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The theory of the polytropic g~is spheres in conjunction with the equation of state of a relativ~stically degenerate electron-gas leads to a unique value for the mass of a star built on this model. This mass (=0.910) is interpreted as representing the upper limit to the mass of an ideal white dwarf
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S. Chandrasekhar (Wed,) studied this question.
synapsesocial.com/papers/6a04ca7d61fd4009c9ad3e48 — DOI: https://doi.org/10.1086/143324
S. Chandrasekhar
Stanley Medical College
The Astrophysical Journal
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