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

dc.contributor.author	Kalita, Surajit
dc.contributor.author	Sarmah, Lupamudra
dc.contributor.author	Wojnar, Aneta
dc.date.accessioned	2023-10-26T05:23:21Z
dc.date.available	2023-10-26T05:23:21Z
dc.date.issued	2022-12
dc.identifier.citation	Universe, Vol. 8, No. 12, 647	en_US
dc.identifier.issn	2218-1997
dc.identifier.uri	http://hdl.handle.net/2248/8290
dc.description	Open Access	en_US
dc.description	This 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.abstract	A 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.iso	en	en_US
dc.publisher	Multidisciplinary Digital Publishing Institute	en_US
dc.relation.uri	https://doi.org/10.3390/universe8120647
dc.rights	© 2022 by the authors.
dc.subject	Cooling process	en_US
dc.subject	White dwarf	en_US
dc.subject	Modified gravity	en_US
dc.subject	Chandrasekhar limit	en_US
dc.title	Cooling Process of White Dwarf Stars in Palatini f(R) Gravity	en_US
dc.type	Article	en_US