I have always struggled to visualize the correctness of the commutation relation for the generators of the boost in the Lorentz group. We have [Ki,Kj]=iϵijkLk
I fail to picture this. For definiteness' sake, let's take a point
→x in my coordinate system, lying in the
Oxy plane. The difference between boosting first in the
x and then in the
y direction, and boosting first in the
y and then in the
x direction ammounts simply to a rotation in the
Oxy plane, since
[K1,K2]=iL3
I must be doing something wrong when I draw this on a paper. I realize that this holds at the infinitesimal level, but a simple drawing should be able to realize this principle 'at first order' shouldn't it ? My problem is that when I draw it, I end up with the same situation regardless of which direction I boost into first.
Visualizing this is, in my opinion, pretty tricky because boosts generally act in four dimensions (time included!) and it's hard to draw 4D on a piece of paper. Fortunately, for this question, you can get around this artistic limitation.
Here's what I did right after reading your question to attempt to visualize what's going on. I encourage you to try to draw each step. The picture I ended up drawing is at the end.
If we order our coordinates in the standard way (t,x,y,z), then boosts with boost parameter β in the x and y directions are given by Λx(β)=(γ−γβ00−γβγ0000100001),Λy(β)=(γ0−γβ00100−γβ0γ00001)
We can now attempt to apply these transformations to some point in the
x-
y plane in different orders and draw the results. The key to visualizing the math I'm about to do is to note that both of these boosts do nothing to the
z coordinate of any spacetime point because there is a
1 in the lower right hand corner of each transformation matrix with zeros to its left and above. As a result, we can ignore the
z axis and draw spacetime diagrams in which the time axis is vertical and the
x-
y plane is horizontal.
For simplicity, let's see what happens to the point ex=(0,1,0,0)t. Here I will use a superscript t for transpose since I want to emphasize that points in spacetime will be written as column vectors. The point ex is simply the three-dimensional unit vector along the x-axis at time zero. What happens when we apply a small boost in the y-direction followed by a small boost in the x-direction? Well, let's compute; Λx(β)Λy(β)ex≈ex+(−β,β2/2,0,0)t
The
≈ symbol means that I have simply dropped lower order terms in the Taylor expansion in
β about
β=0. The point is translated backward in time and forward in
x. Now what happens when we apply the transformations in the other order and then expand the result?
Λy(β)Λx(β)ex≈ex+(−β,β2/2,β2,0)t
The same thing happens to the time and
x components as in the first order, but now the point is also shifted forward in
y a bit. When we subtract these two, we therefore get
(Λx(β)Λy(β)−Λy(β)Λx(β))ex≈(0,0,−β2,0)t
Does this agree with what a rotation in
z would do? Well a rotation in
z by an angle
ϕ looks like this:
Rz(ϕ)=(10000cosϕsinϕ00−sinϕcosϕ00001)
If you Taylor expand this about
ϕ=0, you'll get
Rz(ϕ)≈I+(000000ϕ00−ϕ000000)
So a rotation in
z acts on the point
ex to give
Rz(ϕ)ex≈ex+(0,0,−ϕ,0)t
In other words, it subtracts a bit from the
y-coordinate. But this subtraction is precisely what happened in the case of of the two boosts acting in different orders once we identify
ϕ=β2!

I know that this was all rather mathematical, but I can't see a way of getting around doing some math so as to be able to draw what happens to a point you choose under a given small boost or rotation.
No comments:
Post a Comment