Quark matter core in neutron star

Details Quark matter core in neutron star Quark matter core in neutron star

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jpha...13.3105a&link_type=abstract

Journal of Physics A - Mathematical and General, vol. 13, Sept. 1980, p. 3105-3112.

Physics

2

Equations Of State, Neutron Stars, Quantum Chromodynamics, Quarks, Stellar Models, Baryons, Cores, Phase Transformations, Stellar Structure, Supermassive Stars, Systems Stability

Scientific paper

The possible phase transition to quark matter in a neutron star is considered using the neutron matter equation of state proposed recently by Canuto, Datta, and Kalman which involves spin-2 meson interaction among nucleons. The corresponding equation of state for quark matter is taken from quantum chromodynamics. The Oppenheimer-Volkoff equation is then numerically solved to investigate the stability of a superdense system with quarkion cores.

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