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

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.

arXiv comment14 pages including 3 figures; invited article to the collection "Modified Theories of Gravity and Cosmological Applications" in Universe; accepted for publication

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Cited by in corpus (4)

• Metric-affine effects in crystallization processes of white dwarfs
• White dwarfs in regularized 4D Einstein-Gauss-Bonnet gravity
• Effects of modified gravity on microscopic properties and cooling timescale of white dwarfs
• White dwarf cooling in $f(R,T)$ gravity