gouranja
- 11
- 0
Hi,
I don't think this belongs in the homework section since this is a graduate course.
My question is regarding making a field theory generally covariant by including a metric tensor g_{\mu\nu}(x)in the Lagransian density, and it's transformation under infinitesimal coordinate change.
If I transform the coordinates according to:
x^{\mu}\rightarrow x^{\mu}'=x^{\mu}+\epsilon^{\mu}(x)
The metric must be transformed according to:
g_{\mu\nu}(x)\rightarrow g'_{\mu'\nu'}(x')=\frac{\partial x^{\alpha}}{\partial x^{\mu}'}\frac{\partial x^{\beta}}{\partial x^{\nu}'}g_{\alpha\beta}(x)
which I understand well. But according to the textbook I'm reading the infitesimal result is:
\delta g_{\mu\nu}(x)=\epsilon_{\mu;\nu}+\epsilon_{\nu;\mu}
(with covariant derivatives).
I have tried using:
\frac{\partial x^{\alpha}}{\partial x^{\mu}'}\simeq\delta_{\mu}^{\alpha}-\frac{\partial\epsilon^{\alpha}}{\partial x^{\mu}}+O(\epsilon^{2})
to obtain:
\delta g_{\mu\nu}(x)=-g_{\mu\alpha}\partial_{\nu}\epsilon^{\alpha}-g_{\nu\alpha}\partial_{\mu}\epsilon^{\alpha}
but I don't know how to obtain the textbook result.
Can someone clue me in on how to do it?
Thanks
I don't think this belongs in the homework section since this is a graduate course.
My question is regarding making a field theory generally covariant by including a metric tensor g_{\mu\nu}(x)in the Lagransian density, and it's transformation under infinitesimal coordinate change.
If I transform the coordinates according to:
x^{\mu}\rightarrow x^{\mu}'=x^{\mu}+\epsilon^{\mu}(x)
The metric must be transformed according to:
g_{\mu\nu}(x)\rightarrow g'_{\mu'\nu'}(x')=\frac{\partial x^{\alpha}}{\partial x^{\mu}'}\frac{\partial x^{\beta}}{\partial x^{\nu}'}g_{\alpha\beta}(x)
which I understand well. But according to the textbook I'm reading the infitesimal result is:
\delta g_{\mu\nu}(x)=\epsilon_{\mu;\nu}+\epsilon_{\nu;\mu}
(with covariant derivatives).
I have tried using:
\frac{\partial x^{\alpha}}{\partial x^{\mu}'}\simeq\delta_{\mu}^{\alpha}-\frac{\partial\epsilon^{\alpha}}{\partial x^{\mu}}+O(\epsilon^{2})
to obtain:
\delta g_{\mu\nu}(x)=-g_{\mu\alpha}\partial_{\nu}\epsilon^{\alpha}-g_{\nu\alpha}\partial_{\mu}\epsilon^{\alpha}
but I don't know how to obtain the textbook result.
Can someone clue me in on how to do it?
Thanks