Derivation of Lorentz algebra commutation relation

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Homework Help Overview

The discussion revolves around the derivation of the Lorentz algebra commutation relations, specifically focusing on the generators of the Lorentz algebra and their properties. The original poster seeks to demonstrate the commutation relation involving the generators and explore a representation of the Lorentz group.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the distribution of terms in the expression for the commutation relation and how to relate certain factors to the metric tensor. Questions arise regarding the relationship between the Kronecker delta and the metric tensor, as well as the implications of raising indices.

Discussion Status

The discussion is active, with participants engaging in clarifying the relationships between various mathematical expressions. Some guidance has been offered regarding the manipulation of indices and the interpretation of terms, but no consensus has been reached on the exact relationships being explored.

Contextual Notes

Participants are navigating the complexities of tensor notation and the properties of the metric tensor within the context of the Lorentz algebra. There is an emphasis on understanding the implications of different mathematical identities and their relevance to the problem at hand.

spaghetti3451
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Homework Statement



1. Show that the Lorentz algebra generator ##J^{\mu \nu} = i(x^{\mu}\partial^{\nu}-x^{\nu}\partial^{\mu})## lead to the commutation relation ##[J^{\mu \nu}, J^{\rho \sigma}] = i(g^{\nu \rho}J^{\mu \sigma} - g^{\mu \rho}J^{\nu \sigma}-g^{\nu \sigma}J^{\mu \rho}+g^{\mu \sigma}J^{\nu \rho})##.

2. Show that one particular representation of the the Lorentz group given by ##(J^{\mu \nu})_{\alpha \beta} = i(\delta^{\mu}_{\alpha}\delta^{\nu}_{\beta}-\delta^{\mu}_{\beta}\delta^{\nu}_{\alpha})##.

Homework Equations



The Attempt at a Solution



##[J^{\mu \nu}, J^{\rho \sigma}]##

##= J^{\mu \nu}J^{\rho \sigma}-J^{\rho \sigma}J^{\mu \nu}##

##= -(x^{\mu}\partial^{\nu}-x^{\nu}\partial^{\mu})(x^{\rho}\partial^{\sigma}-x^{\sigma}\partial^{\rho})+(x^{\rho}\partial^{\sigma}-x^{\sigma}\partial^{\rho})(x^{\mu}\partial^{\nu}-x^{\nu}\partial^{\mu})##.

How do I get the metric tensor from here?
 
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When you distribute terms you will find various factors like ##\partial^\nu x^\rho##.
 
How are those factors related to the metric tensor?

As far as I know, a term like ##\partial_{\nu}x^{\rho}## gives the Kronecker delta ##\delta_{\nu}^{\rho}##, not the metric tensor.
 
Now raise the index.
 
So, you say ##\delta_{\nu}^{\rho}## equals ##g^{\nu \rho}##?
 
Or, do I use ##\delta_{\nu}^{\rho} = g^{\nu \rho}g_{\nu \rho}##?
 
failexam said:
So, you say ##\delta_{\nu}^{\rho}## equals ##g^{\nu \rho}##?

Not exactly, ##\partial^\nu x^\rho = g^{\nu\mu} \partial_\mu x^\rho##. So use the result for ##\partial_\mu x^\rho## here.
 

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