1 00:00:01,950 --> 00:00:04,540 So, what constitutes a symmetry in quantum physics? 2 00:00:04,540 --> 00:00:08,316 We've talked about some of this before, but here's, here it is to be made 3 00:00:08,316 --> 00:00:11,526 explicit. So, let's suppose we have a solution to 4 00:00:11,526 --> 00:00:14,546 the Schrodinger equation. We have a wave function which evolves in 5 00:00:14,546 --> 00:00:21,540 accordance with the Schrodinger equation. And let's, let's suppose there's an 6 00:00:21,540 --> 00:00:29,854 operator, U, that commutes with H. So, U U for which minus HU is identically 7 00:00:29,854 --> 00:00:35,350 zero everywhere. Then, I think you can see that if we 8 00:00:35,350 --> 00:00:44,100 apply U to psi on this, so first of all the U is to be not time dependent. 9 00:00:44,100 --> 00:00:46,512 I mean, there could be some trivial time dependence that this one the equitation 10 00:00:46,512 --> 00:00:49,215 is still satisfied. But we're looking primarily for things 11 00:00:49,215 --> 00:00:55,194 that don't, don't change in time. so it passes through the time derivative. 12 00:00:55,194 --> 00:01:03,060 And then, it also passes through H so because of the commutation relationship. 13 00:01:03,060 --> 00:01:09,380 So, you can see that now if psi is solution, then U psi is also a solution. 14 00:01:10,610 --> 00:01:14,453 So this, this means that if we do have a symmetry, we can use it to, either to 15 00:01:14,453 --> 00:01:18,737 generate different solutions that have the same evolution as an underlying wave 16 00:01:18,737 --> 00:01:23,829 function. Or more significantly we can 17 00:01:23,829 --> 00:01:29,950 simultaneously diagonalize U and H, the Hamiltonian matrix. 18 00:01:29,950 --> 00:01:35,345 So we can, we can, in this, in the time independent Schrodinger's equation, we 19 00:01:35,345 --> 00:01:41,490 can look for for solutions that are eigenfunctions of U. 20 00:01:41,490 --> 00:01:46,114 And for the case of case of discrete symmetries it's, it's they give a lot of 21 00:01:46,114 --> 00:01:51,140 practical guidance on how to construct wave functions. 22 00:01:51,140 --> 00:01:57,530 It, it's easy to generate functions that are eigenfunctions of U. 23 00:01:57,530 --> 00:02:04,160 And then that, that provides say, a smaller basis for expiration of the the 24 00:02:04,160 --> 00:02:08,630 Hamiltonian. Why is symmetry useful? 25 00:02:08,630 --> 00:02:13,481 Well, the point is, one point is, it gives you a way of organizing work that's 26 00:02:13,481 --> 00:02:18,153 highly efficient. So for example, a graphene is this, this 27 00:02:18,153 --> 00:02:23,910 new material relatively new material, subject to recent Nobel Prize in Physics. 28 00:02:23,910 --> 00:02:29,466 It's a it's a two dimensional network. And so if you have a large, if you have a 29 00:02:29,466 --> 00:02:33,882 large sheet of graphene, there are many electrons, there's many, there's many 30 00:02:33,882 --> 00:02:38,564 nuclei. if you can focus your solution on solving 31 00:02:38,564 --> 00:02:42,596 solving wave functions and have a particular symmetry that conforms to the 32 00:02:42,596 --> 00:02:48,444 symmetry to the underlying graphene. there's a lot less work to do, and you've 33 00:02:48,444 --> 00:02:52,201 better predictive capabilities. There's, there's some things where you 34 00:02:52,201 --> 00:02:56,533 can actually determine what type of what type of electronic orbitals being excited 35 00:02:56,533 --> 00:03:05,032 by looking at an angular distribution. So in a case like this symmetry is widely 36 00:03:05,032 --> 00:03:12,740 used to simplify practical calculations or analysis of experimental data. 37 00:03:12,740 --> 00:03:16,962 Another example, discreet symmetry. So this is a schematic of the green laser 38 00:03:16,962 --> 00:03:21,642 pointer which is described in an accessible form in the co, additional 39 00:03:21,642 --> 00:03:27,270 materials in the course. And so, this is sort of a hypothetical 40 00:03:27,270 --> 00:03:31,140 example, but it's, it's emblematic of things that happen in the real world. 