How to Derive the Conservation Law for the FRW Metric?

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SUMMARY

The discussion focuses on deriving the conservation law for the Friedmann-Robertson-Walker (FRW) metric, specifically addressing the equation ##\nabla^a T_{ab}=0##. The author employs the Levi-Civita connection and analyzes the energy-momentum tensor components, particularly in the comoving frame where ##u^a=(c,\vec{0})##. Key challenges include understanding the implications of choosing a specific frame of reference and the behavior of the covariant derivative on scalars and constants. The author concludes that the scale factor ##a## is crucial for reaching the desired result.

PREREQUISITES
  • Understanding of the Friedmann-Robertson-Walker (FRW) metric
  • Familiarity with covariant derivatives and the Levi-Civita connection
  • Knowledge of energy-momentum tensors in general relativity
  • Concept of comoving frames in cosmology
NEXT STEPS
  • Study the derivation of the energy-momentum tensor for perfect fluids in general relativity
  • Learn about the implications of the scale factor ##a## in cosmological models
  • Explore the properties of the Levi-Civita connection in different coordinate systems
  • Investigate the principle of equivalence and its applications in general relativity
USEFUL FOR

Researchers and students in theoretical physics, particularly those focusing on cosmology and general relativity, will benefit from this discussion. It is also valuable for anyone looking to deepen their understanding of conservation laws in curved spacetime.

Markus Kahn
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Homework Statement
Given the FRW metric
$$d s^{2}=-d t^{2}+a(t)^{2}\left[\frac{d r^{2}}{1-k r^{2}}+r^{2}\left(d \theta^{2}+\sin ^{2} \theta d \varphi^{2}\right)\right]$$
and the Stress-energy tensor of an ideal fluid,
$$T_{a b}=(P+\rho) u_{a} u_{b}+P g_{a b}, \quad \text{where}\quad P=\omega \rho\quad \text{and}\quad u^a:=\frac{dx^a}{d\tau},$$
My Prof. claimed during yesterdays lecture that one can show that the zero component of the convervation equation of ##T_{ab}## results in
$$\frac{d}{d t} \log \rho\propto\frac{d}{d t} \log a(t)\tag{1}.$$
I've been trying to show this now for a while and I just can't figure it out...
Relevant Equations
All given above.
My attempt:
  1. Realize we can work in whatever coordinate system we want, therefore we might as well work in the rest frame of the fluid. In this case ##u^a=(c,\vec{0})##.
  2. The conservation law reads ##\nabla^a T_{ab}=0##. Let us pick the Levi-Civita connection so that we don't have to worry about ##\nabla g##. We then get $$\begin{align*}\nabla^a T_{ab} &= \nabla^a\left((1+\omega)\rho u_{a} u_{b}+\omega\rho g_{a b}\right)\\&= (1+\omega)\nabla^a(\rho u_au_b)+ \omega g_{ab}\nabla^a\rho\\&\overset{(*)}{=} (1+\omega) u_au_b\nabla^a\rho+ \omega g_{ab}\nabla^a\rho\\&= \left((1+\omega) u_au_b+ \omega g_{ab}\right)\nabla^a\rho,\end{align*}$$ where in ##(*)## we use the fact that ##u^a## are constant in the comoving frame.
  3. For the zero component I now get $$\begin{align*}\nabla_a T^{a0} &= \left((1+\omega) u^au^0+ \omega g^{a0}\right)\nabla_a\rho = \left((1+\omega)c u^a+ \omega g^{a0}\right)\nabla_a\rho\\&= -(1+\omega)c^2 \nabla_0\rho -\omega \nabla_0\rho\\&= -(1+\omega)c^2 \partial_t\rho -\omega \partial_t\rho\\&\overset{!}{=}0 \end{align*}$$ I don't really think there is a way to get to the claimed result from here, since I'm completely missing the scale factor ##a##.
Questions
I suspect that my problem lies in the fact that I'm not sure if
  • I'm actually allowed to pick a specific frame of reference and work in it and
  • I understand correctly how the covariant derivative acts on scalars (##\rho##) and constant values (##u^a##, since they are only zero or ##c## in the comoving frame).
The answer to the second question is, I think, that the covariant derivative in this case just acts like a "normal" derivative. But I'm of course not sure and it isn't working... So I'm presumably misunderstanding something. Any hints on how to show this are appreciated!
 
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Yes. It is better to pick up a specific frame. By Principal of equivalence, it should hold in every frame. In the comoving frame in which fluid elements is at origin, the connection coefficient simplify considerably.

Some Hints:
##\nabla_j T^{0j}=\frac {\partial T^{0j}}{\partial x_j}+ \Gamma^0_{\mu\nu}T^{\mu\nu}+\Gamma^{\mu}_{\mu\nu}T^{0\nu}##

Now: ##T^{00}=\rho, T^{0i}=0, T^{ij}=P##And near origin ##g_{ij}=a^2 \delta_{ij}##
 

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