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Chandrasekhar's perturbation method-oriented theories up to third order for uniformly and differentially-rotating polytropic stars: Error-removing techniques

V. S. Geroyannis, F. N. Valvi

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Key concepts: Polytropic process, Chandrasekhar limit, Physics, Polytrope, Perturbation (astronomy), Stars, Perturbation theory (quantum mechanics), Cosmology

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Chandrasekhar's perturbation method-oriented theories up to third order for uniformly and differentially-rotating polytropic stars: Error-removing techniques — Research Paper | ScholarLens