Dissipative collapse in the presence of Λ

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dc.contributor.author Govender, M
dc.contributor.author Thirukkanesh, S.
dc.date.accessioned 2019-08-08T07:31:19Z
dc.date.available 2019-08-08T07:31:19Z
dc.date.issued 2009
dc.identifier.uri http://www.digital.lib.esn.ac.lk/handle/123456789/3947
dc.description.abstract We present the general junction conditions for the smooth matching of a spherically symmetric, shear-free spacetime to Vaidya’s outgoing metric across a four-dimensional time-like hypersurface in the presence of a cosmological constant. These results generalise earlier treatments by Santos and co-workers on radiating stellar models. We study the thermal evolution of a particular radiating model within the framework of extended irreversible thermodynamics. DOI: https://link.springer.com/article/10.1007/s10773-009-0163-2 en_US
dc.language.iso en en_US
dc.publisher International Journal of Theoretical Physics en_US
dc.subject Gravitational collapse en_US
dc.subject Cosmological constant en_US
dc.subject Irreversible thermodynamics en_US
dc.title Dissipative collapse in the presence of Λ en_US
dc.type Article en_US
dc.identifier.sslno 21 en_US
dc.identifier.doi https://link.springer.com/article/10.1007/s10773-009-0163-2 en_US


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