Role of equation of states and thermodynamic potentials in avoidance of trapped surfaces in gravitational collapse
DOI10.1007/s10714-019-2653-8zbMath1437.83049arXiv1903.01126OpenAlexW2919213088WikidataQ126558170 ScholiaQ126558170MaRDI QIDQ2294993
Terricia Govender, Rituparno Goswami
Publication date: 12 February 2020
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1903.01126
Applications of differential geometry to physics (53Z05) Space-time singularities, cosmic censorship, etc. (83C75) 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)
Cites Work
- Unnamed Item
- Singularity theorems and their consequences
- Generalized Vaidya solutions.
- Cosmic censorship conjecture revisited: covariantly
- Interiors of Vaidya's radiating metric: Gravitational collapse
- Spherically symmetric models for charged stars and voids: I. Charge bound
- Spherically symmetric models for stars and voids II: constraints on the radial pressures
- SPHERICAL COLLAPSE WITH HEAT FLOW AND WITHOUT HORIZON
- Relativistic Cosmology
- Gravitational Collapse and Spacetime Singularities
- The Large Scale Structure of Space-Time
- On Continued Gravitational Contraction
This page was built for publication: Role of equation of states and thermodynamic potentials in avoidance of trapped surfaces in gravitational collapse
