Curvature Singularity: Necessary & Sufficient Conditions

In summary: But physically, you might be more interested in whether the Lorentzian manifold is well-behaved or not. That's a tensorial object, and it can't be tested with scalars. So the definition of a curvature singularity is more subtle and involves geodesic incompleteness.In summary, the necessary and sufficient conditions for a singularity are complex and not always dependent on one specific factor, such as a scalar quantity blowing up. A singularity can also be present even if the metric is no longer singular at a specific point, and it ultimately comes down to the presence of geodesic incompleteness in the Lorentzian manifold.
  • #1
binbagsss
1,254
11
For a physical singularity I think it is sufficient that anyone scalar quantity blows up,
Why is it not a necessary condition that all blow up?

For a curvature singularity am I correct in thinking that it is a sufficient condition to find a coordinate system in which the metric coefficient no longer blows up at that point?

Is the only necessary condition for a curvature singularity to check that all non scalar quantites are not infinite?

Thanks.
 
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  • #2
The necessary and sufficient conditions for a singularity are non-trivial. It is not always necessary or sufficient for anyone of the scalar curvatures or tensor curvatures or metric coefficients to "blow up". Indeed, even the definition of a singularity itself is complicated. This is why Hawking and Penrose (and others) worked so hard on their singularity theorems. There are cases where the scalar curvature is 0 everywhere, but the curvature tensor can be singular. Or There can be cases where the scalar curvatures or curvature tensor itself is singular only "at infinity" where no observer can reach.

The best, most general, criterion we have of a singularity, as best as we can figure, is the presence of geodesic incompleteness.

See Wald chapter 9 for details.
 
  • #3
Matterwave said:
The necessary and sufficient conditions for a singularity are non-trivial. It is not always necessary or sufficient for anyone of the scalar curvatures or tensor curvatures or metric coefficients to "blow up". .

In lecture notes on GR by Sean.M. Carroll he has that a sufficient condition to prove a singularity is that if there exists any (and not all) scalar quantity constructed from the Riemann tensor that goes to infinity at some point, the point is a singularity.

I don't understand how finding a coordinate system in which the metric is no longer singular at some point can not be a sufficient condition to disprove a signularty ? Does anyone have any examples, e.g. a coordinate system in which the singular nature of r=0 dissapears for the Schwarzschild metric,

thanks.
 
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  • #4
binbagsss said:
I don't understand how finding a coordinate system in which the metric is no longer singular at some point can not be a sufficient condition to disprove a signularty ? Does anyone have any examples, e.g. a coordinate system in which the singular nature of r=0 dissapears for the Schwarzschild metric,

Your suggestion is a little complicated to carry out, for the following reason: By definition, any solution of Einstein's Field Equations is a pseudo-Riemannian manifold, which means that for any event [itex]e[/itex] there is a neighborhood that can be described with nonsingular coordinates. So in that sense, there are no singularities. The point (or line, actually [itex]r=0[/itex] is not part of the manifold, strictly speaking. That's why "geodesic incompleteness" is relevant. A timelike geodesic in the neighborhood of [itex]r=0[/itex] will, in a finite amount of proper time, leave the manifold. Or said another way, there is a maximum finite amount of proper time such that the geodesic cannot be extended past that time.
 
  • #5
stevendaryl said:
Your suggestion is a little complicated to carry out, for the following reason: By definition, any solution of Einstein's Field Equations is a pseudo-Riemannian manifold, which means that for any event [itex]e[/itex] there is a neighborhood that can be described with nonsingular coordinates. So in that sense, there are no singularities. The point (or line, actually [itex]r=0[/itex] is not part of the manifold, strictly speaking. That's why "geodesic incompleteness" is relevant. A timelike geodesic in the neighborhood of [itex]r=0[/itex] will, in a finite amount of proper time, leave the manifold. Or said another way, there is a maximum finite amount of proper time such that the geodesic cannot be extended past that time.

And so the definition of a curvature singulairty is not a singularity that can be removed by good choice of coordinates?
Instead what's a good definition for curvature and physical singularity?
 
  • #6
binbagsss said:
the definition of a curvature singulairty is not a singularity that can be removed by good choice of coordinates?

Correct. Note that the definitions people have been giving you involve scalars going to infinity. A scalar is an invariant and can't be changed by changing coordinates.
 

1. What is a curvature singularity?

A curvature singularity is a point in space-time where the curvature of space-time becomes infinite. This means that any physical quantities, such as density or temperature, also become infinite at this point.

2. What are the necessary conditions for a curvature singularity to exist?

The necessary conditions for a curvature singularity to exist are a strong gravitational field and matter that is compressed to an infinitely small point. This occurs in black holes and the Big Bang singularity, for example.

3. Are there any sufficient conditions for a curvature singularity to exist?

Yes, there are sufficient conditions for a curvature singularity to exist. These include an infinite density of matter, a point of infinite curvature in space-time, and a breakdown of the laws of physics.

4. Can a curvature singularity be avoided or prevented?

There is currently no known way to avoid or prevent a curvature singularity from occurring. However, some theories, such as string theory, propose the existence of a "cosmic censorship" principle that would prevent singularities from being observable.

5. How are curvature singularities related to the concept of space-time curvature?

Curvature singularities are directly related to the concept of space-time curvature. They occur when the curvature of space-time becomes infinite, indicating a point of infinite density and a breakdown of the laws of physics. Curvature singularities play a crucial role in our understanding of the universe and the behavior of matter and energy within it.

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