GRAVITATIONAL COLLAPSE MODEL WITH DISSIPATION

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dc.contributor.author	Abilmazhinova, Madina
dc.date.accessioned	2023-06-02T10:36:43Z
dc.date.available	2023-06-02T10:36:43Z
dc.date.issued	2023
dc.identifier.citation	Abilmazhinova, M. (2023). Gravitational collapse model with dissipation. School of Sciences and Humanities	en_US
dc.identifier.uri	http://nur.nu.edu.kz/handle/123456789/7177
dc.description.abstract	Radiating 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.language.iso	en	en_US
dc.publisher	School of Sciences and Humanities	en_US
dc.rights	Attribution-NonCommercial-ShareAlike 3.0 United States	*
dc.rights.uri	http://creativecommons.org/licenses/by-nc-sa/3.0/us/	*
dc.subject	Type of access: Restricted	en_US
dc.subject	Radiating spherically-symmetric collapsing model	en_US
dc.title	GRAVITATIONAL COLLAPSE MODEL WITH DISSIPATION	en_US
dc.type	Master's thesis	en_US
workflow.import.source	science