Maximum mass of neutron stars

Details Maximum mass of neutron stars Maximum mass of neutron stars

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006phrvc..73e8801s&link_type=abstract

Physical Review C, vol. 73, Issue 5, id. 058801

Physics

51

Nuclear Matter Aspects Of Neutron Stars, Hyperon-Nucleon Interactions, Many-Body Theory, Neutron Stars

Scientific paper

We determine the structure of neutron stars within a Brueckner-Hartree-Fock approach based on realistic nucleon-nucleon, nucleon-hyperon, and hyperon-hyperon interactions. Our results indicate rather low maximum masses below 1.4 solar masses. This feature is insensitive to the nucleonic part of the EOS due to a strong compensation mechanism caused by the appearance of hyperons and represents thus strong evidence for the presence of nonbaryonic “quark” matter in the interior of heavy stars.

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