wavelength changes is it becomes shorter. 1573 01:18:49,940 --> 01:18:53,240 So if you have a light happily propagating in free space, 1574 01:18:53,240 --> 01:18:54,710 and then, all of a sudden, there's 1575 01:18:54,710 --> 01:18:58,850 an abrupt interface and light enters a dielectric, 1576 01:18:58,850 --> 01:19:01,048 the wavelengths becomes shorter. 1577 01:19:01,048 --> 01:19:02,090 Now, what does that mean? 1578 01:19:02,090 --> 01:19:05,680 Does this mean that, for example, if I have red light, 1579 01:19:05,680 --> 01:19:12,050 and the red light goes into glass, the light becomes green? 1580 01:19:12,050 --> 01:19:14,980 That's actually not what we observe, right? 1581 01:19:14,980 --> 01:19:21,040 if you observe, many of you have seen, 1582 01:19:21,040 --> 01:19:23,140 if you put a yellow pencil in glass, 1583 01:19:23,140 --> 01:19:24,310 the pencil remains yellow. 1584 01:19:24,310 --> 01:19:27,180 It does not turn blue, right? 1585 01:19:27,180 --> 01:19:30,650 So what is a possible-- does anybody know the explanation? 1586 01:19:30,650 --> 01:19:32,315 Yeah. 1587 01:19:32,315 --> 01:19:33,940 AUDIENCE: The frequency stays the same. 1588 01:19:33,940 --> 01:19:36,835 So if you see the frequency as it comes out, 1589 01:19:36,835 --> 01:19:39,210 it's just going to be affecting pretty much [INAUDIBLE].. 1590 01:19:39,210 --> 01:19:40,627 GEORGE BARBASTATHIS: That's right. 1591 01:19:42,850 --> 01:19:45,940 So very correctly, he said that the frequency of the light 1592 01:19:45,940 --> 01:19:47,350 remains the same. 1593 01:19:47,350 --> 01:19:50,320 Anybody want to guess why the frequency of the light 1594 01:19:50,320 --> 01:19:55,600 might remain the same but the wavelength can change? 1595 01:20:03,140 --> 01:20:04,307 AUDIENCE: The speed changes. 1596 01:20:04,307 --> 01:20:05,723 GEORGE BARBASTATHIS: That's right. 1597 01:20:05,723 --> 01:20:06,588 The speed, yes. 1598 01:20:10,046 --> 01:20:10,750 That's right. 1599 01:20:10,750 --> 01:20:12,840 So both of you are right. 1600 01:20:12,840 --> 01:20:15,810 So first of all, they can change simultaneously, 1601 01:20:15,810 --> 01:20:19,440 the wavelength and the speed, because of this equation. 1602 01:20:19,440 --> 01:20:21,950 We said that the speed of light-- 1603 01:20:21,950 --> 01:20:26,720 I mean the speed of light in vacuum, or in general-- 1604 01:20:26,720 --> 01:20:31,410 well, in vacuum, it is related to the frequency 1605 01:20:31,410 --> 01:20:33,900 of the wavelength by this equation over here. 1606 01:20:33,900 --> 01:20:37,860 Well, you can then divide the two sides of the equation by n, 1607 01:20:37,860 --> 01:20:39,787 and the question remains the same. 1608 01:20:39,787 --> 01:20:40,995 But that's not very physical. 1609 01:20:40,995 --> 01:20:42,352 I did a mathematical trick. 1610 01:20:42,352 --> 01:20:43,560 What the hell does that mean? 1611 01:20:43,560 --> 01:20:45,020 I divided both sides by n. 1612 01:20:48,212 --> 01:20:50,420 That doesn't have to be correct, and this is, indeed, 1613 01:20:50,420 --> 01:20:54,910 the dispersion relation in a dielectrical material. 1614 01:20:54,910 --> 01:20:57,820 But you don't really know, which one should you divide? 1615 01:20:57,820 --> 01:20:59,770 Should you divide the wavelength by n, 1616 01:20:59,770 --> 01:21:02,200 or should you divide the frequency by n? 1617 01:21:02,200 --> 01:21:04,840 Or maybe divide both by square root n? 1618 01:21:04,840 --> 01:21:06,530 All of these are possibilities. 