Quantitative Meaning of Ricci Tensor

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SUMMARY

The Ricci tensor is a fundamental concept in general relativity that describes the curvature of spacetime due to gravity. It specifically relates to the evolution of volume along geodesics, but its relationship with volume changes is not universally applicable. The discussion highlights that while the Ricci tensor can govern volume evolution under specific conditions, such as in irrotational, shear-free geodesic congruences, it does not do so in general cases. For a deeper understanding, references to works by Manfredo do Carmo and John Baez provide valuable geometric interpretations and mathematical justifications.

PREREQUISITES
  • Understanding of general relativity principles
  • Familiarity with Riemannian geometry concepts
  • Knowledge of geodesics and their properties
  • Basic comprehension of tensor calculus
NEXT STEPS
  • Study the Raychaudhuri equation and its implications on geodesic congruences
  • Explore the geometric interpretations of the Ricci tensor in Manfredo do Carmo's texts
  • Investigate the mathematical foundations presented by John Baez regarding the Ricci tensor
  • Learn about the relationship between the Ricci tensor and cosmological models in general relativity
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Students and researchers in physics, particularly those focusing on general relativity, cosmology, and differential geometry, will benefit from this discussion.

flyinjoe
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Hello,

I am studying general relativity right now and I am very curious about the Ricci tensor and its meaning. I keep running into definitions that explain how the Ricci tensor describes the deviation in volume as a space is affected by gravity. However, I have yet to find any quantitative explanation of this definition. How can volume differences be calculated with the Ricci tensor? What role does the Ricci tensor play in the volume changes?

Thanks!
 
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flyinjoe said:
I am studying general relativity right now and I am very curious about the Ricci tensor and its meaning. I keep running into definitions that explain how the Ricci tensor describes the deviation in volume as a space is affected by gravity. However, I have yet to find any quantitative explanation of this definition. How can volume differences be calculated with the Ricci tensor? What role does the Ricci tensor play in the volume changes?
In general there's no such relationship. Maybe you're talking about a cosmological situation, in which the expansion rate of the universe can be related to the matter density? Please give us a quote/reference where you found this.
 
Hi Bill,

Thanks for the response. In this paper:
http://arxiv.org/pdf/gr-qc/0401099v1.pdf
the author writes, "So in roughly the same sense that the Riemann tensor governs the evolution of a vector or a displacement parallel propagated along a geodesic, the Ricci tensor governs the evolution of a small volume parallel propagated along a geodesic."
 
That is not true in general. It is only true if the geodesic belongs to an irrotational, shear-free time-like geodesic congruence in which case the claim follows from the Raychaudhuri equation. Otherwise the vorticity and shear of the congruence will both contribute to the evolution of the volume of the geodesic ball, in which case the Ricci tensor won't be the only thing governing the evolution.
 
Ok, excellent. So what, if anything, is the geometric or physical meaning of the Ricci tensor if it has no general relationship with volume?
 
You can interpret it that way, but you have to be careful.

http://math.ucr.edu/home/baez/einstein/node3.html

The rate at which a ball BEGINS to shrink, not just shrink, for one thing. Secondly, notice Baez's "fine print". This interpretation only works in a local reference frame in which the ball is initially at rest.
The mathematical justification can be found here:

http://math.ucr.edu/home/baez/einstein/node10.html

Just a little index-gymnastics directly from Einstein's equation, so I don't think it's in question.
 

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