GRAVITATIONAL COLLAPSE MODEL WITH DISSIPATION

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dc.contributor.authorAbilmazhinova, Madina
dc.date.accessioned2023-06-02T10:36:43Z
dc.date.available2023-06-02T10:36:43Z
dc.date.issued2023
dc.description.abstractRadiating spherically-symmetric collapsing model is studied. Exterior Vaidya spacetime is matched with the interior of a perfect fluid with a heat flow. Junction conditions and field equations are derived, revealing that a nonzero pressure at the boundary is necessary to satisfy the boundary conditions. Solution for model with assumption that the fluid trajectories are geodesics is found. When heat flux is set to zero, it is demonstrated that the model becomes that of an Oppenheimer and Snyder.en_US
dc.identifier.citationAbilmazhinova, M. (2023). Gravitational collapse model with dissipation. School of Sciences and Humanitiesen_US
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/7177
dc.language.isoenen_US
dc.publisherSchool of Sciences and Humanitiesen_US
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectType of access: Restricteden_US
dc.subjectRadiating spherically-symmetric collapsing modelen_US
dc.titleGRAVITATIONAL COLLAPSE MODEL WITH DISSIPATIONen_US
dc.typeMaster's thesisen_US
workflow.import.sourcescience

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