1 00:00:00,570 --> 00:00:05,640 PROFESSOR: Einstein's argument, we consider again our atoms. 2 00:00:05,640 --> 00:00:08,900 And this time we're going to use the thermal equilibrium. 3 00:00:08,900 --> 00:00:14,460 We're going to really make use of that fact. 4 00:00:14,460 --> 00:00:20,870 So, again, we have level b and level a. 5 00:00:20,870 --> 00:00:23,280 And this is Einstein's argument. 6 00:00:33,570 --> 00:00:37,310 And we're going to have no populations. 7 00:00:37,310 --> 00:00:41,450 If we discuss equilibrium, we can consider a system in a box. 8 00:00:41,450 --> 00:00:44,300 And there's a few billion atoms. 9 00:00:44,300 --> 00:00:47,150 And there's some atoms whose electron 10 00:00:47,150 --> 00:00:49,160 is going to be in state b. 11 00:00:49,160 --> 00:00:52,880 Some atoms whose electrons are going to be in state a. 12 00:00:52,880 --> 00:00:59,270 Let's call these numbers Nb and Na. 13 00:00:59,270 --> 00:01:11,090 And we also have photons at temperature T 14 00:01:11,090 --> 00:01:20,440 and have a beta parameter 1 over the Boltzmann constant times T. 15 00:01:20,440 --> 00:01:23,450 So this is the process we're going to consider. 16 00:01:23,450 --> 00:01:26,335 So what's going to happen? 17 00:01:28,910 --> 00:01:34,460 If we came up from the edition that we've built from 806, 18 00:01:34,460 --> 00:01:36,320 we would think, OK, there's going 19 00:01:36,320 --> 00:01:42,800 to be absorption process and stimulated emission process. 20 00:01:42,800 --> 00:01:44,770 And between the two, they're going 21 00:01:44,770 --> 00:01:47,060 to be able to reach equilibrium. 22 00:01:47,060 --> 00:01:52,800 We don't believe this is not a process that can equilibrate. 23 00:01:52,800 --> 00:01:54,760 So this would be our intuition. 24 00:01:54,760 --> 00:01:58,640 The intuition for people that lived 25 00:01:58,640 --> 00:02:04,250 at the beginning of last century was rather different. 26 00:02:04,250 --> 00:02:08,810 They felt that there would be absorption process 27 00:02:08,810 --> 00:02:12,590 and there was spontaneous emission. 28 00:02:12,590 --> 00:02:16,010 The thing that you probably intuitively would think, 29 00:02:16,010 --> 00:02:20,000 if you are at a high level, you spontaneously decay. 30 00:02:20,000 --> 00:02:23,330 So the thing that was not known to them 31 00:02:23,330 --> 00:02:26,660 was this stimulated emission. 32 00:02:26,660 --> 00:02:31,700 That is what Einstein is credited for discovering here. 33 00:02:31,700 --> 00:02:35,090 People felt, and I think the paper finds that makes clear 34 00:02:35,090 --> 00:02:37,460 that the intuition, is that you have 35 00:02:37,460 --> 00:02:41,990 spontaneous emission, in which spontaneously 36 00:02:41,990 --> 00:02:47,570 by some kind of instability, the higher state goes 37 00:02:47,570 --> 00:02:48,890 to the bottom. 38 00:02:48,890 --> 00:02:51,860 And you have absorption. 39 00:02:51,860 --> 00:02:54,410 But then Einstein figured out that you couldn't achieve 40 00:02:54,410 --> 00:02:56,222 equilibrium in that way. 41 00:02:56,222 --> 00:02:57,680 Well, the way we're going to do it, 42 00:02:57,680 --> 00:03:00,650 we're going to put the two things we know-- 43 00:03:00,650 --> 00:03:03,440 the absorption and the stimulated 44 00:03:03,440 --> 00:03:06,380 emission-- and see that we don't get it 45 00:03:06,380 --> 00:03:08,450 to work, the equilibrium. 46 00:03:08,450 --> 00:03:14,210 But then when we add the spontaneous emission, we will. 47 00:03:14,210 --> 00:03:18,260 And as it turns out, the spontaneous emission 48 00:03:18,260 --> 00:03:21,080 is a little harder to calculate. 