Orthogonality of the coefficients of the Lorentz transformation

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Homework Help Overview

The discussion revolves around the orthogonality of the coefficients of the Lorentz transformation in the context of flat spacetime. The original poster presents the coefficients defined by the partial derivatives of transformed coordinates and seeks to demonstrate that these coefficients satisfy a specific orthogonality condition involving the Kronecker delta symbol.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to relate the orthogonality condition to an arbitrary four-vector and applies Einstein's summation rule but encounters difficulties in equating the resulting expression to the four-vector.
  • One participant notes the relationship between the transpose of the coefficients and suggests a different orthogonality condition involving the transpose.
  • Another participant mentions a standard proof approach that involves the invariance of the norm of a four-vector under Lorentz transformations.

Discussion Status

The discussion is active, with participants exploring different aspects of the problem. Some guidance has been offered regarding the relationship between the coefficients and their transposes, but there is no explicit consensus on the original problem's setup or the correctness of the textbook reference.

Contextual Notes

Participants are questioning the assumptions made in the original problem statement, particularly regarding the absence of the transpose in the orthogonality condition. There is also a mention of potential discrepancies with textbook definitions.

Sigurdsson
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Homework Statement


For flat spacetime the coefficients of the Lorentz transformation are defined as

[itex]\alpha^{\nu}_{\mu} = \frac{\partial x^{' \nu}}{\partial x^{\mu}}[/itex]

Whereas the Lorentz transformation is

[itex]\begin{pmatrix} x_1' \\ x_2' \\ x_3' \\ x_4' \end{pmatrix} = \begin{pmatrix} \alpha_0^0 & \alpha_1^0 & \alpha_2^0 & \alpha_3^0 \\ \alpha_0^1 & \alpha_1^1 & \alpha_2^1 & \alpha_3^1 \\ \alpha_0^2 & \alpha_1^2 & \alpha_2^2 & \alpha_2^3 \\ \alpha_0^3 & \alpha_1^3 & \alpha_2^3 & \alpha_3^3 \end{pmatrix} \begin{pmatrix}x_1 \\ x_2 \\ x_3 \\ x_4 \end{pmatrix}[/itex]

Here's the problem, show that the coefficients are orthogonal. That is

[itex]\alpha^{\nu}_{\lambda} \alpha^{\lambda}_{\mu} = \delta^{\nu}_{\mu}[/itex]

The last term is the Kronicker-Delta symbol


The Attempt at a Solution



Let's define some arbitrary four vector [itex]\mathbf{A}[/itex]

[itex]\delta^{\nu}_{\mu} A^{\mu} = \alpha^{\nu}_{\lambda} \alpha^{\lambda}_{\mu} A^{\mu} = \frac{\partial x^{' \nu}}{\partial x^{\lambda}} \frac{\partial x^{' \lambda}}{\partial x^{\mu}} A^{\mu}[/itex]

[itex]\delta^{\nu}_{\mu} A^{\mu} = \frac{\partial x^{' \lambda}}{\partial x^{\lambda}} A^{' \nu}[/itex]

Now according to Einsteins summation rule we should have

[itex]\mathbf{A} = \sum_{ \nu = 0}^{3} \left( \frac{\partial x^{' 0}}{\partial x^{0}} A^{' \nu} + \frac{\partial x^{' 1}}{\partial x^{1}} A^{' \nu} + \frac{\partial x^{' 2}}{\partial x^{2}} A^{' \nu} + \frac{\partial x^{' 3}}{\partial x^{3}} A^{' \nu} \right)[/itex]

This is where I get stuck. I have no idea how the sum on the right side should be equal to our 4-vector [itex]\mathbf{A}[/itex].

Any ideas?
 
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please note that the transpose of [tex]\alpha^{\mu}_{\nu} = \frac{\partial x'^{\mu}}{\partial x^{\nu}}[/tex] is [tex](\alpha^T)^{\mu}_{\nu} = \frac{\partial x^{\mu}}{\partial x'^{\nu}}[/tex] and you are supposed to show that

[tex]\alpha^{\mu}_{\nu} (\alpha^T)^{\nu}_{\sigma} = \delta^{\mu}_{\sigma}[/tex]
 
sgd37 said:
... you are supposed to show that

[tex]\alpha^{\mu}_{\nu} (\alpha^T)^{\nu}_{\sigma} = \delta^{\mu}_{\sigma}[/tex]

This I have solved with your excellent advice my dear sir

[tex]\mathbf{A} = \delta^{\nu}_{\mu} A^{\mu} = \alpha^{\nu}_{\lambda} (\alpha^T)^{\lambda}_{\mu} A^{\mu} = \frac{\partial x^{\nu}}{\partial x^{' \lambda} } \frac{\partial x^{' \lambda} }{\partial x^{\mu}}A^{\mu} = \frac{\partial x^{\nu}}{\partial x^{\mu}} A^{\mu} = \mathbf{A}[/tex]


But this is of course different from my original problem where there was no transpose. Could it be that my textbook is wrong?
 
The standard proof is to start off with the requirement that the norm of a 4-vector be a scalar/invariant wrt a Lorentz transformation. So x'2=x2.
 

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