Spherical gravitational collapse: Tangential pressure and related equations of state

DOI10.1023/A:1001919219247zbMath0964.83018arXivgr-qc/9901080MaRDI QIDQ1585713

R. Smith

Publication date: 17 July 2001

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

Full work available at URL: https://arxiv.org/abs/gr-qc/9901080

zbMATH Keywords

cosmic censorshipspherical collapse

Mathematics Subject Classification ID

Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (8)

Three-layered compact star in modified Buchdahl-I spatial metric with distinct equations of state ⋮ Inhomogeneities as a possible factor responsible for the acceleration of the universe: a \((2+1)\)-gravity study ⋮ Gravitational collapse with tachyon field and barotropic fluid ⋮ Naked singularity formation in \(f(\mathcal R)\) gravity ⋮ Static vacuum solutions in non-Riemannian gravity ⋮ Influence of intrinsic spin in the formation of singularities for inhomogeneous effective dust space-times ⋮ The geometry of black hole singularities ⋮ The Lemaître-Schwarzschild problem revisited

Cites Work

• The problem of a self-gravitating scalar field
• Scalar field counterexamples to the cosmic censorship hypothesis
• On the occurrence of naked singularity in spherically symmetric gravitational collapse
• A simple derivation of the naked singularity in spherical dust collapse
• The final fate of spherical inhomogeneous dust collapse

This page was built for publication: Spherical gravitational collapse: Tangential pressure and related equations of state