49 00:03:21,080 --> 00:03:24,500 If we were to do it in 806, it probably 50 00:03:24,500 --> 00:03:28,120 would be a matter of two lectures involving 51 00:03:28,120 --> 00:03:29,470 an electromagnetic field. 52 00:03:29,470 --> 00:03:31,370 So we will not do it. 53 00:03:31,370 --> 00:03:36,140 But the good thing is that Einstein's argument tells you 54 00:03:36,140 --> 00:03:40,160 the speed of spontaneous emission, the rate 55 00:03:40,160 --> 00:03:43,310 of spontaneous emission, in terms 56 00:03:43,310 --> 00:03:47,660 of this rate of stimulated emission or absorption. 57 00:03:47,660 --> 00:03:50,300 So it does the calculation for you 58 00:03:50,300 --> 00:03:54,750 by some other thermodynamical means. 59 00:03:54,750 --> 00:03:59,285 So we're going to use here three facts. 60 00:04:02,230 --> 00:04:03,580 One is that the-- 61 00:04:03,580 --> 00:04:10,960 three facts-- one is the populations are in equilibrium. 62 00:04:19,730 --> 00:04:26,430 So Na dot is they stop changing is equal to 0. 63 00:04:26,430 --> 00:04:29,690 And Nb dot is equal to 0. 64 00:04:29,690 --> 00:04:34,040 They don't stop changing because nothing happens. 65 00:04:34,040 --> 00:04:37,010 All the time there will be emission, 66 00:04:37,010 --> 00:04:38,450 and there will be absorption. 67 00:04:38,450 --> 00:04:42,020 But if you reach equilibrium, the number of atoms 68 00:04:42,020 --> 00:04:45,810 remain the same on every state. 69 00:04:45,810 --> 00:04:49,370 So that's our statement that the populations 70 00:04:49,370 --> 00:04:52,610 achieve equilibrium. 71 00:04:52,610 --> 00:04:58,040 The second statement is that the equilibrium is thermodynamical. 72 00:04:58,040 --> 00:05:02,510 So it's thermal equilibrium. 73 00:05:06,800 --> 00:05:14,540 That is Nb over Na, for example, is the Boltzmann factor e 74 00:05:14,540 --> 00:05:20,990 to the minus beta, Eb over e to the minus beta Ea. 75 00:05:20,990 --> 00:05:35,430 And this is equal to e to the minus beta h bar omega ba. 76 00:05:35,430 --> 00:05:39,600 You get e to the minus beta, eb minus ea. 77 00:05:39,600 --> 00:05:44,700 But eb minus ea is h bar omega ba. 78 00:05:44,700 --> 00:05:48,690 So that's thermal equilibrium. 79 00:05:48,690 --> 00:05:53,370 And the last thing that we need is 80 00:05:53,370 --> 00:05:55,590 a statement about the photons. 81 00:05:55,590 --> 00:05:58,860 What do they do when they have equilibrium? 82 00:05:58,860 --> 00:06:03,340 And that was known already due the work of Planck 83 00:06:03,340 --> 00:06:06,070 and others, black body equilibrium. 84 00:06:06,070 --> 00:06:09,510 So we need to know something about the thermal radiation. 85 00:06:17,500 --> 00:06:22,620 And the way one describes this is in terms of a function 86 00:06:22,620 --> 00:06:25,420 U of omega d omega. 87 00:06:25,420 --> 00:06:28,240 In the black body radiation, there 88 00:06:28,240 --> 00:06:30,725 are at a given temperature, there 89 00:06:30,725 --> 00:06:32,920 are photons with very little energy. 90 00:06:32,920 --> 00:06:36,280 There are some largest number of photons 91 00:06:36,280 --> 00:06:38,740 with some energy associated with temperature, 92 00:06:38,740 --> 00:06:39,790 and then it decays. 93 00:06:39,790 --> 00:06:43,040 So you have photons of all energy. 94 00:06:43,040 --> 00:06:47,290 So if you want a description of what's going on in black body 95 00:06:47,290 --> 00:06:51,730 radiation, you can consider the energy 96 00:06:51,730 --> 00:06:55,270 in the photons in the frequency range. 97 00:06:55,270 --> 00:06:57,490 But you even must be more precise. 98 00:06:57,490 --> 00:07:03,550 It is the energy per unit volume in a frequency range. 