Nested solutions of gravitational condensate stars

DOI10.1088/1361-6382/AD2317arXiv2310.13946OpenAlexW4391837333MaRDI QIDQ6153392

Luciano Rezzolla, Unnamed Author

Publication date: 19 March 2024

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2310.13946

zbMATH Keywords

black holesgravitational collapseanisotropic starsgravastarsgravitational condensate stars

Mathematics Subject Classification ID

Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Cites Work

• Lorentzian causality theory
• Relativistic Hydrodynamics
• General Relativistic Fluid Spheres
• Where are all the gravastars? Limits upon the gravastar model from accreting black holes
• Surface tension and negative pressure interior of a non-singular ‘black hole’
• How to tell a gravastar from a black hole
• Constraints on horizonless objects after the EHT observation of Sagittarius A*
• Gravastar: An alternative to black hole
• Stability of a vacuum non-singular black hole
• Gravastars must have anisotropic pressures
• A connection between regular black holes and horizonless ultracompact stars

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