Non static and isotropic solution for Einstein Field Eq

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Discussion Overview

The discussion revolves around the characteristics of non-static and spherically symmetric solutions to the Einstein field equations, particularly focusing on the presence of non-diagonal terms in the Ricci tensor. Participants explore theoretical implications, mathematical formulations, and the distinctions between isotropic and anisotropic solutions.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant questions whether a non-diagonal term, specifically R[r][t], appears in the Ricci tensor for non-static, spherically symmetric solutions.
  • Another participant clarifies that spherically symmetric solutions are not isotropic and notes that the Ricci tensor is zero in vacuum solutions, while non-vacuum solutions will have an (r,t) term.
  • Some participants argue that FRW spacetime is both spherically symmetric and isotropic, contrasting it with Schwarzschild spacetime, which is not isotropic.
  • There is a discussion on the formulation of the "non-static" assumption, with references to using a metric ansatz involving angular coordinates and functions of r and t.
  • Participants express interest in the mathematical details and formulations used to derive results, with references to specific equations in Synge's book.
  • One participant mentions Birkhoff's theorem, stating that any spherically symmetric solution of the vacuum Einstein equation is static, while noting the conditions under which this holds.
  • Another participant indicates they are new to general relativity and seeking to understand these concepts better.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between spherically symmetric and isotropic solutions, and there is no consensus on the implications of the non-static assumption or the presence of non-diagonal terms in the Ricci tensor.

Contextual Notes

There are unresolved aspects regarding the definitions of isotropy and the implications of Birkhoff's theorem, as well as the specific mathematical formulations that lead to different conclusions about the nature of the solutions.

Leonardo Machado
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Hello dear friends, today's question is:

In a non static and spherically simetric solution for Einstein field equation, will i get a non diagonal term on Ricci tensor ? A R[r][/t] term ?

I'm getting it, but not sure if it is right.

Thanks.
 
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Note that spherically symmetric is not the same as isotropic. Your title says one, your post says another. A spherically symmetric solution is anisotropic.

Isoptropic, non-static solutions include all the FLRW solutions except where cosmological constant exactly balances the expansion.

The spherically symmetric non-static vacuum solution is unique (without cosmological constant, at least). It is the interior of an eternal Schwarzschild BH. The Ricci tensor is identically zero because it is vacuum. For non-vacuum solutions, you will, indeed get an (r,t) Ricci term (given normal meaning of such coordinates). This should be the only non diagonal term [ noting (r,t) obviously = (t,r) term].
 
PAllen said:
A spherically symmetric solution is anisotropic.

This is not quite correct. FRW spacetime is spherically symmetric and also isotropic. The key is that FRW spacetime is spherically symmetric about every point. A spacetime like Schwarzschild spacetime, which is not isotropic, is not.

More technically: "spherically symmetric" means there is a 3-parameter family of spacelike Killing vector fields with the commutation relations of SO(3). But that does not preclude there being more than one such family. In FRW spacetime, there is an infinite number of such families (one centered on each spatial point--and to be really technical, there is such an infinite family in each spacelike hypersurface, instead of just one as there is in Schwarzschild spacetime).
 
Leonardo Machado said:
I'm getting it, but not sure if it is right.

Can you post your actual math?
 
PeterDonis said:
Can you post your actual math?
Is there some reason you want this? For non-vacuum case, the existence of this term is well known.
 
PAllen said:
Is there some reason you want this?

I'm interested in how the "non-static" assumption is formulated.
 
PeterDonis said:
I'm interested in how the "non-static" assumption is formulated.
You just use a metric ansatz with angular coordinates, and two unknown functions of r and t. Different formulations of the ansatz lead to different styles of coordinates. In all such set ups, you find the Ricci tensor is diagonal except for the r,t components. One reference for this is chapter 7, section 3, of Synge's book.
 
PAllen said:
You just use a metric ansatz with angular coordinates, and two unknown functions of r and t.

Are you referring to equations (70) and (71) of Synge? The first is a general ansatz with three unknown functions, and the second gives different specializations that determine one of the functions in terms of the other two.
 
Yes, that's the way Birkhoff's theorem is proven, i.e., you make a ansatz for a spherically symmetric solution of the free Einstein equation. Then you'll get out that in fact the metric components are necessarily time-independent, i.e., any spherically symmetric solution of the vacuum Einstein equation is static.
 
  • #10
PeterDonis said:
Are you referring to equations (70) and (71) of Synge? The first is a general ansatz with three unknown functions, and the second gives different specializations that determine one of the functions in terms of the other two.
Yes. Or, as is done earlier in that chapter, simpler forms of the ansatz for different coordinate styles are given. Those equations (70, 71) use a most general form to derive universal results.
 
  • #11
vanhees71 said:
Yes, that's the way Birkhoff's theorem is proven, i.e., you make a ansatz for a spherically symmetric solution of the free Einstein equation. Then you'll get out that in fact the metric components are necessarily time-independent, i.e., any spherically symmetric solution of the vacuum Einstein equation is static.
Note, Birkhoff really states the existence of an extra killing field. Only if it is time like do you then get staticity. Thus, the BH exterior is static, while the interior is not because dt is space like in the interior, so you have an axial extra killing field.
 
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  • #12
PAllen said:
Is there some reason you want this? For non-vacuum case, the existence of this term is well known.

I'm coursing general relativity for the first time, first contact with these strange spaces. :wink:
 

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