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"Don't panic!"
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I've been reading Straumann's book "General Relativity & Relativistic Astrophysics". In it, he claims that the twice contracted Bianchi identity: $$\nabla_{\mu}G^{\mu\nu}=0$$ (where ##G^{\mu\nu}=R^{\mu\nu}-\frac{1}{2}g^{\mu\nu}R##) is a consequence of the diffeomorphism (diff) invariance of the Einstein-Hilbert (EH) action. Now, I can show (I think) that the EH action is diff invariant, by considering a infinitesimal diff, generated by a vector field ##X##: $$\delta_{X}S_{EH}=\phi^{\ast}S_{EH}-S_{EH}=\int_{M}\mathcal{L}_{X}\left(d^{4}x\sqrt{-g}R\right)=\int_{M}\left[\mathcal{L}_{X}\left(d^{4}x\sqrt{-g}\right)R +d^{4}x\sqrt{-g}\mathcal{L}_{X}\left(R\right)\right]\\ \qquad\qquad\qquad\quad\;\;=\int_{M}d^{4}x\sqrt{-g}\left[\nabla_{\mu}X^{\mu}R+X^{\mu}\nabla_{\mu}R\right]=\int_{M}d^{4}x\sqrt{-g}\,\nabla_{\mu}\left(X^{\mu}R\right)\\ =\int_{\partial M}d^{3}x\sqrt{h}\,n_{\mu}X^{\mu}R=0\;\;\qquad\qquad\qquad\quad$$ where ##h_{ij}## is the induced metric on the boundary ##\partial M## of the manifold ##M##, with ##n^{\mu}## the normal vector to the boundary. The last equality follows upon the assumption that ##X^{\mu}## has compact support in ##M##.
However, I'm unsure how one uses this fact to derive the (twice-contracted) Bianchi identity?
Straumann simply writes: $$\delta S=\int_{M}d^{4}x\sqrt{-g}\left(\frac{1}{\sqrt{-g}}\frac{\delta S_{EH}}{\delta g^{\mu\nu}}\right)\delta g^{\mu\nu}=\int_{M}d^{4}x\sqrt{-g}\,G_{\mu\nu}\delta g^{\mu\nu}=-\int_{M}d^{4}x\sqrt{-g}\,G^{\mu\nu}\delta g_{\mu\nu}$$ and notes that for an infinitesimal diff (generated by some vector field ##X##), ##\delta g_{\mu\nu}=2\nabla_{(\mu}X_{\nu)}##, such that $$\delta_{X} S=-2\int_{M}d^{4}x\sqrt{-g}\,G^{\mu\nu}\nabla_{\mu}X_{\nu}=2\int_{M}d^{4}x\sqrt{-g}\,X_{\nu}\nabla_{\mu}G^{\mu\nu}=0$$ and so, since ##X^{\nu}## is arbitrary, it must be that ##\nabla_{\mu}G^{\mu\nu}=0##.
What confuses me about this, is that one neglects the effect of the Lie derivative on ##d^{4}x## in this case (in the proof that the EH action is diff invariant, it was taken into account). Is the point that an infinitesimal diff is carried out in the *same* coordinate chart, and so ##d^{4}x## doesn't change in this case?
However, I'm unsure how one uses this fact to derive the (twice-contracted) Bianchi identity?
Straumann simply writes: $$\delta S=\int_{M}d^{4}x\sqrt{-g}\left(\frac{1}{\sqrt{-g}}\frac{\delta S_{EH}}{\delta g^{\mu\nu}}\right)\delta g^{\mu\nu}=\int_{M}d^{4}x\sqrt{-g}\,G_{\mu\nu}\delta g^{\mu\nu}=-\int_{M}d^{4}x\sqrt{-g}\,G^{\mu\nu}\delta g_{\mu\nu}$$ and notes that for an infinitesimal diff (generated by some vector field ##X##), ##\delta g_{\mu\nu}=2\nabla_{(\mu}X_{\nu)}##, such that $$\delta_{X} S=-2\int_{M}d^{4}x\sqrt{-g}\,G^{\mu\nu}\nabla_{\mu}X_{\nu}=2\int_{M}d^{4}x\sqrt{-g}\,X_{\nu}\nabla_{\mu}G^{\mu\nu}=0$$ and so, since ##X^{\nu}## is arbitrary, it must be that ##\nabla_{\mu}G^{\mu\nu}=0##.
What confuses me about this, is that one neglects the effect of the Lie derivative on ##d^{4}x## in this case (in the proof that the EH action is diff invariant, it was taken into account). Is the point that an infinitesimal diff is carried out in the *same* coordinate chart, and so ##d^{4}x## doesn't change in this case?