DYNAMICAL SYMMETRY WITH GENERAL INITIAL AREA RADIUS IN QUASI-SPHERICAL GRAVITATIONAL COLLAPSE, AND ANISOTROPY AND INHOMOGENEITY OF SPACE–TIME

DOI10.1142/S0218271808011857zbMath1151.83304OpenAlexW2059215850MaRDI QIDQ3527365

Subenoy Chakraborty, Anusua Bajeva, Tanwi Bandyopadhyay

Publication date: 29 September 2008

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0218271808011857

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Space-time singularities, cosmic censorship, etc. (83C75)

Cites Work

• Quasi-spherical gravitational collapse in any dimension
• LARGE DYNAMICAL SYMMETRY OF QUASI-SPHERICAL GRAVITATIONAL COLLAPSE WITH RADIAL AND TANGENTIAL PRESSURES AND ANISOTROPY AND INHOMOGENEITY OF SPACE–TIME
• A STUDY OF HIGHER DIMENSIONAL INHOMOGENEOUS COSMOLOGICAL MODEL
• DYNAMICAL SYMMETRY IN GRAVITATIONAL COLLAPSE WITH GENERAL INITIAL AREA RADIUS
• NAKED SINGULARITIES IN HIGHER DIMENSIONAL GRAVITATIONAL COLLAPSE
• ROLE OF PRESSURE IN QUASI-SPHERICAL GRAVITATIONAL COLLAPSE
• A DYNAMICAL SYMMETRY OF THE QUASI-SPHERICAL (OR SPHERICAL) COLLAPSE
• QUASI-SPHERICAL GRAVITATIONAL COLLAPSE AND THE ROLE OF INITIAL DATA, ANISOTROPY AND INHOMOGENEITY

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