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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.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.identifier.issn | 22181997 | |
| dc.identifier.uri | http://localhost:8080/xmlui/handle/123456789/2037 | |
| dc.identifier.uri | https://idr-sdlib.iitbhu.ac.in/handle/123456789/2037 | |
| 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 |
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