Surrounded Vaidya black holes: apparent horizon properties

Abstract

We study the thermodynamical features and dynamical evolutions of various apparent horizons associated with the Vaidya evaporating black hole surrounded by the cosmological fields of dust, radiation, quintessence, cosmological constant-like and phantom. In this regard, we address in detail how do these surrounding fields contribute to the characteristic features of a surrounded dynamical black hole in comparison to a dynamical black hole in an empty background.

arXiv comment23 pages

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Cited by in corpus (8)

• Hairy Kiselev Black Hole Solutions
• Surrounded Vaidya Solution by Cosmological Fields
• On quasinormal modes for the Vaidya metric in asymptotically anti-de Sitter spacetime
• Dynamical Photon Spheres in Charged Black Holes and Naked Singularities
• Generalized Vaidya spacetime: horizons, conformal symmetries, surface gravity and diagonalization
• D-bound and Bekenstein Bound for the Surrounded Vaidya Black Hole
• Gravitational wave pulse and memory effects for hairy Kiselev black hole and its analogy with Bondi-Sachs formalism
• Generalized Vaidya Spacetime in Cotton and Conformal Killing Theories