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arXiv · 2012.13927

White dwarf stars in modified gravity

Aneta Wojnar
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Abstract

A few questions related to white dwarfs' physics is posed. It seems that the modified gravity framework can be a good starting point to provide alternative explanations to cooling processes, their age determination, and Chandrasekhar mass limits. Moreover, we have also obtained the Chandrasekhar limit coming from Palatini $f(\mathcal{R})$ gravity provided by a simple Lane-Emden model.

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Aneta Wojnar. 2021-02-28. White dwarf stars in modified gravity. https://doi.org/10.1142/s0219887821400065

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