99 00:07:03,550 --> 00:07:07,740 Because if it's different, the energy of the black body 100 00:07:07,740 --> 00:07:10,600 cavities, this room or it's a little box. 101 00:07:10,600 --> 00:07:16,340 So it's an energy per volume per frequency range. 102 00:07:16,340 --> 00:07:18,085 And that's what this quantity is. 103 00:07:18,085 --> 00:07:20,220 So let me write it. 104 00:07:20,220 --> 00:07:41,450 Energy per unit volume in the frequency range dw. 105 00:07:41,450 --> 00:07:46,610 In other words, it's kind of a proxy for the number of photons 106 00:07:46,610 --> 00:07:47,270 available. 107 00:07:47,270 --> 00:07:51,950 All the photos have at some value of the frequency, 108 00:07:51,950 --> 00:07:53,030 of energy e omega. 109 00:07:53,030 --> 00:07:55,850 So if you know the energy, you basically 110 00:07:55,850 --> 00:08:01,550 are getting here the number of photons with frequency omega 111 00:08:01,550 --> 00:08:04,805 in that range per unit volume, all that stuff. 112 00:08:07,590 --> 00:08:11,750 So this has a formula. 113 00:08:11,750 --> 00:08:16,290 And the formula that was known to people 114 00:08:16,290 --> 00:08:25,680 was this quantities and then omega cube, d omega, over e 115 00:08:25,680 --> 00:08:30,230 to the beta h bar omega minus 1. 116 00:08:34,649 --> 00:08:40,390 So this is the basis of the calculation. 117 00:08:43,200 --> 00:08:44,070 What do we do? 118 00:08:44,070 --> 00:08:46,670 We have to consider the possible processes. 119 00:08:49,630 --> 00:08:54,120 OK, so our processes are absorption. 120 00:08:58,050 --> 00:09:02,700 And in this case, we go from a to b. 121 00:09:02,700 --> 00:09:10,320 And let's try to write a rate for them. 122 00:09:13,380 --> 00:09:17,700 So what would the rate depend on? 123 00:09:17,700 --> 00:09:22,060 Well, here's some little assumptions. 124 00:09:22,060 --> 00:09:26,890 Certainly, if you don't have particles in the a state, 125 00:09:26,890 --> 00:09:28,470 you cannot have this process. 126 00:09:28,470 --> 00:09:33,780 So this process, the total rate that we observe in the box 127 00:09:33,780 --> 00:09:35,820 will depend on an Na. 128 00:09:35,820 --> 00:09:38,760 The more particles you have in this state 129 00:09:38,760 --> 00:09:45,240 a, the larger the probability that you get the transitions, 130 00:09:45,240 --> 00:09:46,435 and the larger the rate. 131 00:09:49,900 --> 00:09:55,240 It will also be affected by the number of photons 132 00:09:55,240 --> 00:10:01,090 available at that frequency that can 133 00:10:01,090 --> 00:10:05,360 produce a transition in proportional to that. 134 00:10:05,360 --> 00:10:12,200 And finally, the quantity that our study of perturbation 135 00:10:12,200 --> 00:10:15,910 theory will tell us about, but at that time, 136 00:10:15,910 --> 00:10:23,380 finds that was not known, it's a transition coefficient, Bab, 137 00:10:23,380 --> 00:10:25,940 he called it. 138 00:10:25,940 --> 00:10:27,780 And this is the unknown one. 139 00:10:31,280 --> 00:10:32,890 And this is what we don't know. 140 00:10:32,890 --> 00:10:35,430 We know U. We assume we know Na. 141 00:10:35,430 --> 00:10:41,640 This is the transition rate per atom 142 00:10:41,640 --> 00:10:44,560 and then multiplied by the number of atoms. 143 00:10:44,560 --> 00:10:50,340 So this is transition rate per atom. 144 00:10:58,330 --> 00:11:05,750 Then we have the process of spontaneous emission. 145 00:11:05,750 --> 00:11:11,480 And then we will be another coefficient, Bba. 146 00:11:11,480 --> 00:11:15,230 And it would depend on the number of particles 147 00:11:15,230 --> 00:11:19,580 that are in the state b, because spontaneous emissions 148 00:11:19,580 --> 00:11:22,040 that transition from b to a. 149 00:11:24,710 --> 00:11:27,940 We call it-- oh, not spontaneous stimulated. 