1619 01:21:06,530 --> 01:21:10,660 So the physical argument that allows you to decide 1620 01:21:10,660 --> 01:21:12,410 whether to divide is what-- 1621 01:21:12,410 --> 01:21:13,600 I'm sorry, your name? 1622 01:21:13,600 --> 01:21:14,020 AUDIENCE: Uh, Liz. 1623 01:21:14,020 --> 01:21:14,950 GEORGE BARBASTATHIS: What Alice-- 1624 01:21:14,950 --> 01:21:15,648 Alice, right? 1625 01:21:15,648 --> 01:21:16,440 AUDIENCE: Just Liz. 1626 01:21:16,440 --> 01:21:17,940 GEORGE BARBASTATHIS: Liz, I'm sorry. 1627 01:21:17,940 --> 01:21:21,740 So the physical argument is what Liz just said, 1628 01:21:21,740 --> 01:21:26,950 which is that the energy of the photon cannot change. 1629 01:21:26,950 --> 01:21:29,650 Because the photon-- well, I haven't said it yet, 1630 01:21:29,650 --> 01:21:34,110 but the photon is a fundamental quantum mechanical particle. 1631 01:21:34,110 --> 01:21:35,920 It cannot be divided-- 1632 01:21:35,920 --> 01:21:39,310 well, it can be divided in some special cases. 1633 01:21:39,310 --> 01:21:43,120 But in the approximation that we deal with here, 1634 01:21:43,120 --> 01:21:45,860 the photon must maintain its energy. 1635 01:21:45,860 --> 01:21:47,860 So therefore, the frequency of the photon 1636 01:21:47,860 --> 01:21:49,640 must remain the same. 1637 01:21:49,640 --> 01:21:53,890 New, the temporal frequency is conserved. 1638 01:21:53,890 --> 01:21:56,890 So if the wavelength changes because light entered 1639 01:21:56,890 --> 01:21:59,290 into matter, then the velocity must 1640 01:21:59,290 --> 01:22:04,278 change to compensate in the dispersion relationship. 1641 01:22:04,278 --> 01:22:08,590 OK, in our context here, the only thing 1642 01:22:08,590 --> 01:22:13,617 that can happen to the photon is it can disappear. 1643 01:22:13,617 --> 01:22:14,950 And it doesn't really disappear. 1644 01:22:14,950 --> 01:22:16,840 It gets converted to heat, right? 1645 01:22:16,840 --> 01:22:19,270 So when the light hits the material, 1646 01:22:19,270 --> 01:22:22,980 it actually heats the material in discrete quanta. 1647 01:22:22,980 --> 01:22:27,300 Some of the photons that come from the light source, 1648 01:22:27,300 --> 01:22:31,620 discrete quantities that are equal to-- 1649 01:22:31,620 --> 01:22:33,810 you cannot see it over there because I erased it. 1650 01:22:33,810 --> 01:22:36,210 But discrete quantities of approximately 10 1651 01:22:36,210 --> 01:22:40,560 to the minus 19 joules, one of them at a time 1652 01:22:40,560 --> 01:22:43,800 can be converted to heat and heat the material. 1653 01:22:43,800 --> 01:22:48,330 But you cannot get 60% of the photon energy to go to heat 1654 01:22:48,330 --> 01:22:49,200 the material. 1655 01:22:49,200 --> 01:22:51,330 That's not the correct way to think about it. 1656 01:22:51,330 --> 01:22:54,540 If 60% of the energy goes into heating the material, 1657 01:22:54,540 --> 01:22:57,840 it means that 60% of individual photons 1658 01:22:57,840 --> 01:23:02,580 died and gave up their energy to the molecules of the material. 1659 01:23:02,580 --> 01:23:05,690 If you have a single photon arriving into a material, 1660 01:23:05,690 --> 01:23:08,690 it will either survive and go through impact, 1661 01:23:08,690 --> 01:23:10,820 or it will die and be converted to heat. 1662 01:23:10,820 --> 01:23:13,980 You cannot have 60% of an individual photon heating 1663 01:23:13,980 --> 01:23:15,280 the material. 1664 01:23:15,280 --> 01:23:17,220 OK, so because of this line of reasoning, 1665 01:23:17,220 --> 01:23:18,845 that really requires quantum mechanics. 1666 01:23:18,845 --> 01:23:22,160 So I cannot really justify it very well without spending 1667 01:23:22,160 --> 01:23:23,710 a semester of quantum mechanics. 