DISSIPATIVE COLLAPSE OF THE SPHERICAL STELLAR OBJECT

dc.contributor.authorAryngazin, Ansar
dc.date.accessioned2023-06-05T07:58:04Z
dc.date.available2023-06-05T07:58:04Z
dc.date.issued2023
dc.description.abstractIn this research we investigate the shear-free, non-viscous perfect fluid model describing stellar object that emits radiation that leads to dissipation. We study matching of the interior metric with the exterior outgoing Vaidya metric via junction conditions. We also impose regularity and energy conditions in order for the model to be physically realistic. We find solution to main Einstein field equations, analyze and emphasize the features of the solution, specifically the impact of dissipation of the density 𝜌, pressure 𝑝 and mass 𝑚 functions, and present the resulted analysis in plots. We compare obtained solution to the conventional OSD collapse model and to solutions found in previous works, and investigate the prospects of the implementation of obtained results on future research in modified GR.en_US
dc.identifier.citationAryngazin, A. (2023). Dissipative collapse of the spherical stellar object. School of Sciences and Humanitiesen_US
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/7181
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.subjectspherical stellar objecten_US
dc.subjectDissipative collapseen_US
dc.titleDISSIPATIVE COLLAPSE OF THE SPHERICAL STELLAR OBJECTen_US
dc.typeMaster's thesisen_US
workflow.import.sourcescience

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