Absolute stability limit for relativistic charged spheres

DOI10.1007/s10714-007-0539-7zbMath1148.83308arXiv0705.4452OpenAlexW2008279936MaRDI QIDQ937059

Alessandro Giuliani, Tony Rothman

Publication date: 20 August 2008

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

Full work available at URL: https://arxiv.org/abs/0705.4452

zbMATH Keywords

Reissner-Nordström solutionOppenheimer-Volkov equationExtremal black holesStellar stability

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (6)

Sharp bounds on the critical stability radius for relativistic charged spheres ⋮ Buchdahl compactness limit and gravitational field energy ⋮ An exact family of Einstein-Maxwell Wyman-Adler solution in general relativity ⋮ Charged anisotropic models with complexity-free condition ⋮ Regular models with quadratic equation of state ⋮ The Einstein-Vlasov system/kinetic theory

Cites Work

• Minimum mass-radius ratio for charged gravitational objects
• Microscopic origin of the Bekenstein-Hawking entropy
• General Relativistic Fluid Spheres
• Relativistic charged spheres: II. Regularity and stability
• The Large Scale Structure of Space-Time

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