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Hyperonic equation of state

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Abstract

An equation of state for cold matter at neutron star densities, ϱ>1014 gm/cm3, is evaluated. The gas is considered to be a degenerate mixture of neutrons, protons, leptons, hyperons and massive baryons. We derive the equilibrium equations including the effects of nuclear interactions among all the hadrons.

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Langer, W.D., Rosen, L.C. Hyperonic equation of state. Astrophys Space Sci 6, 217–227 (1970). https://doi.org/10.1007/BF00651223

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  • DOI: https://doi.org/10.1007/BF00651223

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