Radiant gravitational collapse with anisotropy in pressures and bulk viscosity
DOI10.1007/S10714-023-03098-4zbMath1528.83052arXiv2210.14288OpenAlexW4366000325MaRDI QIDQ6174867
M. F. A. da Silva, A. C. Mesquita
Publication date: 15 July 2023
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2210.14288
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Galactic and stellar structure (85A15) Viscosity solutions to PDEs (35D40) Dark matter and dark energy (83C56)
Cites Work
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Dynamical instability and the expansion-free condition
- New solutions of Einstein equations in spherical symmetry: The cosmic censor to the court
- Anisotropic stars. II: Stability
- Radiating stars with exponential Lie symmetries
- The stability of relativistic stars and the role of the adiabatic index
- Embedding condition describing shearing, dissipative collapse
- Relativistic Hydrodynamics
- GRAVITATIONAL COLLAPSE WITH TANGENTIAL PRESSURE
- ON ANISOTROPIC DARK ENERGY
- DRESSING A NAKED SINGULARITY: AN EXAMPLE
- Energy conditions for an imperfect fluid
- Some models of anisotropic spheres in general relativity
- The Maximum Mass of Ideal White Dwarfs
- GRAVITATIONAL COLLAPSE OF SPHERICALLY SYMMETRIC PERFECT FLUID WITH KINEMATIC SELF-SIMILARITY
- Non-local equation of state in general relativistic radiating spheres
- Physical Processes in Naked Singularity Formation
- RADIATING GRAVITATIONAL COLLAPSE WITH SHEAR VISCOSITY AND BULK VISCOSITY
- RECENT DEVELOPMENTS IN GRAVITATIONAL COLLAPSE AND SPACETIME SINGULARITIES
- Spherical Symmetry and Mass-Energy in General Relativity. I. General Theory
- The Large Scale Structure of Space-Time
- GRAVITATIONAL COLLAPSE OF SELF-SIMILAR AND SHEAR-FREE FLUID WITH HEAT FLOW
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- On Massive Neutron Cores
- On Continued Gravitational Contraction
- Radially Symmetric Distributions of Matter
- ‘Newtonian’ Time in General Relativity
- Lie symmetries, Painlevé analysis, and global dynamics for the temporal equation of radiating stars
This page was built for publication: Radiant gravitational collapse with anisotropy in pressures and bulk viscosity