How Does Rapidity Influence the Lorentz Transformation Matrix?

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SUMMARY

The discussion focuses on deriving the Lorentz transformation matrix \(\Lambda\) in terms of rapidity \(\theta\) within a two-dimensional Minkowski space. The key equations involve rapidity relations \(\beta = \tanh \theta\) and \(\gamma = \cosh \theta\). The preservation of the inner product leads to the conditions \(\lambda_1^2 - \lambda_3^2 = 1\), \(\lambda_2^2 - \lambda_4^2 = -1\), and \(\lambda_1 \lambda_2 = \lambda_3 \lambda_4\). Ultimately, the transformation matrix is expressed as \(\Lambda = \begin{pmatrix} \cosh \theta & \pm \sinh \theta \\ \pm \sinh \theta & \cosh \theta \end{pmatrix}\), confirming that \(\lambda = \cosh \theta\) relates to rapidity.

PREREQUISITES
  • Understanding of Minkowski space and its properties
  • Familiarity with hyperbolic functions, specifically \(\cosh\) and \(\sinh\)
  • Knowledge of Lorentz transformations and their significance in relativity
  • Basic linear algebra, particularly matrix operations and inner products
NEXT STEPS
  • Study the derivation of the velocity 4-vector in special relativity
  • Explore the relationship between rapidity and velocity in relativistic contexts
  • Learn about the geometric interpretation of Lorentz transformations
  • Investigate applications of Lorentz transformations in particle physics
USEFUL FOR

This discussion is beneficial for physics students, particularly those studying special relativity, as well as educators and researchers interested in the mathematical foundations of Lorentz transformations.

Brian-san
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1. Homework Statement :
Consider a two dimensional Minkowski space (1 spatial, 1 time dimension). What is the condition on a transformation matrix \Lambda, such that the inner product is preserved? Solve this condition in terms of the rapidity.

2. Homework Equations :
Rapidity Relations:
\beta=tanh\theta, \gamma=cosh\theta

Inner Product:
u^T \eta u

3. The Attempt at a Solution :
From the definition of inner product, to preserve inner product when u'=\Lambda u, we must have \Lambda^T\eta\Lambda=\eta

In matrix form:
\left[ \begin{array}{cc} \lambda_1 & \lambda_3 \\ \lambda_2 & \lambda_4 \end{array} \right]\left[ \begin{array}{cc} 1 & 0 \\ 0 & -1 \end{array} \right]\left[ \begin{array}{cc} \lambda_1 & \lambda_2 \\ \lambda_3 & \lambda_4 \end{array} \right]=\left[ \begin{array}{cc} 1 & 0 \\ 0 & -1 \end{array} \right]

This gives three relations:
\lambda_1^2-\lambda_3^2=1, \lambda_2^2-\lambda_4^2=-1, \lambda_1\lambda_2=\lambda_3\lambda_4

After substituting and solving the equations, letting \lambda_1=\lambda, I get the final form of the matrix as:
\Lambda=\left[ \begin{array}{cc} \lambda & \pm\sqrt{\lambda^2-1} \\ \pm\sqrt{\lambda^2-1} & \lambda \end{array} \right]

The two matrices are inverses of each other which can be shown easily. Since the Lorentz transformations are like rotations that mix space and time dimensions, I know the final result in terms of rapidity should be:
\Lambda=\left[ \begin{array}{cc} cosh\theta & \pm sinh\theta \\ \pm sinh\theta & cosh\theta \end{array} \right]

However, I'm not sure how to get the final step I need, by showing \lambda=cosh\theta. All I can say for sure is based on how the transformations behave at v=0 (returns identity matrix), and v=c (rapidity is infinite), is that λ(0)=1 and the function is strictly increasing to infinity. Obviously hyperbolic cosine fits that description, but so do a lot of other functions. So, I'm not sure what specifically will let me get the function I need.

Thanks.
 
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What you have so far is correct. You have shown that you can write

\Lambda = \begin{pmatrix} \cosh \rho & \pm \sinh \rho \\ \pm \sinh \rho & \cosh \rho \end{pmatrix}

for some quantity \rho. What is left is to show that \rho is, in fact, the rapidity. To accomplish that, you should take a particle at rest and then boost it to some velocity \beta = v/c; then show how \rho is related to \beta.

I.e., you should know independently what the velocity 4-vector (2-vector in this case) should look like after a boost from rest, so use that to find how to interpret the parameter \rho.
 

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