Nonexistence of closed timelike geodesics in Kerr spacetimes

Fuente: arXiv
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Auteur principal: Sanzeni, Giulio
Format: Preprint
Publié: 2024
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author Sanzeni, Giulio
author_facet Sanzeni, Giulio
contents The Kerr-star spacetime is the extension over the horizons and in the negative radial region of the Kerr spacetime. Despite the presence of closed timelike curves below the inner horizon, we prove that the timelike geodesics cannot be closed in the Kerr-star spacetime. Since the existence of closed null geodesics was ruled out by the author in Sanzeni [arXiv:2308.09631v3 (2024)], this result shows the absence of closed causal geodesics in the Kerr-star spacetime.
format Preprint
id arxiv_https___arxiv_org_abs_2409_09094
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Nonexistence of closed timelike geodesics in Kerr spacetimes
Sanzeni, Giulio
General Relativity and Quantum Cosmology
Differential Geometry
The Kerr-star spacetime is the extension over the horizons and in the negative radial region of the Kerr spacetime. Despite the presence of closed timelike curves below the inner horizon, we prove that the timelike geodesics cannot be closed in the Kerr-star spacetime. Since the existence of closed null geodesics was ruled out by the author in Sanzeni [arXiv:2308.09631v3 (2024)], this result shows the absence of closed causal geodesics in the Kerr-star spacetime.
title Nonexistence of closed timelike geodesics in Kerr spacetimes
topic General Relativity and Quantum Cosmology
Differential Geometry
url https://arxiv.org/abs/2409.09094