Curvature Singularity: Necessary & Sufficient Conditions

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SUMMARY

The discussion centers on the necessary and sufficient conditions for curvature singularities in general relativity. It is established that the presence of geodesic incompleteness serves as a general criterion for identifying singularities, while scalar quantities derived from the Riemann tensor can indicate singular behavior. The conversation highlights that finding a coordinate system where the metric is nonsingular does not negate the existence of a singularity, particularly in cases like the Schwarzschild metric at r=0. The complexity of defining singularities is underscored, referencing the work of Hawking and Penrose and the importance of scalar and tensor curvatures.

PREREQUISITES
  • Understanding of general relativity and Einstein's Field Equations
  • Familiarity with Riemannian geometry and curvature tensors
  • Knowledge of geodesic incompleteness and its implications
  • Basic concepts of scalar and tensor quantities in physics
NEXT STEPS
  • Study Hawking and Penrose's singularity theorems for deeper insights
  • Explore Wald's "General Relativity" chapter 9 for detailed criteria on singularities
  • Investigate the implications of geodesic incompleteness in various metrics
  • Learn about the Schwarzschild solution and its coordinate systems
USEFUL FOR

Physicists, mathematicians, and students of general relativity seeking to understand the complexities of curvature singularities and their implications in theoretical physics.

binbagsss
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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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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.
 
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.
 
Last edited:
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 e there is a neighborhood that can be described with nonsingular coordinates. So in that sense, there are no singularities. The point (or line, actually r=0 is not part of the manifold, strictly speaking. That's why "geodesic incompleteness" is relevant. A timelike geodesic in the neighborhood of r=0 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.
 
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 e there is a neighborhood that can be described with nonsingular coordinates. So in that sense, there are no singularities. The point (or line, actually r=0 is not part of the manifold, strictly speaking. That's why "geodesic incompleteness" is relevant. A timelike geodesic in the neighborhood of r=0 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?
 
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.
 

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