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- W4297675223 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." @default.
- W4297675223 created "2022-09-30" @default.
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- W4297675223 date "2022-09-05" @default.
- W4297675223 modified "2023-09-27" @default.
- W4297675223 title "Cooling process of white dwarf stars in Palatini $f(R)$ gravity" @default.
- W4297675223 doi "https://doi.org/10.48550/arxiv.2209.02095" @default.
- W4297675223 hasPublicationYear "2022" @default.
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