The vacuum Einstein equations and flat spacetime

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Discussion Overview

The discussion revolves around the vacuum Einstein equations (VEE) in general relativity (GR), specifically addressing the implications of a zero Ricci tensor and the nature of spacetime curvature in the absence of matter. Participants explore concepts related to flat and curved spacetimes, the role of fields, and the interpretation of vacuum states.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • Some participants note that the VEE (Rab=0) indicates that spacetime can be curved even without matter, raising the question of what causes this curvature.
  • One participant suggests that nearby matter creates a field that extends into space, influencing the curvature of spacetime.
  • Another participant questions whether the absence of matter or fields in a vacuum implies that spacetime is flat, seeking clarification on the nature of vacuum in GR.
  • Some argue that spacetime can be curved in the absence of matter, using the example of an isolated spherical star where the outside solution is the curved vacuum Schwarzschild solution.
  • There is a discussion about the analogy of electric fields existing without charges, suggesting that curvature can exist independently of mass.
  • One participant introduces the Friedmann-Robertson-Walker metric with zero density, indicating that curvature can exist without mass or energy.
  • Another participant presents mathematical expressions related to the Ricci components and scalar curvature in the context of the FLRW metric, emphasizing the complexity of curvature in different scenarios.

Areas of Agreement / Disagreement

Participants generally agree that spacetime can be curved in the absence of matter, but there is no consensus on the specific mechanisms or interpretations of this phenomenon. Multiple competing views remain regarding the nature of vacuum and the role of fields in curving spacetime.

Contextual Notes

Participants express uncertainty about the implications of vacuum states, the definitions of total energy in flat versus curved spacetimes, and the historical context of GR in relation to quantum field theory. There are unresolved mathematical steps and assumptions regarding curvature and energy-momentum tensors.

xiaomaclever
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Rencently, I found myself confused by some fundamental concepts in GR. I hope someone can help me with that.

We all know the vacuum Einstein equation (VEE) without the cosmological constant \Lambda is Rab=0. Since I learn GR the words " matters bend the spacetime " been told again and again. I know the zero Rici tensor does not mean flat spacetime while the zero Riemann tensor do. So the VEE means spacetime may be still curved without matter. Who curves it?
Until now we have many solutions for the VEE, which one is the real metric if there are really this vacuum state? Is this a paradox? I feel a flat spacetime is better in vacuum so that it is the only one .

Another question. If we are in flat spacetime, e.g. Minkowski spacetime,the Ricci tensor is zero. According to the general Einstein equation the energy momentum tensor should also be zero. Whether that means the total energy must be zero in flat spacetime. What about curved spacetime?

Thanks !
 
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Hi xiaomaclever,


We all know the vacuum Einstein equation (VEE) without the cosmological constant \Lambda is Rab=0. Since I learn GR the words " matters bend the spacetime " been told again and again. I know the zero Rici tensor does not mean flat spacetime while the zero Riemann tensor do. So the VEE means spacetime may be still curved without matter. Who curves it?
The matter nearby curves it. Just think of classical fields. The matter creates a field [itex]g_{\mu\nu}[/itex] which extends into the space around it. This field isn't the same as an electric fileld, but it shares that property.

Another question. If we are in flat spacetime, e.g. Minkowski spacetime,the Ricci tensor is zero. According to the general Einstein equation the energy momentum tensor should also be zero. Whether that means the total energy must be zero in flat spacetime. What about curved spacetime?
I'm not sure what you mean by 'total energy'. Are you using a quantum field analogy ?
 
Do you mean the fields curve the spacetime? I know in QFT the vacuum is not nothing but with the fields which all reside in the ground states, namely no excitations. So this case it will still have vacuum energy which will curve the spacetime. But you should know at the time of GR's generation the QFT was not found. Certainly I don't know what is the vacuum in Einstein's mind. I want to know if there is noting in vacuum,no matter,no fields,Is spacetime curved?
 
Yes, spacetime can be curved in the local absence of matter. Take an isolated spherical star. Inside the star there is matter, and the solution is not the vacuum Schwarzschild solution. Outside the star, there is no matter, and by Birkhoff's theorem, the solution is the vacuum Schwarzschild solution, which is curved.
 
atyy said:
Yes, spacetime can be curved in the local absence of matter. Take an isolated spherical star. Inside the star there is matter, and the solution is not the vacuum Schwarzschild solution. Outside the star, there is no matter, and by Birkhoff's theorem, the solution is the vacuum Schwarzschild solution, which is curved.

you do not explain who curves the spacetime in vacuum, that's my question.
 
atyy said:
Yes, spacetime can be curved in the local absence of matter.

As an analogy, an electric field can exist at a certain point in space even though there is no charge at that point. The field at that point is determined by the field at nearby points according to Laplace's equation.
 
It might help to note that "curved" has two distinct meanings which can be illustrated in 3D by the curvature of part of a cone (which can be locally matched by a flat piece of paper) and the curvature of part of a sphere (which cannot).

Loosely speaking the space-time curvature of the gravitational field outside a mass-energy distribution is like the curvature of part of a cone, and the space-time curvature inside a mass-energy distribution is like the curvature of part of a sphere.
 
xiaomaclever said:
you do not explain who curves the spacetime in vacuum, that's my question.

Curvature can be an intrinsic property of spacetime, it is not necessary to have mass. Think of the Friedmann-Robertson-Walker-metric with rho=0 and k=+-1. Also, there is no a priori reason why the background metric of spacetime shouldn't be the Schwarzschild metric. M would then be an arbitrary parameter instead of some Newtonian mass. Of course this does not agree with our observations of an homogeneous universe, but theoretically it's thinkable.
You can also think of it as living on a sphere (of any dimension). It is curved, even if there is no mass on it. Or (anti) de Sitter-spaces.


So what I'm trying to say: Mass does bend spacetime, but that doesn't mean spacetime can't be bent without mass or energy.
 
  • #10
amanheis raises an interesting case. For the FLRW the first two Ricci components are

[tex] R_{00}=-\frac{3\,\partial t\left( \partial t R\left( t\right) \right) }{R\left( t\right) }[/tex]

[tex] R_{11}=-\frac{R\left( t\right) \,\partial t\left( \partial t\left( R\left( t\right) \right) \right) +2\,{\partial t\left( R\left( t\right) \right) }^{2}+2\,k}{k\,{r}^{2}-1}[/tex]

and the scalar curvature is

[tex] R=\frac{6\,\left( R\left( t\right) \,\partial t\left( \partial t\left( R\left( t\right) \right) \right) +{\partial t\left( R\left( t\right) \right) }^{2}+k\right) }{{R\left( t\right) }^{2}}[/tex]

where k is -1,0 or 1.

Draw your own conclusions. If all the derivatives are zero ( static universe ) then there is still spatial curvature and a non-zero scalar curvature if k is not 0.

The greatest effect comes from the expansion itself.
 

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