Lorentz Transformations and Orthogonal Transformations in Euclidean Space, Lecture notes of Relativity Theory

The concept of orthogonal transformations in Euclidean space R2 (and Rn) and Lorentz transformations. It explains how to find all invertible linear changes of variable that preserve the length of a vector and the wave equation. The document also provides the matrix for rotations of the plane and linear changes of variable that preserve the Laplace operator.

Typology: Lecture notes

2021/2022

Uploaded on 05/11/2023

stagist
stagist 🇺🇸

4.1

(27)

265 documents

1 / 3

Toggle sidebar

This page cannot be seen from the preview

Don't miss anything!

bg1
Lorentz Transformations
Orthogonal Transformations
In Euclideal space R2(and Rn), it is valuable to find all the
invertible linear changes of variable y=Rx that preserve the
length of a vector
kRxk=kxk
so that
y2
1+y2
2=x2
1+x2
2.
These are orthogonal transformations. Say
x1=ay1+by2
x2=cy1+dy2.
Then
x2
1+x2
2= (a2+c2)y2
1+ 2(ab +cd)y1y2+ (b2+d2)y2
2.
We therefore want
a2+c2= 1, ab +cd = 0,and b2+d2= 1
There are four variables and only three conditions so we will
have one free parameter. To satisfy the first condition it is
natural to let a= cos θand c= sin θ. For the second condition,
let b=c=sin θand d=a= cos θ. The third condition is
also satisfied. This gives the matrix
R=cos θsin θ
sin θcos θ
These are the rotations of ther plane R2.
1
pf3

Partial preview of the text

Download Lorentz Transformations and Orthogonal Transformations in Euclidean Space and more Lecture notes Relativity Theory in PDF only on Docsity!

Lorentz Transformations

Orthogonal Transformations

In Euclideal space R^2 (and Rn), it is valuable to find all the invertible linear changes of variable y = Rx that preserve the length of a vector ‖Rx‖ = ‖x‖

so that y^21 + y 22 = x^21 + x^22.

These are orthogonal transformations. Say

x 1 =ay 1 + by 2 x 2 =cy 1 + dy 2.

Then

x^21 + x^22 = (a^2 + c^2 )y 12 + 2(ab + cd)y 1 y 2 + (b^2 + d^2 )y 22.

We therefore want

a^2 + c^2 = 1, ab + cd = 0, and b^2 + d^2 = 1

There are four variables and only three conditions so we will have one free parameter. To satisfy the first condition it is natural to let a = cos θ and c = sin θ. For the second condition, let b = −c = − sin θ and d = a = cos θ. The third condition is also satisfied. This gives the matrix

R =

cos θ − sin θ sin θ cos θ

These are the rotations of ther plane R^2.

By a similar computation, these are also the only linear changes of variable that preserve the Laplace operator

∂^2 u ∂x^21

∂^2 u ∂x^22

∂^2 u ∂y 12

∂^2 u ∂y 22

Lorentz Transformations

It is also valuable to find all linear changes of variable

x′^ =αx + βt t′^ =γx + δt

that preserve the wave equation

∂^2 u ∂t^2

− c^2 ∂^2 u ∂x^2

∂^2 u ∂t′^2

− c^2 ∂^2 u ∂x′^2

where c is a constant (the speed of sound or light).

By the chain rule,

utt−c^2 uxx = (δ^2 −c^2 γ^2 )ut′t′+2(βδ−c^2 αγ)ux′t′+(β^2 −c^2 α^2 )ux′x′.

Thus we want

δ^2 − c^2 γ^2 = 1, βδ − c^2 αγ = 0, and β^2 − c^2 α^2 = −c^2

First pick γ and δ so that δ^2 −c^2 γ^2 = 1, and then let β = ±c^2 γ, α = ±δ. To preserve orientation we use the + signs. Since c^2 α^2 − β^2 = c^2 and cosh^2 σ − sinh^2 σ = 1, it is traditional to write α = cosh σ, β = c sinh σ. For any real σ the transforma- tion

x′^ = (cosh σ) x + (c sinh σ) t t′^ = (

c

sinh σ) x + (cosh σ) t