1668 01:23:23,710 --> 01:23:25,640 But because of this line of reasoning, 1669 01:23:25,640 --> 01:23:28,460 the energy of the photon is invalid. 1670 01:23:28,460 --> 01:23:31,490 Therefore, nu is invariant. 1671 01:23:31,490 --> 01:23:34,540 So believe it or not, I have watched someone at a conference 1672 01:23:34,540 --> 01:23:37,473 stand up and say, well, doesn't the light really become green? 1673 01:23:37,473 --> 01:23:38,890 And that was an optics conference, 1674 01:23:38,890 --> 01:23:40,550 so it was very embarrassing. 1675 01:23:40,550 --> 01:23:42,850 But it's very useful to remember. 1676 01:23:42,850 --> 01:23:50,120 No, light does not become green when it enters glass. 1677 01:23:50,120 --> 01:23:52,875 And in any case, your eyes respond to the energy 1678 01:23:52,875 --> 01:23:53,750 of the photon, right? 1679 01:23:53,750 --> 01:23:57,950 Because-- well, I haven't said how your eyes perceive color 1680 01:23:57,950 --> 01:23:59,480 yet, but they respond to the energy. 1681 01:23:59,480 --> 01:24:01,605 So you still perceive it as red, because the energy 1682 01:24:01,605 --> 01:24:06,570 of the photon is still red. 1683 01:24:06,570 --> 01:24:11,030 OK, so having said that now, having 1684 01:24:11,030 --> 01:24:13,910 said that the index of refraction 1685 01:24:13,910 --> 01:24:17,060 is a property of the material, I can conceive of materials 1686 01:24:17,060 --> 01:24:21,207 where the index of refraction is a function of position. 1687 01:24:21,207 --> 01:24:22,290 And if that was the case-- 1688 01:24:26,157 --> 01:24:27,615 the bad thing about any measures is 1689 01:24:27,615 --> 01:24:29,720 you have to wait for them to finish. 1690 01:24:29,720 --> 01:24:31,950 OK, so you can conceive materials 1691 01:24:31,950 --> 01:24:34,140 where the index of refraction is variable. 1692 01:24:34,140 --> 01:24:36,780 So the example I gave before is the air, where, 1693 01:24:36,780 --> 01:24:40,480 because of temperature, pressure, and so on, 1694 01:24:40,480 --> 01:24:41,830 the index changes. 1695 01:24:41,830 --> 01:24:43,540 So if the index is functional position, 1696 01:24:43,540 --> 01:24:46,805 you can define a quantity that is called the optical path 1697 01:24:46,805 --> 01:24:47,305 length. 1698 01:24:47,305 --> 01:24:50,430 So if you follow the trajectory of the ray-- 1699 01:24:50,430 --> 01:24:53,580 so here is the ray, and that is its trajectory-- 1700 01:24:53,580 --> 01:24:59,650 you can integrate the index of refraction 1701 01:24:59,650 --> 01:25:03,190 in small, individual segments as the light propagates 1702 01:25:03,190 --> 01:25:06,450 along the ray. 1703 01:25:06,450 --> 01:25:09,210 So the basic principle that I would 1704 01:25:09,210 --> 01:25:12,810 like you to carry with you when you leave this class today 1705 01:25:12,810 --> 01:25:16,140 is that the basic law that covers 1706 01:25:16,140 --> 01:25:20,780 light propagation in the ray description 1707 01:25:20,780 --> 01:25:22,950 is that this quantity, the optical path, 1708 01:25:22,950 --> 01:25:23,850 must be preserved-- 1709 01:25:23,850 --> 01:25:25,963 I'm sorry, it must be minimized. 1710 01:25:25,963 --> 01:25:27,380 Of course, it has to be preserved. 1711 01:25:27,380 --> 01:25:29,475 It also has to be minimized. 1712 01:25:29,475 --> 01:25:31,350 So if you have different paths-- for example, 1713 01:25:31,350 --> 01:25:35,480 if you compare the path gamma and the path gamma prime-- 1714 01:25:35,480 --> 01:25:40,510 the light will take the path where this quantity is minimal, 1715 01:25:40,510 --> 01:25:41,415 OK? 1716 01:25:41,415 --> 01:25:43,040 Now, that sounds very abstract, I know, 1717 01:25:43,040 --> 01:25:45,650 but I will make it more specific with examples. 