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White Dwarf mass-radius relation

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arxiv 2012.01242 v2 pith:3PO6WQXS submitted 2020-12-02 astro-ph.HE

Federico Ambrosino This is my paper · ORCID
classification astro-ph.HE
keywords mass-radiusproblemwhiteaimsbetacaseconsidereddecay
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abstract

This paper aims to provide an introduction to the problem of determining the mass-radius relationship for white dwarfs. Both Newtonian and general relativistic case are examined, electromagnetic interactions are considered and the problem of $\beta$-decay equilibrium is discussed in particular for Helium WD

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Cited by 1 Pith paper

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  1. Detecting White Dwarf Binary Mergers with Gravitational Waves

    gr-qc 2025-10 conditional novelty 6.0 of 10

    MAGIS Space and AEDGE could detect white-dwarf-binary mergers in the 10 mHz–1 Hz band, giving early warning of Type Ia supernova explosions at rates of roughly one every four years and a few hundred per year, respectively.

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