THE SPHERICAL SYMMETRY BLACK HOLE COLLAPSE IN EXPANDING UNIVERSE

DOI10.1142/S0218271812500393zbMath1263.83089arXiv1102.1062MaRDI QIDQ4911494

Javad T. Firouzjaee

Publication date: 15 March 2013

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1102.1062

zbMATH Keywords

singularityapparent horizoncosmological black holes

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (7)

Cosmological black holes: the spherical perfect fluid collapse with pressure in a FRW background ⋮ Quasiperiodic oscillations, weak field lensing and shadow cast around black holes in symmergent gravity ⋮ Energy condition and cosmic censorship conjecture in the perfect fluid collapse ⋮ Cosmic matter flux may turn Hawking radiation off ⋮ Conformally Schwarzschild black holes in an accelerating universe ⋮ Complete solutions to the metric of spherically collapsing dust in an expanding spacetime with a cosmological constant ⋮ Primordial black holes in linear and non-linear regimes

Cites Work

• Asymptotically FRW black holes
• Dynamical Horizons: Energy, Angular Momentum, Fluxes, and Balance Laws
• Structures in the Universe by Exact Methods
• Strengths of naked singularities in Tolman-Bondi spacetimes
• The Mass-Particle in an Expanding Universe
• Black hole evaporation in an expanding universe
• Generic Isolated Horizons and Their Applications
• The Influence of the Expansion of Space on the Gravitation Fields Surrounding the Individual Stars
• Corrections and Additional Remarks to our Paper: The Influence of the Expansion of Space on the Gravitation Fields Surrounding the Individual Stars
• General Relativity

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