Physics
Scientific paper
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.
Asensio Ramos Andrés
Polls Artur
Schulze Hans-Josef
Vidana Isaac
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