Cooling Process of White Dwarf Stars in Palatini f(R) Gravity

dc.contributor.author	Kalita S.; Sarmah L.; Wojnar A.
dc.date.accessioned	2025-05-23T11:23:54Z
dc.description.abstract	A simple cooling model of white dwarf stars is re-analyzed in Palatini (Formula presented.) 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. © 2022 by the authors.
dc.identifier.doi	https://doi.org/10.3390/universe8120647
dc.identifier.uri	http://172.23.0.11:4000/handle/123456789/9532
dc.relation.ispartofseries	Universe
dc.title	Cooling Process of White Dwarf Stars in Palatini f(R) Gravity

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