QUASI-SPHERICAL STAR OF DARK MATTER AND DARK ENERGY AND A STUDY OF ITS COLLAPSE DYNAMICS
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Publication:3502586
DOI10.1142/S0217732307023468zbMath1140.85300OpenAlexW2126708074MaRDI QIDQ3502586
Subenoy Chakraborty, Tanwi Bandyopadhyay
Publication date: 26 May 2008
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0217732307023468
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Galactic and stellar structure (85A15) Galactic and stellar dynamics (85A05)
Cites Work
- A class of inhomogeneous cosmological models
- Quasi-spherical gravitational collapse in any dimension
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- Precursory singularities in spherical gravitational collapse
- Gravitational collapse with non-vanishing tangential stresses: II. A laboratory for cosmic censorship experiments
- Initial data and the end state of spherically symmetric gravitational collapse
- Nakedness and curvature strength of a shell-focusing singularity in spherically symmetric spacetime with vanishing radial pressure
- What role do pressures play in determining the final end state of gravitational collapse?
- Physical Processes in Naked Singularity Formation
- A STUDY OF HIGHER DIMENSIONAL INHOMOGENEOUS COSMOLOGICAL MODEL
- ROLE OF PRESSURE IN QUASI-SPHERICAL GRAVITATIONAL COLLAPSE
- On Continued Gravitational Contraction
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