1718 01:25:45,650 --> 01:25:47,990 For those of you who are mechanical engineers-- or, more 1719 01:25:47,990 --> 01:25:50,030 likely, applied mechanicians-- this 1720 01:25:50,030 --> 01:25:51,710 is reminiscent of another principle 1721 01:25:51,710 --> 01:25:55,010 that you may have learned in your Lagrangian mechanics. 1722 01:25:55,010 --> 01:25:58,790 You can make the same, the exact same arguments 1723 01:25:58,790 --> 01:26:02,510 about particles moving in a gravitational field. 1724 01:26:02,510 --> 01:26:04,670 Particles moving in-- that's the reason 1725 01:26:04,670 --> 01:26:07,660 why stars rotate around the sun, why 1726 01:26:07,660 --> 01:26:09,110 they have elliptical trajectories, 1727 01:26:09,110 --> 01:26:11,140 and so on, and so forth-- is because they also 1728 01:26:11,140 --> 01:26:16,200 obey a minimum path principle. 1729 01:26:16,200 --> 01:26:21,320 And well, let's see it in action here. 1730 01:26:21,320 --> 01:26:23,590 So we apply this principle-- we'll 1731 01:26:23,590 --> 01:26:25,600 apply it in several occasions during the class, 1732 01:26:25,600 --> 01:26:29,290 but today, I would like to apply to discover 1733 01:26:29,290 --> 01:26:31,570 what happens to light when it arrives 1734 01:26:31,570 --> 01:26:34,490 at an interface between two dialectics. 1735 01:26:34,490 --> 01:26:38,058 So on the left, you have one dielectric-- say air-- 1736 01:26:38,058 --> 01:26:39,850 and on the right-hand side of an interface, 1737 01:26:39,850 --> 01:26:42,705 you have another dielectric-- say glass. 1738 01:26:42,705 --> 01:26:44,080 So what will happen to the light? 1739 01:26:44,080 --> 01:26:46,180 Well, two things will happen. 1740 01:26:46,180 --> 01:26:48,250 Some fraction of the light energy-- that is, 1741 01:26:48,250 --> 01:26:52,060 some fraction of individual photons-- 1742 01:26:52,060 --> 01:26:54,080 will be reflected. 1743 01:26:54,080 --> 01:26:59,440 And some other fraction of the light will enter the interface, 1744 01:26:59,440 --> 01:27:02,080 but it might enter at an angle that 1745 01:27:02,080 --> 01:27:04,240 is different than the angle of arrival. 1746 01:27:07,710 --> 01:27:12,120 That portion of light that goes in, we call it refracted. 1747 01:27:12,120 --> 01:27:14,370 So this is the refracted portion of the light. 1748 01:27:14,370 --> 01:27:16,710 It's a little bit confusing, because the two terms 1749 01:27:16,710 --> 01:27:19,020 are the same except for two letters. 1750 01:27:19,020 --> 01:27:21,690 So I hope you can sort of recapture the difference. 1751 01:27:21,690 --> 01:27:26,010 One is reflected, and the other is refracted. 1752 01:27:26,010 --> 01:27:28,750 So the question is, what is the direction that these rays 1753 01:27:28,750 --> 01:27:31,040 propagate at the interface? 1754 01:27:31,040 --> 01:27:34,810 So we will invoke the minimal path principle for that. 1755 01:27:34,810 --> 01:27:36,750 So consider, first, reflection. 1756 01:27:36,750 --> 01:27:38,220 And what I'm about to say applies 1757 01:27:38,220 --> 01:27:42,600 to the electric interface just as well as a mirror, a metal 1758 01:27:42,600 --> 01:27:45,080 or metallic mirror. 1759 01:27:45,080 --> 01:27:46,910 So the minimum path principle says 1760 01:27:46,910 --> 01:27:49,850 that the light must be reflected symmetrically. 