Black holes in the turbulence phase of viscous rip cosmology

DOI10.1142/S0219887819500300zbMath1411.83142arXiv1901.00002OpenAlexW3103289550MaRDI QIDQ4625458

Iver Brevik, Mubasher Jamil

Publication date: 22 February 2019

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

Full work available at URL: https://arxiv.org/abs/1901.00002

zbMATH Keywords

singularityblack holelate universephantom fluidviscous universeturbulent universe

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Isotropic turbulence; homogeneous turbulence (76F05)

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Cites Work

• Generalized second law of thermodynamics for a phantom energy accreting BTZ black hole
• Primordial black holes in phantom cosmology
• Black holes in bulk viscous cosmology
• Quantum de Sitter cosmology and phantom matter
• Turbulence accelerating cosmology from an inhomogeneous dark fluid
• Dark energy and viscous cosmology
• Characteristic properties of two different viscous cosmology models for the future universe
• LITTLE RIP COSMOLOGICAL MODELS WITH TIME-DEPENDENT EQUATION OF STATE
• Spherical accretion by normal and phantom Einstein–Maxwell–dilaton black holes
• Viscous cosmology for early- and late-time universe
• Accretion on Reissner–Nordström–(anti)-de Sitter black hole with global monopole

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