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On the Maximum Mass of General Relativistic Uniformly Rotating White Dwarfs

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arxiv 1210.7088 v1 pith:OX5SRWPT submitted 2012-10-26 astro-ph.SR gr-qc

Kuantay Boshkayev , Jorge Rueda , Remo Ruffini This is my paper · ORCID
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The properties of uniformly rotating white dwarfs are analyzed within the framework of general relativity. Hartle's formalism is applied to construct self-consistently the internal and external solutions to the Einstein equations. The mass, the radius, the moment of inertia and quadrupole moment of rotating white dwarfs have been calculated as a function of both the central density and rotation period of the star. The maximum mass of rotating white dwarfs for stable configurations has been obtained.

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  1. Modified electron dispersion relations in degenerate white dwarfs

    astro-ph.SR 2026-07 conditional novelty 5.0 of 10

    A negative logarithmic deformation of the electron dispersion relation stiffens white-dwarf matter and allows maximum masses from about 1.45 to 1.61 solar masses under standard TOV gravity.

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