1
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So because it's not really possible to straightforwardly drive to Maxwell's equation most of the time

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and discourse, we will just discuss these equations and in the end come up with the results that we

3
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compare to experiments so that we understand or that we see that everything makes sense and everything

4
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fits together.

5
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However, this very special lecture is a bit more theoretical because here we want to motivate how we

6
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can construct Maxwell's relations based on symmetry arguments.

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So if you cannot follow this lecture 100 percent, it's no big deal because this is somewhat an exotic

8
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lecture, because here we really go into theoretical physics and do everything a bit different.

9
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But I think it's really worth it to do this because when I was a student, I really, really like this

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lecture.

11
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So for this lecture, I really have to credit my professor, Ingrid Mantashe, who came up with this

12
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nice explanation.

13
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So that was first discussed several objects, for example, at the time, or the position vector or

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the velocity and understand how these objects relate or how they behave under certain symmetry operations.

15
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So you will later understand or realize why this is important.

16
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So, for example, we can consider the time what happens if we, for example, apply a space inversion

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operation?

18
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So this means we take the whole space and put a minus sign in front of it?

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Well, the time T doesn't care at all about the space because these are independent variables, at least

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in a non relativistic world.

21
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So in this sense, the time is symmetric under space inversion.

22
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So this just means it does not change when we change our minds.

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Are it?

24
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The same is also true for the for the derivative aspect to time, because this is something like one

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over T.

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So it doesn't really matter here.

27
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And if we apply a time inversion operation, this means that we change T to minus T and of course T

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changes to minus T.

29
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So this is not really an application of these concepts.

30
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This is really the definition of the of the time inversion operator and then here also for the space

31
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inversion operator.

32
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So time inversion means the.

33
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Yeah.

34
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The time is a..

35
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Symmetric and space inversion means that the space is a..

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Symmetric.

37
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So here when we take the position vector and we apply a space inversion operation, this does not matter

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at all because when we when we invert the time, the spaces unaffected.

39
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So it's symmetric.

40
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But when we apply the space inversion, then of course we get this minus sign here.

41
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And now the same thing is true for the derivative aspect to space.

42
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So this would be true for the derivative with respect to X, Y, Z, and also when we take this whole

43
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vector here, does KNOBLER operator.

44
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So this operator is symmetric at a time inversion and it's a..

45
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Symmetric under space inversion.

46
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Now, we can also take the velocity, so here the velocity is basically the derivative of the position

47
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with respect to the time.

48
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So it's something like position divided by time.

49
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So now, since this is just the quotient of these two quantities, we can take these two rows here and

50
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divide them.

51
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So if we have a..

52
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Symmetric divided by symmetric or if we have the other way around, in both cases, we will get an anti

53
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symmetry.

54
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So the velocities aren't symmetric with respect to time inversion and with respect to space inversion.

55
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Now, the acceleration is the second derivative of space time, so this is something like our over T-square.

56
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So here we have to take this one here squares and both of these will be symmetric and so on.

57
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The forward is space inversion.

58
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Just will give us an A. symmetric function like here.

59
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And for time inversion, this will give us a symmetric function because here we get the minus sign twice.

60
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Now, that force is exactly the same thing because it's just mass times acceleration and the mass is,

61
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of course, independent of time inversion and space inversion.

62
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And the charged density is also it's just a scalar.

63
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So it's also, yeah, really trivial, I would say, like the mass.

64
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So it's symmetric in both cases.

65
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However, if we take the current density, which is basically charged density multiplied by the velocity,

66
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then we get the same symmetric symmetry, transformation, behavior as for the velocity.

67
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So we get a..

68
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Symmetric behavior for the time inversion and for the space inversion.

69
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This was just some examples where you can understand how these objects, for example, acceleration

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or the velocity, behave when we reverse the time or the space.

71
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And I hope that this makes sense to you, because, for example, if you think of sitting in a car going

72
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with a certain velocity, if you would film yourself and then rewind the film, you would see that you

73
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go backwards.

74
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And also, if you would look in the mirror, for example, you would also see that you go into the opposite

75
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direction.

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So in both cases, this is a..

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Symmetric under these two operations.
