Shear-free radiating collapse and conformal flatness

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dc.creatorHerrera, L.
dc.creatorDenmat, G. Le
dc.creatorSantos, N. O.
dc.creatorWang, A.
dc.date2004-01-07
dc.date2005-09-12
dc.date.accessioned2026-07-07T11:30:05Z
dc.date.available2026-07-07T11:30:05Z
dc.descriptionHere we study some general properties of spherical shear-free collapse. Its general solution when imposing conformal flatness is reobtained [1,2] and matched to the outgoing Vaidya spacetime. We propose a simple model satisfying these conditions and study its physical consequences. Special attention deserve, the role played by relaxational processes and the conspicuous link betweeen dissipation and density inhomogeneity.
dc.description13 pages Latex. Some misprints in eqs.(17), (30) and (35) have been corrected
dc.identifierhttps://arxiv.org/abs/gr-qc/0401022
dc.identifierhttp://arxiv.org/abs/gr-qc/0401022
dc.identifierInt.J.Mod.Phys.D13:583-592,2004
dc.identifierdoi:10.1142/S0218271804004840
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196911
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleShear-free radiating collapse and conformal flatness
dc.typetext

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