41 00:03:31,140 --> 00:03:34,430 Let's say you you, you need to design a laser that's going to operate a certain 42 00:03:34,430 --> 00:03:39,150 wavelength region. Say that the telecommunications region, 43 00:03:39,150 --> 00:03:43,691 very important area. and you know of some sharp line systems 44 00:03:43,691 --> 00:03:50,169 that can be used to get lasing action. But may be the the specific measurements 45 00:03:50,169 --> 00:03:56,310 of the relative transition probabilities haven't been made in those systems. 46 00:03:56,310 --> 00:04:00,370 So, you know, how do you, so here's a set of, here's a set of levels of the 47 00:04:00,370 --> 00:04:05,406 Neodymium 3+ ion. Now, you'll, in principle, you can have a 48 00:04:05,406 --> 00:04:10,060 transition between any two, any of these, these levels. 49 00:04:10,060 --> 00:04:13,946 But it may be that some of those transitions are forbidden, or they're 50 00:04:13,946 --> 00:04:19,300 very weak, for reasons of symmetry. So appreciating the the so-called 51 00:04:19,300 --> 00:04:23,975 selection rules that are dictated by symmetry considerations. 52 00:04:23,975 --> 00:04:26,060 This is a very important practical concern. 53 00:04:26,060 --> 00:04:28,452 Okay, now we're going to talk about parity. 54 00:04:28,452 --> 00:04:33,990 So one might say this is some sense the simplest discrete symmetry that's, that's 55 00:04:33,990 --> 00:04:40,202 basically, let's say it's a symmetry associated with the vacuum. 56 00:04:40,202 --> 00:04:45,450 Rather than with a crystal or particular molecular structure. 57 00:04:45,450 --> 00:04:48,180 and it's the that the parity transformation is something that inverts 58 00:04:48,180 --> 00:04:51,113 all coordinates of the the particles of the system. 59 00:04:51,113 --> 00:04:53,540 All the spacial coordinates of the particles of a system. 60 00:04:53,540 --> 00:04:55,565 All the spacial coordinates of the particles of a system. 61 00:04:55,565 --> 00:05:00,481 Okay, I hope that was relatively straightforward. 62 00:05:00,481 --> 00:05:06,510 clearly the potential is unaffected by the parity transformation. 63 00:05:06,510 --> 00:05:09,160 You change the sign of both things. You're taking the absolute value. 64 00:05:09,160 --> 00:05:12,595 It's still a difference. Now, you do have to think a little bit, 65 00:05:12,595 --> 00:05:16,640 perhaps about the kinetic energy operator. 66 00:05:16,640 --> 00:05:20,564 but I'll just say it this way. The kinetic energy is a gradient sorry, 67 00:05:20,564 --> 00:05:25,422 the momentum is a gradient. I think that was made explicit in the 68 00:05:25,422 --> 00:05:30,922 statements of the inline video. And so the gradient of a function, with 69 00:05:30,922 --> 00:05:35,855 respect to a coordinate, does change sign under inversion. 70 00:05:35,855 --> 00:05:41,553 But since the Hamiltonian depends upon the square of the gradient that's doesn't 71 00:05:41,553 --> 00:05:45,277 matter. Okay, well, now let's just take a, make a 72 00:05:45,277 --> 00:05:49,112 slight modification to this problem, which again, corresponds to real thing 73 00:05:49,112 --> 00:05:55,220 that one might do in the laboratory. So now we, you know, we, let's say we're 74 00:05:55,220 --> 00:05:59,550 in the lab, we study that previous system. 75 00:05:59,550 --> 00:06:02,500 Now, we want to understand it's response to an electric field. 76 00:06:02,500 --> 00:06:05,685 You know, by the way, the response of the hydrogen atom to an electric field was 77 00:06:05,685 --> 00:06:09,930 one of the first problems studied by Schrodinger in his early papers. 