1761 01:27:49,850 --> 01:27:54,200 So the reflected ray makes the same angle 1762 01:27:54,200 --> 01:27:57,078 with the normal as the incident ray, because that's 1763 01:27:57,078 --> 01:27:58,120 the minimum path, really. 1764 01:27:58,120 --> 01:28:04,140 If you force the light to go to a different path-- 1765 01:28:04,140 --> 01:28:06,308 for example, this way-- 1766 01:28:06,308 --> 01:28:08,850 then you can see very easily, it is a very simple calculation 1767 01:28:08,850 --> 01:28:16,192 to show that P, O, tilde p-prime is longer than P, O, P, OK? 1768 01:28:16,192 --> 01:28:18,150 I will let you think about that on your selves. 1769 01:28:18,150 --> 01:28:21,390 You can very easily convince yourselves that this is true. 1770 01:28:21,390 --> 01:28:25,170 And therefore, the light must follow the symmetric path. 1771 01:28:25,170 --> 01:28:26,850 So this is rule number one. 1772 01:28:26,850 --> 01:28:29,660 Let me skip the next slide. 1773 01:28:29,660 --> 01:28:32,980 I'll skip a little bit, and then I'll come back to this later. 1774 01:28:32,980 --> 01:28:35,010 But I want to first say something else. 1775 01:28:44,690 --> 01:28:47,120 OK. 1776 01:28:47,120 --> 01:28:49,150 When we think about the law of-- 1777 01:28:49,150 --> 01:28:52,070 let's say we think about the refracted light. 1778 01:28:52,070 --> 01:28:54,220 The [INAUDIBLE] is the medium. 1779 01:28:54,220 --> 01:28:56,680 OK, so the first thing we need to do in order 1780 01:28:56,680 --> 01:28:59,938 to complete this calculation is to define two points 1781 01:28:59,938 --> 01:29:00,480 from the ray. 1782 01:29:00,480 --> 01:29:03,550 So let's say you have point p on the incident ray 1783 01:29:03,550 --> 01:29:06,460 and then point p-prime on the refracted ray. 1784 01:29:09,250 --> 01:29:12,560 So let's compute this quantity of the optical path. 1785 01:29:12,560 --> 01:29:15,910 So the optical part equals the index 1786 01:29:15,910 --> 01:29:18,460 of refraction on the leg on the left, 1787 01:29:18,460 --> 01:29:21,790 times the length of the day from p 1788 01:29:21,790 --> 01:29:25,525 to the interface, and then the index of refraction 1789 01:29:25,525 --> 01:29:28,270 in n prime on the right-hand side, 1790 01:29:28,270 --> 01:29:32,430 times the length of the ray from the interface to p prime. 1791 01:29:32,430 --> 01:29:35,280 So this, I will repeat what I have on the slide. 1792 01:29:35,280 --> 01:29:37,072 I will repeat it on the blackboard. 1793 01:29:41,010 --> 01:29:45,250 So you have n times the hypotenuse. 1794 01:29:45,250 --> 01:29:47,805 So my notation here is x for this distance, 1795 01:29:47,805 --> 01:29:49,980 z for this distance. 1796 01:29:49,980 --> 01:29:58,350 So that's the hypotenuse plus n prime, 1797 01:29:58,350 --> 01:30:01,600 times the other hypotenuse. 1798 01:30:01,600 --> 01:30:05,340 So this other hypotenuse, if I call h the vertical distance 1799 01:30:05,340 --> 01:30:08,160 between the two points, simple geometry 1800 01:30:08,160 --> 01:30:10,300 solves that this other hypotenuse 1801 01:30:10,300 --> 01:30:11,660 is something like that. 1802 01:30:19,610 --> 01:30:27,570 OK, so the question here-- 1803 01:30:27,570 --> 01:30:28,860 how do I pose the question? 1804 01:30:28,860 --> 01:30:29,960 What is the unknown here? 1805 01:30:38,700 --> 01:30:42,930 What have I left unspecified? 1806 01:30:42,930 --> 01:30:45,170 Let me start with what I have already specified. 1807 01:30:45,170 --> 01:30:47,810 I specified theta, the angle of incidence. 1808 01:30:47,810 --> 01:30:51,060 I specified the two points, p and p prime. 