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

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Homework Help Overview

The discussion revolves around proving that the constant ##C## in the equation ##R_{\mu\nu}=Cg_{\mu\nu}## is indeed a constant in the context of four-dimensional spacetime. The problem involves concepts from general relativity, specifically the Ricci tensor and metric compatibility.

Discussion Character

  • Exploratory, Conceptual clarification, Assumption checking

Approaches and Questions Raised

  • The original poster attempts to derive the constancy of ##C## using metric compatibility and the properties of the Ricci tensor. They also explore whether the form of ##R_{\mu\nu}## implies that the manifold is maximally symmetric, questioning the validity of this reasoning.

Discussion Status

Participants are engaging with the original poster's reasoning, with some questioning the clarity of notation and the definition of ##C##. There are references to external resources that may provide additional context, but no consensus has been reached regarding the implications of the original poster's arguments.

Contextual Notes

There is a mention of notation issues in LaTeX, which may affect the clarity of the discussion. The original poster also reflects on the relationship between the constant ##C## and the properties of the manifold, indicating a potential gap in understanding that is being explored.

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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