This Quantum World/Appendix/Relativity/Lorentz transformations: Difference between revisions

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Lorentz transformations (general form)

We want to express the coordinates t and 𝐫=(x,y,z) of an inertial frame 1 in terms of the coordinates t and 𝐫=(x,y,z) of another inertial frame 2. We will assume that the two frames meet the following conditions:


  1. their spacetime coordinate origins coincide (t=0,𝐫=0 mark the same spacetime location as t=0,𝐫=0),
  2. their space axes are parallel, and
  3. 2 moves with a constant velocity 𝐰 relative to 1.


What we know at this point is that whatever moves with a constant velocity in 1 will do so in 2. It follows that the transformation t,𝐫t,𝐫 maps straight lines in 1 onto straight lines in 2. Coordinate lines of 1, in particular, will be mapped onto straight lines in 2. This tells us that the dashed coordinates are linear combinations of the undashed ones,


t=At+𝐁𝐫,𝐫=C𝐫+(𝐃𝐫)𝐰+t.


We also know that the transformation from 1 to 2 can only depend on 𝐰, so A, 𝐁, C, and 𝐃 are functions of 𝐰. Our task is to find these functions. The real-valued functions A and C actually can depend only on w=|𝐰|=+𝐰𝐰, so A=a(w) and C=c(w). A vector function depending only on 𝐰 must be parallel (or antiparallel) to 𝐰, and its magnitude must be a function of w. We can therefore write 𝐁=b(w)𝐰, 𝐃=[d(w)/w2]𝐰, and =e(w)𝐰. (It will become clear in a moment why the factor w2 is included in the definition of 𝐃.) So,


t=a(w)t+b(w)𝐰𝐫,𝐫=c(w)𝐫+d(w)𝐰𝐫w2𝐰+e(w)𝐰t.


Let's set 𝐫 equal to 𝐰t. This implies that 𝐫=(c+d+e)𝐰t. As we are looking at the trajectory of an object at rest in 2, 𝐫 must be constant. Hence,

c+d+e=0.

Let's write down the inverse transformation. Since 1 moves with velocity 𝐰 relative to 2, it is


t=a(w)tb(w)𝐰𝐫,𝐫=c(w)𝐫+d(w)𝐰𝐫w2𝐰e(w)𝐰t.


To make life easier for us, we now chose the space axes so that 𝐰=(w,0,0). Then the above two (mutually inverse) transformations simplify to


t=at+bwx,x=cx+dx+ewt,y=cy,z=cz,
t=atbwx,x=cx+dxewt,y=cy,z=cz.


Plugging the first transformation into the second, we obtain


t=a(at+bwx)bw(cx+dx+ewt)=(a2bew2)t+(abwbcwbdw)x,
x=c(cx+dx+ewt)+d(cx+dx+ewt)ew(at+bwx)
     =(c2+2cd+d2bew2)x+(cew+dewaew)t,
y=c2y,
z=c2z.


The first of these equations tells us that

a2bew2=1  and  abwbcwbdw=0.

The second tells us that

c2+2cd+d2bew2=1  and  cew+dewaew=0.

Combining abwbcwbdw=0 with c+d+e=0 (and taking into account that w0), we obtain b(a+e)=0.

Using c+d+e=0 to eliminate d, we obtain e2bew2=1 and e(a+e)=0.

Since the first of the last two equations implies that e0, we gather from the second that e=a.

y=c2y tells us that c2=1. c must, in fact, be equal to 1, since we have assumed that the space axes of the two frames a parallel (rather than antiparallel).

With c=1 and e=a, c+d+e=0 yields d=a1. Upon solving e2bew2=1 for b, we are left with expressions for b,c,d, and e depending solely on a:

b=1a2aw2,c=1,d=a1,e=a.

Quite an improvement!

To find the remaining function a(w), we consider a third inertial frame 3, which moves with velocity 𝐯=(v,0,0) relative to 2. Combining the transformation from 1 to 2,


t=a(w)t+1a2(w)a(w)wx,x=a(w)xa(w)wt,


with the transformation from 2 to 3,


t=a(v)t+1a2(v)a(v)vx,x=a(v)xa(v)vt,


we obtain the transformation from 1 to 3:


t=a(v)[a(w)t+1a2(w)a(w)wx]+1a2(v)a(v)v[a(w)xa(w)wt]
     =[a(v)a(w)1a2(v)a(v)va(w)w]t+[]x,
x=a(v)[a(w)xa(w)wt]a(v)v[a(w)t+1a2(w)a(w)wx]
     =[a(v)a(w)a(v)v1a2(w)a(w)w]x[]t.


The direct transformation from 1 to 3 must have the same form as the transformations from 1 to 2 and from 2 to 3, namely


t=a(u)t+1a2(u)a(u)ux,x=a(u)xa(u)ut,


where u is the speed of 3 relative to 1. Comparison of the coefficients marked with stars yields two expressions for a(u), which of course must be equal:


a(v)a(w)1a2(v)a(v)va(w)w=a(v)a(w)a(v)v1a2(w)a(w)w.


It follows that [1a2(v)]a2(w)w2=[1a2(w)]a2(v)v2, and this tells us that


K=1a2(w)a2(w)w2=1a2(v)a2(v)v2


is a universal constant. Solving the first equality for a(w), we obtain

a(w)=1/1+Kw2.

This allows us to cast the transformation

t=at+bwx,x=cx+dx+ewt,y=cy,z=cz,

into the form


t=t+Kwx1+Kw2,x=xwt1+Kw2,y=y,z=z.


Trumpets, please! We have managed to reduce five unknown functions to a single constant.

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