A ambiguous variation of Einstein-Hilbert action

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In summary, the conversation discusses the variation of Einstein-Hilbert action and its implications for the vacuum field equations. It is proven that there is no need to consider an antisymmetric tensor in the equations, as the energy-momentum tensor is already symmetric and the metric is also symmetric. However, any antisymmetric tensor added to the equations must be divergenceless in order to satisfy covariant energy-momentum conservation.
  • #1
archipatelin
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A ambiguous variation of Einstein--Hilbert action

Variation of EH action is:
[tex]
\delta S_{EH}=\int_{\Omega}{\delta(R\sqrt{-g})dx^4}=
\int_{\Omega}{G_{\mu\nu}\delta{g^{\mu\nu}}\sqrt{-g}dx^4}=0,
[/tex]​
where
[tex]
G_{\mu\nu}:=R_{\mu\nu}-\frac{1}{2}g_{\mu\nu}R
[/tex]​
is symmetric einstein's tensor.

The action have to be extremal for each volume [tex]\Omega[/tex]. This implicate
[tex]
G_{\mu\nu}\delta{g^{\mu\nu}}=0.
[/tex]​
Becouse variation of metric is arbitrary and [tex]G_{\mu\nu}[/tex] is principal independed on [tex]\delta{g^{\mu\nu}}[/tex], latest equation is equivalent with
[tex]
G_{\mu\nu}=0.
[/tex]​
This are ordinary einstein's vacuum equations.

But variation of metric is symmetric tensor, therefore more general form of vacuum
field equations are
[tex]
S_{\mu\nu}:=G_{(\mu\nu)}+F_{[\mu\nu]}=0,
[/tex]​
where [tex]F_{\mu\nu}[/tex] is whatever antisymmetric tensor build it from metric and its derivations.

Why we can ignore this tensor (it is proven that there is not exist)?
 
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  • #2


Because the righthand side is the energy momentum tensor, which per definition is symmetric (well, for special-relativistic field theories this is not entirely true, which is the cause for the need of something called the Belinfante tensor).

Also, the metric is symmetric, so theoretically you could add ANY antisymmetric tensor to your expression, because contracting it with [itex]\delta g_{\mu\nu}[/itex] gives zero anyway. However, this term has to be divergenceless due to covariant energy-momentum conservation. Which tensor should that be?
 

1. What is the Einstein-Hilbert action?

The Einstein-Hilbert action is a mathematical expression used in the theory of general relativity to describe the dynamics of spacetime. It is a way to express the gravitational field equations, which describe how matter and energy interact with the geometry of spacetime.

2. What do you mean by "ambiguous variation" of the Einstein-Hilbert action?

The ambiguous variation of the Einstein-Hilbert action refers to a modified version of the original action that includes additional terms or factors. This variation is often used in theoretical physics to explore alternative theories of gravity or to incorporate new physical concepts.

3. How does the "ambiguous variation" affect the predictions of general relativity?

The ambiguous variation can lead to different predictions compared to the original Einstein-Hilbert action. This can result in new or modified equations of motion for particles and fields, and potentially lead to different predictions for the behavior of gravity in extreme conditions, such as near black holes.

4. What are some examples of "ambiguous variations" of the Einstein-Hilbert action?

Some examples include the f(R) theory, where the Ricci scalar in the action is replaced by a function of the Ricci scalar, and the Gauss-Bonnet theory, where an additional term involving the Gauss-Bonnet curvature is added to the action. These variations are often motivated by attempts to reconcile general relativity with quantum mechanics or to explain the accelerating expansion of the universe.

5. How do scientists test the validity of "ambiguous variations" of the Einstein-Hilbert action?

Scientists can test these variations by comparing their predictions to experimental or observational data. For example, they can compare the predictions of the f(R) theory to the observed rotation curves of galaxies or to the behavior of gravitational waves. They can also use mathematical tools, such as perturbation theory, to analyze the behavior of these variations in specific scenarios.

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