Example of curvature scalar diverging at infinity?

Overall, Geroch's article highlights the important distinction between true singularities and apparent singularities in general relativity. In summary, polynomial scalar invariants constructed from the Riemann tensor can diverge at infinite distance, indicating an apparent singularity rather than a true singularity. An example of this is seen in the Schwarzschild metric, where the Kretschmann scalar diverges at infinite distance, suggesting the presence of a singularity. This distinction is important in understanding the concept of singularities in general relativity.
  • #1
jinawee
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Reading Geroch's "What is a Singularity in General Relativity?", it seems that polynomial scalar invariants constructed from the Riemann tensor can diverge if we are at infinite distance, and not in a true singularity.

Can someone give an example of space-time whose scalar invariant diverges at infinity?
 
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  • #2


Sure, here is an example of a space-time whose scalar invariant diverges at infinity:

Consider the Schwarzschild metric, which describes the space-time around a non-rotating, spherically symmetric mass. The scalar invariant in this case is the Kretschmann scalar, given by:

K = R_abcdR^abcd

where R_abcd is the Riemann tensor. In this metric, as we approach infinite distance (r → ∞), the Kretschmann scalar diverges, indicating a singularity at infinity. This can be seen by calculating the Kretschmann scalar at different values of r:

At r = 2M (where M is the mass of the object), K = 48M^2/r^6
As r → ∞, K → ∞

This shows that the scalar invariant diverges at infinity in the Schwarzschild metric, indicating the presence of a singularity at infinite distance.
 

Related to Example of curvature scalar diverging at infinity?

1. What is a curvature scalar diverging at infinity?

A curvature scalar diverging at infinity is a mathematical concept used in the study of curved spaces, such as in Einstein's theory of general relativity. It refers to a scalar quantity, which measures the overall curvature of a space, becoming infinitely large as the distance from a given point in the space approaches infinity.

2. What is an example of a curvature scalar diverging at infinity?

An example of a curvature scalar diverging at infinity is the Schwarzschild metric, which describes the curvature of space around a non-rotating, spherical mass. As the distance from the mass increases, the curvature scalar becomes infinitely large, indicating that the space becomes more and more curved.

3. Why is a curvature scalar diverging at infinity important in general relativity?

A curvature scalar diverging at infinity is important in general relativity because it is used to describe the gravitational field around massive objects, such as stars and planets. This allows us to understand how the curvature of space affects the motion of objects in the presence of gravity.

4. How is a curvature scalar diverging at infinity related to the concept of spacetime curvature?

A curvature scalar diverging at infinity is directly related to the concept of spacetime curvature, as it is a measure of the overall curvature of a space. In general relativity, gravity is described as the curvature of spacetime, and a curvature scalar diverging at infinity indicates a strong gravitational field in that region of space.

5. Can a curvature scalar diverging at infinity be negative?

Yes, a curvature scalar diverging at infinity can be negative. This means that the space is negatively curved, which is a characteristic of an expanding universe. In general relativity, this is referred to as a negative cosmological constant, which is thought to be responsible for the observed acceleration of the expansion of the universe.

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