Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8183782 | Nuclear Physics A | 2013 | 6 Pages |
Abstract
Hyperon single-particle potentials are calculated in pure neutron matter in the framework of the lowest-order Brueckner theory, using two recent baryon-baryon interactions, the SU6 quark-model potential and the potential derived from the chiral effective field theory. These properties are important for understanding neutron star matter on the basis of underlying baryon-baryon interactions. Because the calculated potential of Σâ is strongly repulsive and that of Îâ is also repulsive, these hyperons are unlikely to appear in neutron star matter. The Î potential is attractive enough to appear in high neutron matter as has been commonly expected in microscopic calculations. After showing important contributions of three-nucleon forces in neutron matter, analogous repulsive contributions to the Î potential from the Σâ excitation are estimated by evaluating second-order diagrams.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
M. Kohno,