The model of the black hole enclosed in dust: the flat space case

DOI10.1007/S10714-017-2243-6zbMath1383.83065arXiv1602.01266OpenAlexW3104210507MaRDI QIDQ1707620

P. Jaluvkova, E. M. Kopteva, Zdeněk Stuchlík

Publication date: 3 April 2018

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1602.01266

zbMATH Keywords

black holegeodesicexact solutions of Einstein equationstest particlecosmological backgroundLemaitre-Tolman-Bondi solutionsLTB solution

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Applications of differential geometry to physics (53Z05) Exact solutions to problems in general relativity and gravitational theory (83C15) Equations of motion in general relativity and gravitational theory (83C10)

Cites Work

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• Asymptotically FRW black holes
• Cosmic matter flux may turn Hawking radiation off
• The possibility of cosmic acceleration via spatial averaging in Lemaître–Tolman–Bondi models
• Cosmological black holes: the spherical perfect fluid collapse with pressure in a FRW background
• Inhomogeneous Cosmological Models
• The Mass-Particle in an Expanding Universe
• Spherical Symmetry and Mass-Energy in General Relativity. I. General Theory
• Spherical Symmetry and Mass-Energy in General Relativity. II. Particular Cases

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