78 00:06:09,930 --> 00:06:13,930 So, this is another huge triumph of quantum physics. 79 00:06:13,930 --> 00:06:17,765 It became the first theory that was able to actually predict from first 80 00:06:17,765 --> 00:06:22,020 principles, how matter interacted with electricity. 81 00:06:22,020 --> 00:06:25,499 I mean, that's really huge, right? prior to that there were only these 82 00:06:25,499 --> 00:06:30,450 effective ideas, things had dialectic constants, or they were ideal conductors. 83 00:06:30,450 --> 00:06:35,122 But quantum mechanics turns out to give a really good account of how electric 84 00:06:35,122 --> 00:06:42,220 fields how, how they cause behavior to change in material systems. 85 00:06:42,220 --> 00:06:48,940 So we're going to follow that model and apply an electric field to this system. 86 00:06:48,940 --> 00:06:53,550 So, we have the same, the same particle interactions going on. 87 00:06:53,550 --> 00:06:59,182 But now this is the Ham, this is the Hamiltonian for the potential associated 88 00:06:59,182 --> 00:07:07,920 with the position of a particle of charge Q at position R in electric field. 89 00:07:07,920 --> 00:07:11,742 Just the scale or product. Okay, so now we're, our parity operator 90 00:07:11,742 --> 00:07:15,930 is the same as before, is applied in the same way. 91 00:07:15,930 --> 00:07:19,350 And my question is, is parity conserved in this system? 92 00:07:19,350 --> 00:07:25,050 So I hope, I hope it's evident to you that, this term here, causes, causes 93 00:07:25,050 --> 00:07:31,470 parity to to, to not be conserved in the system. 94 00:07:31,470 --> 00:07:37,160 Because there is a, an externally applied force that has a particular direction. 95 00:07:37,160 --> 00:07:42,272 And so that when you you know, when you change when you change positions in that 96 00:07:42,272 --> 00:07:48,354 force field, you change the energy. So, the, it is, it is the case, it's, 97 00:07:48,354 --> 00:07:53,598 it's, it's, common place that you can break parity by the use by changing 98 00:07:53,598 --> 00:08:01,432 making asymmetries in, in potentials. but once again as you can see from this, 99 00:08:01,432 --> 00:08:06,436 very general Hamiltonian. There's sort of a natural hope that 100 00:08:06,436 --> 00:08:10,670 parity will be conserved in material systems. 101 00:08:10,670 --> 00:08:16,840 And it's largely true but not entirely. So, as I mentioned in the introduction 102 00:08:16,840 --> 00:08:22,538 this is one of the the great experiments and theoretical predictions of mid-20th 103 00:08:22,538 --> 00:08:31,130 century physics that in beta decay, you know, a very fundamental process. 104 00:08:31,130 --> 00:08:34,870 There would, there could be parity-violating interactions. 105 00:08:34,870 --> 00:08:39,910 And this has since become even more widely interesting with the and in the 106 00:08:39,910 --> 00:08:45,748 context of the standard model. Because there are specific predictions 107 00:08:45,748 --> 00:08:50,212 about how parity for non-conserving interactions would be found even in a 108 00:08:50,212 --> 00:08:54,754 spectra of atoms. Which are ordinarily thought to be 109 00:08:54,754 --> 00:09:01,312 completely dominated by these simple electrostatics in quantum mechanics. 110 00:09:02,540 --> 00:09:05,570 Arguments that were illustrated in that previous model. 111 00:09:05,570 --> 00:09:09,020 So, it's a very active field of research a lot of opportunities, both for theory 112 00:09:09,020 --> 00:09:13,301 and experiment. Okay, next time, we're going ahead with 113 00:09:13,301 --> 00:09:17,770 angular momentum. Much more substantial subject. 114 00:09:17,770 --> 00:09:21,924 And one that's going to have a little bit more of a mathematical mathematical 115 00:09:21,924 --> 00:09:25,780 training for those who like that sort of thing.