Space-time inhomogeneity, anisotropy and gravitational collapse
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Publication:695592
DOI10.1007/S10714-012-1406-8zbMath1255.83091arXiv1206.6011OpenAlexW3106164521MaRDI QIDQ695592
Publication date: 21 December 2012
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1206.6011
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Classical and relativistic thermodynamics (80A10) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (12)
Effects of tilted congruence on spherical compact stars ⋮ Shear-free radiating collapse model via Karmarkar condition in f(R) gravity ⋮ Dissipative collapse of a Karmarkar star ⋮ Dissipative cylindrical collapse of charged anisotropic fluid ⋮ Stability and horizon formation during dissipative collapse ⋮ THE ROLE OF THE ELECTROMAGNETIC FIELD IN DISSIPATIVE COLLAPSE ⋮ Structure scalars and evolution equations in \(f(G)\) cosmology ⋮ Study of gravitational collapse for anisotropic Karmarkar star in minimally coupled \(f(R)\) gravity ⋮ Conformally flat polytropes for anisotropic matter ⋮ Self-gravitating spherically symmetric fluid models in Brans-Dicke gravity ⋮ Riccati equations for bounded radiating systems ⋮ Effects of some physical factors on the inhomogeneity in planar symmetry
Cites Work
- Unnamed Item
- Radiating gravitational collapse with an initial inhomogeneous energy density distribution
- Dynamics of charged plane symmetric gravitational collapse
- Charged cylindrical collapse of anisotropic fluid
- Dynamics of non-adiabatic charged cylindrical gravitational collapse
- Radiating gravitational collapse with shear viscosity revisited
- Self-similar and charged radiating spheres: an anisotropic approach
- Cracking of homogeneous self-gravitating compact objects induced by fluctuations of local anisotropy
- The gravitational field of a radiating and contracting spherically-symmetric body with heat flow
- SINGULARITY IN GRAVITATIONAL COLLAPSE OF PLANE SYMMETRIC CHARGED VAIDYA SPACETIME
- NON-ADIABATIC GRAVITATIONAL COLLAPSE OF A SUPERDENSE STAR
- Exact model for a relativistic star
- Charged relativistic spheres with generalized potentials
- General solution for a relativistic star
- RELATIVISTIC GRAVITATIONAL COLLAPSE IN COMOVING COORDINATES: THE POST-QUASISTATIC APPROXIMATION
- Anisotropic geodesic fluid spheres in general relativity
- The final fate of spherical inhomogeneous dust collapse
- PHYSICAL CAUSES OF ENERGY DENSITY INHOMOGENIZATION AND STABILITY OF ENERGY DENSITY HOMOGENEITY IN RELATIVISTIC SELF-GRAVITATING FLUIDS
- Exact solutions for the Tikekar superdense star
- SPHERICAL COLLAPSE WITH HEAT FLOW AND WITHOUT HORIZON
- COLLAPSING INHOMOGENEOUS DUST IN THE BACKGROUND OF PERFECT (OR ANISOTROPIC) FLUID
- On Continued Gravitational Contraction
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