150 00:11:27,940 --> 00:11:29,870 I'm sorry-- stimulated emission. 151 00:11:33,450 --> 00:11:35,150 This is the one we're considering. 152 00:11:35,150 --> 00:11:37,790 It's stimulated by the radiation. 153 00:11:37,790 --> 00:11:40,670 So it's also proportional to the number 154 00:11:40,670 --> 00:11:44,960 of photons present and proportional 155 00:11:44,960 --> 00:11:47,210 to the number of atoms that can be 156 00:11:47,210 --> 00:11:54,470 convinced to do the transition times another coefficient, Bba. 157 00:11:54,470 --> 00:12:02,660 So this is, I think, what we in 806 would do. 158 00:12:02,660 --> 00:12:04,570 We would consider this two processes 159 00:12:04,570 --> 00:12:08,190 and attempt to make it work. 160 00:12:08,190 --> 00:12:10,116 And let's see what we get then. 161 00:12:14,680 --> 00:12:16,800 We're trying to get equilibrium. 162 00:12:16,800 --> 00:12:24,160 So we want the transitions to equilibrate and, therefore, 163 00:12:24,160 --> 00:12:28,490 the populations not to change. 164 00:12:28,490 --> 00:12:30,350 So let's look-- for example-- 165 00:12:30,350 --> 00:12:36,460 you could look at either one, but you can look at Nb dot. 166 00:12:36,460 --> 00:12:40,300 It should be 0. 167 00:12:40,300 --> 00:12:49,590 But it's equal to the rate of absorption 168 00:12:49,590 --> 00:12:56,800 minus the rate of stimulated emission. 169 00:13:02,430 --> 00:13:06,350 You see because the number of particles in b 170 00:13:06,350 --> 00:13:09,800 change because you get some new particles in state 171 00:13:09,800 --> 00:13:12,500 b due to the absorption process. 172 00:13:12,500 --> 00:13:14,840 And it happens with this rate. 173 00:13:14,840 --> 00:13:19,670 And you lose some particle because some atoms 174 00:13:19,670 --> 00:13:22,660 do the transition from the higher level to the lower 175 00:13:22,660 --> 00:13:23,910 level. 176 00:13:23,910 --> 00:13:26,060 So what is the rate of absorption? 177 00:13:26,060 --> 00:13:28,250 We have it here. 178 00:13:28,250 --> 00:13:37,946 It's this one, Bab U of omega ba Na. 179 00:13:37,946 --> 00:13:44,900 And this one is Bba, the same U of omega ba Nb. 180 00:13:47,550 --> 00:13:50,700 And we can factor the U out. 181 00:13:50,700 --> 00:13:53,900 And this is the wrong calculation, I must say, 182 00:13:53,900 --> 00:13:57,560 because we're missing that extra process that 183 00:13:57,560 --> 00:14:02,600 was intuitive to Einstein, but to us it's 184 00:14:02,600 --> 00:14:06,050 a little less clear-- 185 00:14:06,050 --> 00:14:10,700 Nb times U of omega ba. 186 00:14:16,000 --> 00:14:20,500 OK, I can do a one more little thing. 187 00:14:20,500 --> 00:14:21,970 I can factor an Na. 188 00:14:21,970 --> 00:14:35,330 And this becomes Bab minus Bba to the minus beta h bar omega 189 00:14:35,330 --> 00:14:41,020 Ba U of omega ba. 190 00:14:41,020 --> 00:14:50,140 OK, I use the ratio of Na over Nb being thermodynamical. 191 00:14:50,140 --> 00:14:56,080 So Nb over Na was used from point two to get this. 192 00:14:56,080 --> 00:14:57,930 And this should be equal to 0. 193 00:15:00,910 --> 00:15:04,270 But this equation can't be satisfied. 194 00:15:07,170 --> 00:15:08,840 What do you have here? 195 00:15:08,840 --> 00:15:12,730 You should be able to equilibrate at any temperature. 196 00:15:12,730 --> 00:15:15,820 On the other hand, what is our intuition 197 00:15:15,820 --> 00:15:20,320 about these quantities, Bab and Bba? 198 00:15:20,320 --> 00:15:22,690 They should be temperature independent. 199 00:15:22,690 --> 00:15:29,200 These are properties of the geometry of those states 200 00:15:29,200 --> 00:15:32,510 and the overlaps of the wave functions. 