General Relativity: An Introduction for Physicists · Problem 17.4

Linearised general relativity — Hobson, Efstathiou & Lasenby

Physics · trace-reverse-linearised-einstein-equations

Problem

The trace reverse of hμνh_{\mu\nu} is defined by hˉμν≡hμν−12ημνh.\bar{h}_{\mu\nu} \equiv h_{\mu\nu} - \tfrac{1}{2}\eta_{\mu\nu}h. Show that hˉ=−h\bar{h} = -h and hˉˉμν=hμν\bar{\bar{h}}_{\mu\nu} = h_{\mu\nu}. Hence show that the linearised Einstein field equations in Exercise 17.3 can be written as □2hˉμν+ημν∂ρ∂σhˉρσ−∂ν∂ρhˉμρ−∂μ∂ρhˉνρ=−2κTμν.\Box^2\bar{h}_{\mu\nu} + \eta_{\mu\nu}\partial_{\rho}\partial_{\sigma}\bar{h}^{\rho\sigma} - \partial_{\nu}\partial_{\rho}\bar{h}^{\rho}_{\mu} - \partial_{\mu}\partial_{\rho}\bar{h}^{\rho}_{\nu} = -2\kappa T_{\mu\nu}.

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