EFE's question regarding Ricci scalar

In summary, the conversation discusses the issue of writing the Einstein Field Equations (EFE's) and using the definition of the Ricci scalar. It is mentioned that an index can only appear twice, which causes problems when expanding out the second term of the equation. Various solutions are proposed, including relabeling to avoid using the same symbol as both a free and summed index.
  • #1
unchained1978
93
0
Quick question about the EFE's. When writing the einstein tensor [itex]G_{\mu\nu}=R_{\mu\nu}-\frac{1}{2}Rg_{\mu\nu}[/itex], and using the definition of the Ricci scalar [itex]R=g^{\mu\nu}R_{\mu\nu}[/itex], how does this not give you problems when you expand out [itex]R[/itex] so that the second term becomes [itex]-\frac{1}{2}g^{\mu\nu}R_{\mu\nu}g_{\mu\nu}=-2R_{\mu\nu}[/itex] when evaluating the trace, giving you the EFE's as [itex]R_{\mu\nu}=-4πGT_{\mu\nu}[/itex]?
Any help would be appreciated.
 
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  • #2
unchained1978 said:
Quick question about the EFE's. When writing the einstein tensor [itex]G_{\mu\nu}=R_{\mu\nu}-\frac{1}{2}Rg_{\mu\nu}[/itex], and using the definition of the Ricci scalar [itex]R=g^{\mu\nu}R_{\mu\nu}[/itex], how does this not give you problems when you expand out [itex]R[/itex] so that the second term becomes [itex]-\frac{1}{2}g^{\mu\nu}R_{\mu\nu}g_{\mu\nu}=-2R_{\mu\nu}[/itex] when evaluating the trace, giving you the EFE's as [itex]R_{\mu\nu}=-4πGT_{\mu\nu}[/itex]?
Any help would be appreciated.

In anyone term, an index can only appear at most twice, so [itex]-\frac{1}{2}g^{\mu\nu}R_{\mu\nu}g_{\mu\nu}[/itex] is not legal. Maybe you want to write [itex]R=g^{\alpha\beta}R_{\alpha\beta}[/itex], or maybe you want do do something like
[tex]
\begin{align}
\left( R_{\mu\nu}-\frac{1}{2}Rg_{\mu\nu} \right) g^{\mu \nu} &= 8\pi T_{\mu\nu} g^{\mu \nu}\\
-R = 8\pi T^\mu_\mu.
\end{align}
[/tex]
Using [itex]-R = 8\pi T^\alpha_\alpha[/itex] (after relabeling to avoid the same symbol being used as both a free index and a summed index) in [itex]R_{\mu\nu}-\frac{1}{2}Rg_{\mu\nu} = 8\pi T_{\mu\nu}[/itex] gives [itex]R_{\mu\nu} = 8\pi \left( T_{\mu \nu} - \frac{1}{2}T^\alpha_\alpha g_{\mu\nu} \right)[/itex], another useful form of the EFE.
 
  • #3
Thanks, I always thought there was some index trickery involved in resolving this, but I never knew about multiple repeated indices being disallowed.
 

1. What is the Ricci scalar in Einstein's field equations (EFE)?

The Ricci scalar is a mathematical quantity used in Einstein's field equations to describe the curvature of spacetime. It is a measure of the intrinsic curvature at a specific point in spacetime and is calculated using the Riemann curvature tensor.

2. How does the Ricci scalar relate to the theory of general relativity?

The Ricci scalar is an important part of Einstein's general theory of relativity. It is used to describe the curvature of spacetime, which is the fundamental concept in general relativity. The Ricci scalar is included in the Einstein field equations, which are the cornerstone of the theory.

3. Can the Ricci scalar be used to solve Einstein's field equations?

Yes, the Ricci scalar is a crucial component in solving Einstein's field equations. It is used to calculate the energy-momentum tensor, which describes the distribution of energy and momentum in the universe. This, in turn, helps determine the curvature of spacetime and how objects move through it.

4. How is the Ricci scalar related to the energy and matter content of the universe?

The Ricci scalar is related to the energy and matter content of the universe through the energy-momentum tensor. This tensor is used in the Einstein field equations to describe the distribution of energy and matter in the universe, which ultimately affects the curvature of spacetime.

5. Is the Ricci scalar a constant or does it vary in different parts of the universe?

The Ricci scalar is not a constant and can vary in different parts of the universe. It depends on the distribution of energy and matter in that specific region of spacetime. In regions with high concentrations of matter, the Ricci scalar will be higher, indicating a higher curvature of spacetime.

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