Non-adiabatic collapse of a quasi-spherical radiating star

Simple item page
dc.creatorDebnath, Ujjal
dc.creatorNath, Soma
dc.creatorChakraborty, Subenoy
dc.date2003-10-16
dc.date.accessioned2026-07-07T11:30:03Z
dc.date.available2026-07-07T11:30:03Z
dc.descriptionA model is proposed of a collapsing quasi-spherical radiating star with matter content as shear-free isotropic fluid undergoing radial heat-flow with outgoing radiation. To describe the radiation of the system, we have considered both plane symmetric and spherical Vaidya solutions. Physical conditions and thermodynamical relations are studied using local conservation of momentum and surface red-shift. We have found that for existence of radiation on the boundary, pressure on the boundary is not necessary.
dc.description8 Latex pages, No figures, Revtex style
dc.identifierhttps://arxiv.org/abs/gr-qc/0310080
dc.identifierhttp://arxiv.org/abs/gr-qc/0310080
dc.identifierGen.Rel.Grav.37:215-223,2005
dc.identifierdoi:10.1007/s10714-005-0010-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196904
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNon-adiabatic collapse of a quasi-spherical radiating star
dc.typetext

Files

Collections

arXiv