1809 01:30:51,060 --> 01:30:55,225 And I specified the vertical distance h. 1810 01:30:55,225 --> 01:30:56,850 And also, I should say that the z prime 1811 01:30:56,850 --> 01:31:01,750 is also specified, because z and z prime are specified because, 1812 01:31:01,750 --> 01:31:04,560 OK, I have specified the coordinates of p and p prime. 1813 01:31:04,560 --> 01:31:05,130 What is left? 1814 01:31:08,080 --> 01:31:14,178 theta prime, or another quantity that is also left unspecified? 1815 01:31:18,760 --> 01:31:21,150 x and x prime, right? 1816 01:31:21,150 --> 01:31:23,120 Because the ray might go like this. 1817 01:31:27,730 --> 01:31:30,910 All we know is that the line starts at p 1818 01:31:30,910 --> 01:31:32,740 and ends at p prime. 1819 01:31:32,740 --> 01:31:33,880 It can go like this. 1820 01:31:33,880 --> 01:31:35,200 It can go like this. 1821 01:31:35,200 --> 01:31:36,420 It can go like this. 1822 01:31:36,420 --> 01:31:37,990 It can go like this, right? 1823 01:31:37,990 --> 01:31:39,830 Which is the case? 1824 01:31:39,830 --> 01:31:41,860 OK, so therefore, each one of those 1825 01:31:41,860 --> 01:31:43,900 has a different value of x. 1826 01:31:43,900 --> 01:31:46,850 So how do we find x? 1827 01:31:46,850 --> 01:31:52,520 Well, Fermat says that light must minimize this quantity. 1828 01:31:52,520 --> 01:31:55,120 The quantity that I wrote on the blackboard 1829 01:31:55,120 --> 01:31:59,540 and on the slide, Fermat says that it has to be minimized. 1830 01:31:59,540 --> 01:32:03,320 And OPL, by the way, stands for Optical Path Length. 1831 01:32:03,320 --> 01:32:05,070 So to minimize it, I have to compute 1832 01:32:05,070 --> 01:32:10,400 the derivative of this quantity with respect to my unknown. 1833 01:32:10,400 --> 01:32:13,813 I manage to have only one unknown of this quantity. 1834 01:32:13,813 --> 01:32:15,980 To find this unknown, I'd better take the derivative 1835 01:32:15,980 --> 01:32:17,190 and set it to 0. 1836 01:32:17,190 --> 01:32:22,510 So if I take the derivative, I will get n times-- 1837 01:32:22,510 --> 01:32:23,590 what is the derivative? 1838 01:32:23,590 --> 01:32:24,090 Someone? 1839 01:32:29,378 --> 01:32:31,170 I guess I've had more coffee than everyone, 1840 01:32:31,170 --> 01:32:32,825 so I can still do the derivative. 1841 01:32:32,825 --> 01:32:35,960 So it is nx divided by the square root, 1842 01:32:35,960 --> 01:32:42,600 minus n prime h minus x, divided by the other square root, OK? 1843 01:32:45,590 --> 01:32:47,420 OK, give me, now, a simple observation that 1844 01:32:47,420 --> 01:32:48,670 solves the problem right away. 1845 01:32:57,850 --> 01:32:58,880 That's right. 1846 01:32:58,880 --> 01:33:07,240 This quantity, x over the hypotenuse, 1847 01:33:07,240 --> 01:33:08,480 is the sign of this angle. 1848 01:33:08,480 --> 01:33:12,110 This angle is the same as this angle, right? 1849 01:33:12,110 --> 01:33:15,018 Therefore, this quantity is its sine. 1850 01:33:15,018 --> 01:33:16,310 And the same for the other one. 1851 01:33:16,310 --> 01:33:23,000 The other quantity over here is the sine of theta prime. 1852 01:33:23,000 --> 01:33:27,770 So if you substitute these quantities into the derivation, 1853 01:33:27,770 --> 01:33:32,490 then you find this relationship over here. 1854 01:33:32,490 --> 01:33:38,770 n times sine theta must equal n prime times sine theta prime. 1855 01:33:38,770 --> 01:33:42,600 And this is the law of refraction, also known 1856 01:33:42,600 --> 01:33:43,380 as Snell's Law. 1857 01:33:50,320 --> 01:33:53,560 So officially, I think, we're out of time. 1858 01:33:53,560 --> 01:33:56,940 But I can take a couple of very few-- 1859 01:33:56,940 --> 01:33:59,720 I should say very quick questions, 1860 01:33:59,720 --> 01:34:02,148 about that or about anything else. 1861 01:34:02,148 --> 01:34:04,320 Yes? 1862 01:34:04,320 --> 01:34:09,880 AUDIENCE: So how is it that you can assume p and p prime, 1863 01:34:09,880 --> 01:34:11,990 without knowing these other things? 