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Hyperonic equation of state
Authors:William D Langer  Leonard C Rosen
Institution:(1) Goddard Institute for Space Studies, NASA, New York, N.Y., USA;(2) Belfer Graduate School of Science, Yeshiva University, New York, N.Y., USA;(3) Lawrence Radiation Laboratory, Livermore, Calif., USA;(4) Present address: Dept. of Physics and Astronomy, Darthmouth College, Hanover, N.H., USA
Abstract:An equation of state for cold matter at neutron star densities, rhov>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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