When Painlevé–Gullstrand coordinates fail

Abstract Painlevé–Gullstrand coordinates, a very useful tool in spherical horizon thermodynamics, fail in anti-de Sitter space and in the inner region of Reissner–Nordström. We predict this breakdown to occur in any region containing negative Misner–Sharp–Hernandez quasilocal mass because of repulsi...

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Main Authors: Valerio Faraoni, Geneviève Vachon
Format: Article
Language:English
Published: SpringerOpen 2020-08-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-020-8345-4
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author Valerio Faraoni
Geneviève Vachon
author_facet Valerio Faraoni
Geneviève Vachon
author_sort Valerio Faraoni
collection DOAJ
description Abstract Painlevé–Gullstrand coordinates, a very useful tool in spherical horizon thermodynamics, fail in anti-de Sitter space and in the inner region of Reissner–Nordström. We predict this breakdown to occur in any region containing negative Misner–Sharp–Hernandez quasilocal mass because of repulsive gravity stopping the motion of PG observers, which are in radial free fall with zero initial velocity. PG coordinates break down also in the static Einstein universe for completely different reasons. The more general Martel-Poisson family of charts, which normally has PG coordinates as a limit, is reported for static cosmologies (de Sitter, anti-de Sitter and the static Einstein universe).
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spelling doaj.art-3997ea7240f444f689e2042edc599ecb2022-12-21T23:46:08ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-08-018081910.1140/epjc/s10052-020-8345-4When Painlevé–Gullstrand coordinates failValerio Faraoni0Geneviève Vachon1Department of Physics and Astronomy, Bishop’s UniversityDepartment of Physics and Astronomy, Bishop’s UniversityAbstract Painlevé–Gullstrand coordinates, a very useful tool in spherical horizon thermodynamics, fail in anti-de Sitter space and in the inner region of Reissner–Nordström. We predict this breakdown to occur in any region containing negative Misner–Sharp–Hernandez quasilocal mass because of repulsive gravity stopping the motion of PG observers, which are in radial free fall with zero initial velocity. PG coordinates break down also in the static Einstein universe for completely different reasons. The more general Martel-Poisson family of charts, which normally has PG coordinates as a limit, is reported for static cosmologies (de Sitter, anti-de Sitter and the static Einstein universe).http://link.springer.com/article/10.1140/epjc/s10052-020-8345-4
spellingShingle Valerio Faraoni
Geneviève Vachon
When Painlevé–Gullstrand coordinates fail
European Physical Journal C: Particles and Fields
title When Painlevé–Gullstrand coordinates fail
title_full When Painlevé–Gullstrand coordinates fail
title_fullStr When Painlevé–Gullstrand coordinates fail
title_full_unstemmed When Painlevé–Gullstrand coordinates fail
title_short When Painlevé–Gullstrand coordinates fail
title_sort when painleve gullstrand coordinates fail
url http://link.springer.com/article/10.1140/epjc/s10052-020-8345-4
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