Proving ##C## is constant in 4-dim ##R_{\mu\nu}=Cg_{\mu\nu}##

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SUMMARY

The discussion centers on proving that the constant C in the equation ##R_{\mu\nu}=Cg_{\mu\nu}## is indeed constant by applying the covariant derivative to both sides of Einstein's equation. The user demonstrates that the conservation of the energy-momentum tensor leads to the conclusion that ##\nabla_{\nu}C=0##, confirming C's constancy. Additionally, the user questions whether the form of the Ricci tensor ##R_{\mu\nu}## implies that the manifold is maximally symmetric, referencing the properties of the Riemann tensor and Ricci scalar.

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  • Understanding of Einstein's field equations and Ricci tensor
  • Familiarity with covariant derivatives and metric compatibility
  • Knowledge of Riemann curvature and maximally symmetric spaces
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The discussion is beneficial for theoretical physicists, mathematicians specializing in differential geometry, and students studying general relativity who seek to deepen their understanding of curvature and symmetry in manifolds.

crime9894
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Homework Statement
Suppose for a certain 4-dimensional manifold, the Ricci tensor is given by ##R_{\mu}{\nu}=Cg_{\mu}{\nu}## .
Show C is constant (make necessary assumption)
Relevant Equations
Einstein's equation: ##R_{\mu\nu}-\frac{1}{2} Rg_{\mu\nu}=8\pi GT_{\mu\nu}##
This question wasn't particularly hard, so I assume metric compatibility and input Ricci tensor to the left side of Einstein's equation.
$$R_{\mu\nu}-\frac{1}{2} Rg_{\mu\nu}=Cg_{\mu\nu}-\frac{1}{2} (4C)g_{\mu\nu}=-Cg_{\mu\nu}$$
Then apply covariant derivative on both side:
$$\nabla^{\mu}(-Cg_{\mu\nu})=8\pi G\nabla^{\mu}T$$
From metric compatibility and conservation of energy-momentum tensor
$$\nabla_{\nu}C=0$$
Covariant derivative reduce to partial derivative when acted on scalar and thus conclude C is constant.

But now I thought of a different approach:
Maximally symmetric space has its Riemann tensor of the form:
$$R_{abcd}\propto g_{ac}g_{bd}-g_{ad}g_{bc}$$
Contracting both side once reduce it to Ricci tensor
$$R_{ab}\propto g_{ab}$$

So my question is: does it works the way around? Does ##R_{\mu\nu}## having the form ##Cg_{\mu\nu}## concludes the manifold is maximally symmetric?
Maximally symmetric space has constant Ricci scalar ##R## and contracting the Ricci tensor immediately yield desire conclusion.
But I'm not sure if such argument is valid at the first place
 
Last edited:
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What is C? Also, the notation doesn't seem to be working in LaTeX.
 

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