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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8290
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dc.contributor.authorKalita, Surajit-
dc.contributor.authorSarmah, Lupamudra-
dc.contributor.authorWojnar, Aneta-
dc.date.accessioned2023-10-26T05:23:21Z-
dc.date.available2023-10-26T05:23:21Z-
dc.date.issued2022-12-
dc.identifier.citationUniverse, Vol. 8, No. 12, 647en_US
dc.identifier.issn2218-1997-
dc.identifier.urihttp://hdl.handle.net/2248/8290-
dc.descriptionOpen Accessen_US
dc.descriptionThis article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/).-
dc.description.abstractA simple cooling model of white dwarf stars is re-analyzed in Palatini 𝑓(𝑅) gravity. Modified gravity affects the white dwarf structures and consequently their ages. We find that the resulting super-Chandrasekhar white dwarfs need more time to cool down than sub-Chandrasekhar ones, or when compared to the Newtonian models.en_US
dc.language.isoenen_US
dc.publisherMultidisciplinary Digital Publishing Instituteen_US
dc.relation.urihttps://doi.org/10.3390/universe8120647-
dc.rights© 2022 by the authors.-
dc.subjectCooling processen_US
dc.subjectWhite dwarfen_US
dc.subjectModified gravityen_US
dc.subjectChandrasekhar limiten_US
dc.titleCooling Process of White Dwarf Stars in Palatini f(R) Gravityen_US
dc.typeArticleen_US
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