201 00:15:32,510 --> 00:15:35,350 These are atomic physics properties 202 00:15:35,350 --> 00:15:38,030 of the levels of the particles. 203 00:15:38,030 --> 00:15:40,590 We will calculate them. 204 00:15:40,590 --> 00:15:44,440 And here is the input of how many photons there 205 00:15:44,440 --> 00:15:46,480 are, how many atoms there are. 206 00:15:46,480 --> 00:15:49,300 And the number of photons certainly 207 00:15:49,300 --> 00:15:50,560 depend on the temperature. 208 00:15:50,560 --> 00:15:52,780 The number of atoms for equilibrium 209 00:15:52,780 --> 00:15:54,260 depend on the temperature. 210 00:15:54,260 --> 00:15:57,220 But this is a factor that says, well, 211 00:15:57,220 --> 00:16:01,210 how likely is the transition once you have a photon 212 00:16:01,210 --> 00:16:02,890 and once you have an atom? 213 00:16:02,890 --> 00:16:07,990 And that depends like we did for the ionization, calculated 214 00:16:07,990 --> 00:16:10,450 some matrix elements that are totally 215 00:16:10,450 --> 00:16:12,800 independent of temperature. 216 00:16:12,800 --> 00:16:17,830 So these numbers are totally independent of temperature. 217 00:16:17,830 --> 00:16:20,740 And we're asking this to be 0, which 218 00:16:20,740 --> 00:16:23,655 requires this factor to be 0. 219 00:16:23,655 --> 00:16:26,300 And this depends on temperature. 220 00:16:26,300 --> 00:16:31,510 So you cannot attain equilibrium with this way. 221 00:16:31,510 --> 00:16:43,600 So it's impossible to satisfy for all temperatures given 222 00:16:43,600 --> 00:16:48,990 that Bab and Bba are constants. 223 00:17:04,369 --> 00:17:06,589 So we're missing a process. 224 00:17:06,589 --> 00:17:12,700 This is the process that Einstein thought was intuitive, 225 00:17:12,700 --> 00:17:16,214 the process of spontaneous emission. 226 00:17:19,569 --> 00:17:24,490 So we add one more process. 227 00:17:24,490 --> 00:17:29,745 It's called spontaneous emission. 228 00:17:36,820 --> 00:17:40,795 And it's a process also from b to a. 229 00:17:45,373 --> 00:17:48,670 And it's going to have a rate. 230 00:17:48,670 --> 00:17:52,120 But it's not going to depend, that rate, 231 00:17:52,120 --> 00:17:55,570 on the number of photons, because it's happening 232 00:17:55,570 --> 00:17:57,940 independently of the photons. 233 00:17:57,940 --> 00:18:01,420 So we don't have this U factor. 234 00:18:01,420 --> 00:18:06,790 We do have the Nb because each of the b atoms 235 00:18:06,790 --> 00:18:09,160 can spontaneously decay. 236 00:18:09,160 --> 00:18:11,330 But we don't have the U factor. 237 00:18:14,880 --> 00:18:16,710 So what do we have? 238 00:18:16,710 --> 00:18:23,320 A rate, which is the term by a coefficient 239 00:18:23,320 --> 00:18:27,940 that Einstein called it a, that's why the name a and b 240 00:18:27,940 --> 00:18:32,440 coefficients of Einstein, a times and b. 241 00:18:35,490 --> 00:18:38,310 So that's the spontaneous emission rate 242 00:18:38,310 --> 00:18:42,510 per atom multiplied by the number of atoms. 243 00:18:42,510 --> 00:18:47,630 So we go back to our equation-- 244 00:18:47,630 --> 00:18:52,130 rate of absorption minus rate of stimulated emission 245 00:18:52,130 --> 00:18:57,470 minus the rate of spontaneous emission. 246 00:18:57,470 --> 00:19:00,020 So I'll write it here. 247 00:19:00,020 --> 00:19:07,310 0 is equal to Nb dot equal minus A Nb-- 248 00:19:07,310 --> 00:19:10,240 that's the spontaneous emission. 249 00:19:10,240 --> 00:19:11,900 We write it first. 250 00:19:11,900 --> 00:19:13,990 And then we'll write the other two-- 251 00:19:13,990 --> 00:19:30,520 Bba and Nb U omega ba plus Bab U of omega ba Na.