1864 01:34:11,990 --> 01:34:13,365 GEORGE BARBASTATHIS: OK, so I was 1865 01:34:13,365 --> 01:34:15,443 hoping that you would ask that. 1866 01:34:15,443 --> 01:34:16,610 That's a very good question. 1867 01:34:16,610 --> 01:34:19,080 So the way this problem is solved 1868 01:34:19,080 --> 01:34:26,310 is as follows I take for granted that there is a light ray that 1869 01:34:26,310 --> 01:34:28,610 goes between p and p prime. 1870 01:34:28,610 --> 01:34:30,110 The reason I can take it for granted 1871 01:34:30,110 --> 01:34:32,340 is another very basic principle that says 1872 01:34:32,340 --> 01:34:35,040 that if I have a light source-- 1873 01:34:35,040 --> 01:34:40,430 say it's p-- then light propagates 1874 01:34:40,430 --> 01:34:43,460 in spherical bundles. 1875 01:34:43,460 --> 01:34:52,130 So I will actually have many, many rays coming from p. 1876 01:34:52,130 --> 01:34:57,090 And if I have another point, any point out here, p prime, 1877 01:34:57,090 --> 01:35:03,730 I will also have many, many rays arriving here 1878 01:35:03,730 --> 01:35:05,720 from the left-hand side. 1879 01:35:05,720 --> 01:35:09,420 One of these rays has come from p. 1880 01:35:09,420 --> 01:35:14,280 So the question is, how can you connect these rays? 1881 01:35:14,280 --> 01:35:18,450 Well, the principle that allows you to connect them 1882 01:35:18,450 --> 01:35:21,180 is the minimum path principle. 1883 01:35:21,180 --> 01:35:22,860 The problem can become impossible. 1884 01:35:22,860 --> 01:35:25,680 I will show you examples later where, in fact, you 1885 01:35:25,680 --> 01:35:29,723 might have a case where no rays reach p prime. 1886 01:35:29,723 --> 01:35:30,640 You can see that here. 1887 01:35:30,640 --> 01:35:32,970 If I play with the numbers and make one of these-- 1888 01:35:32,970 --> 01:35:35,940 if I play with the numbers so that one of the sines 1889 01:35:35,940 --> 01:35:39,320 becomes bigger than 1, then the problem becomes impossible, 1890 01:35:39,320 --> 01:35:39,820 right? 1891 01:35:39,820 --> 01:35:42,210 So what it means is that light never makes it there. 1892 01:35:45,760 --> 01:35:48,940 So this way of thinking is very typical 1893 01:35:48,940 --> 01:35:53,680 when we deal with minimization principles like Fermat 1894 01:35:53,680 --> 01:35:56,800 and Lagrangian principles in mechanics. 1895 01:35:56,800 --> 01:35:59,830 We assume that our particle, or our system, 1896 01:35:59,830 --> 01:36:03,270 or whatever has followed a trajectory that 1897 01:36:03,270 --> 01:36:06,880 connects an initial point in the space with the final point 1898 01:36:06,880 --> 01:36:08,100 in the space. 1899 01:36:08,100 --> 01:36:10,480 And then we try to find a trajectory that minimizes 1900 01:36:10,480 --> 01:36:13,450 the part between the two points, whether it is optical path 1901 01:36:13,450 --> 01:36:17,800 length, or Lagrangian in mechanics, 1902 01:36:17,800 --> 01:36:20,380 or a lot of other different contexts 1903 01:36:20,380 --> 01:36:22,660 where the same thinking applied. 1904 01:36:29,760 --> 01:36:31,057 Any other questions? 1905 01:36:34,800 --> 01:36:36,250 OK, so I will see you-- 1906 01:36:36,250 --> 01:36:39,100 I will see you all in Singapore next week, 1907 01:36:39,100 --> 01:36:43,500 and I will see you all on video next week.