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Hyperons in neutron stars

Name: Hyperons in neutron stars
Creator: Glendenning, N.K.
Keywords: General Physics, Moment Of Inertia, Equations, Pseudoscalar Mesons, Density, Hyperons, Hadrons, 7. Clean energy, 01 natural sciences, Equations Of State

descriptionPublicationkeyboard_double_arrow_right Article 01 Mar 1987 United States English Publisher:Springer Science and Business Media LLCJournal:Zeitschrift f�r Physik A Atomic Nuclei, volume 326, pages 57-64 (issn: 0930-1151, eissn: 1434-601X,

Authors: Glendenning, N.K.;

doi: 10.1007/bf01294571

Hyperons in neutron stars

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Abstract

Generalized beta equilibrium involving nucleons, hyperons and isobars is examined for neutron star matter. The hyperons produce a considerable softening of the equation of state. It is shown that the observed masses of neutron stars can be used to settle a recent controversy concerning the nuclear compressibility. Compressibilities less than 200 MeV are incompatible with observed masses.

Country

United States

Related Organizations

University of North Texas
United States
University of California System
United States
University of California, Berkeley
United States

Keywords

General Physics, Moment Of Inertia, Equations, Pseudoscalar Mesons, Density, Hyperons, Hadrons, Equations Of State, Baryon Resonances, Pions, Information, P Waves, Baryons, Mechanical Properties, Fermions, Pressure Dependence, Resonance Particles, Bosons, Theoretical Data, Nucleons, Data, Strange Particles 640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar, Mesons, Compressibility, Partial Waves, Pion Condensation, N Resonances, Neutron Stars, Decay, Beta Decay, Mass, Stars, Radio & X-Ray Sources, Physical Properties, Numerical Data, 71 Classical And Quantum Mechanics, Elementary Particles

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