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Main Authors: Beltracchi, Philip, Posada, Camilo
Format: Preprint
Published: 2023
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Online Access:https://arxiv.org/abs/2305.09544
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author Beltracchi, Philip
Posada, Camilo
author_facet Beltracchi, Philip
Posada, Camilo
contents We reconsider the problem of a slowly rotating homogeneous star, or Schwarzschild star, when its compactness goes beyond the Buchdahl bound and approaches the gravastar limit $R\to 2M$. We compute surface and integral properties of such configuration by integrating the Hartle-Thorne structure equations for slowly rotating relativistic masses, at second order in angular velocity. In the gravastar limit, we show that the metric of a slowly rotating Schwarzschild star agrees with the Kerr metric, thus, within this approximation, it is not possible to tell a gravastar from a Kerr black hole by any observations from the spacetime exterior to the horizon.
format Preprint
id arxiv_https___arxiv_org_abs_2305_09544
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Slowly rotating ultracompact Schwarzschild star in the gravastar limit
Beltracchi, Philip
Posada, Camilo
General Relativity and Quantum Cosmology
We reconsider the problem of a slowly rotating homogeneous star, or Schwarzschild star, when its compactness goes beyond the Buchdahl bound and approaches the gravastar limit $R\to 2M$. We compute surface and integral properties of such configuration by integrating the Hartle-Thorne structure equations for slowly rotating relativistic masses, at second order in angular velocity. In the gravastar limit, we show that the metric of a slowly rotating Schwarzschild star agrees with the Kerr metric, thus, within this approximation, it is not possible to tell a gravastar from a Kerr black hole by any observations from the spacetime exterior to the horizon.
title Slowly rotating ultracompact Schwarzschild star in the gravastar limit
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2305.09544