A DYNAMICAL SYMMETRY OF THE QUASI-SPHERICAL (OR SPHERICAL) COLLAPSE

DOI10.1142/S021827180500736XzbMath1098.83023arXivgr-qc/0410031OpenAlexW3099679016MaRDI QIDQ5714684

Naresh Dadhich, Subenoy Chakraborty, Ujjal Debnath

Publication date: 15 December 2005

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

Full work available at URL: https://arxiv.org/abs/gr-qc/0410031

zbMATH Keywords

linear transformationgravitational collapsedynamical symmetrySzekeres metric

Mathematics Subject Classification ID

Space-time singularities, cosmic censorship, etc. (83C75)

Related Items (4)

DYNAMICAL SYMMETRY WITH GENERAL INITIAL AREA RADIUS IN QUASI-SPHERICAL GRAVITATIONAL COLLAPSE, AND ANISOTROPY AND INHOMOGENEITY OF SPACE–TIME ⋮ Collapse dynamics of a star of dark matter and dark energy ⋮ DYNAMICAL SYMMETRY IN GRAVITATIONAL COLLAPSE WITH GENERAL INITIAL AREA RADIUS ⋮ LARGE DYNAMICAL SYMMETRY OF QUASI-SPHERICAL GRAVITATIONAL COLLAPSE WITH RADIAL AND TANGENTIAL PRESSURES AND ANISOTROPY AND INHOMOGENEITY OF SPACE–TIME

Cites Work

• Quasi-spherical gravitational collapse in any dimension
• Initial data and the final fate of inhomogeneous dust collapse
• A STUDY OF HIGHER DIMENSIONAL INHOMOGENEOUS COSMOLOGICAL MODEL
• The Large Scale Structure of Space-Time

This page was built for publication: A DYNAMICAL SYMMETRY OF THE QUASI-SPHERICAL (OR SPHERICAL) COLLAPSE