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	2023-04-17T09:29:23Z
dc.date.available	2023-04-17T09:29:23Z
dc.date.issued	2022-12
dc.identifier.issn	22181997
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/2037
dc.description	This paper is submitted by the author of IIT (BHU), Varanasi	en_US
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.	en_US
dc.language.iso	en	en_US
dc.publisher	MDPI	en_US
dc.relation.ispartofseries	Universe; Article number 647
dc.subject	Chandrasekhar limit; cooling process; modified gravity; white dwarf	en_US
dc.title	Cooling Process of White Dwarf Stars in Palatini f(R) Gravity	en_US
dc.type	Article	en_US