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Ziaie, Amir Hadi; Tavakoli, Yaser

Null fluid collapse in Rastall theory of gravity. (English) Zbl 07765110

Ann. Phys., Berlin 532, No. 10, Article ID 2000064, 12 p. (2020).
Summary: A Vaidya spacetime is considered for gravitational collapse of a type II fluid in the context of the Rastall theory of gravity. For a linear equation of state for the fluid profiles, the conditions under which the dynamical evolution of the collapse can give rise to the formation of a naked singularity are examined. It is shown that depending on the model parameters, strong curvature, naked singularities would arise as exact solutions to the Rastall’s field equations. The allowed values of these parameters satisfy certain conditions on the physical reliability, nakedness, and the curvature strength of the singularity. It turns out that Rastall gravity, in comparison to general relativity, provides a wider class of physically reasonable spacetimes that admit both locally and globally naked singularities.
© 2020 The Authors. Published by Wiley-VCH GmbH

Cited in 2 Documents

MSC:

83C57 Black holes
83C75 Space-time singularities, cosmic censorship, etc.
83D05 Relativistic gravitational theories other than Einstein’s, including asymmetric field theories

Keywords:

black holes; gravitational collapse; modified theories of gravity; naked singularities
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