Einstein’s hole argument and Schwarzschild singularities

According to the Einstein hole argument, vacuum metric solutions are equivalent only if they correspond to the same energy–momentum tensor in the source region. In this paper it is shown that singular coordinates that are used to show Schwarzschild geodesics completeness, introduce the fictive delta...

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Bibliographic Details
Published in:Annals of physics Vol. 452; p. 169274
Main Author: Gogberashvili, Merab
Format: Journal Article
Language:English
Published: Elsevier Inc 01-05-2023
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Summary:According to the Einstein hole argument, vacuum metric solutions are equivalent only if they correspond to the same energy–momentum tensor in the source region. In this paper it is shown that singular coordinates that are used to show Schwarzschild geodesics completeness, introduce the fictive delta-like sources at the horizon. Then, metric tensors obtained by such singular transformations, cannot be considered as solutions of the same Einstein equations with the central source. •Schwarzschild metrics obtained by singular transformations are solutions of different Einstein equations.•The Regge–Wheeler radial variable should contain Heaviside function at the Schwarzschild horizon.•Particles do not cross Schwarzschild sphere, but are absorbed and some reflected by the horizon.
ISSN:0003-4916
1096-035X
DOI:10.1016/j.aop.2023.169274