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White dwarf cooling via gravity portals

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arxiv 2001.06004 v1 pith:XFWSP6UT submitted 2020-01-16 hep-ph astro-ph.SRgr-qc

classification hep-phastro-ph.SRgr-qc
keywords coolingequation-of-stategravitywhiteapproximationbosonscasecompared
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We investigate the impact of gravity portal to properties of white dwarfs, such as equation-of-state as well as cooling time. We find that the interaction between dark matter spin-zero bosons and electrons in the mean field approximation softens the equation-of-state, and the object coolers down slower compared to the usual case.

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  1. Temperature effects on white dwarfs in modified gravity

    gr-qc 2026-08 conditional novelty 4.0 of 10

    Finite temperature makes theoretical white dwarf models in scalar-tensor gravity larger at the same mass, creating a degeneracy with modified gravity signatures.

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