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The maximum mass of ideal white dwarfs

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TLDR
The theory of polytropic gas spheres in conjunction with the equation of state of arelativislically degenerate electrongas leads to a unique value for the mass of a star built on this model.
Abstract
The theory of thepolytropic gas spheres in conjunction with the equation of state of arelativislically degenerate electrongas leads to aunique value for the mass of a star built on this model. This mass (=0.9I⊙) is interpreted as representing the upper limit to the mass of an ideal white dwarf.

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Beyond the Cosmological Standard Model

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Quantum-Spacetime Phenomenology

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Stationary Black Holes: Uniqueness and Beyond

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