skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Isospin- and momentum-dependent effective interactions for the baryon octet and the properties of hybrid stars

Journal Article · · Physical Review. C, Nuclear Physics
 [1];  [2];  [3];  [4]
  1. Cyclotron Institute, Texas A and M University, College Station, Texas 77843-3366 (United States)
  2. Department of Physics, Shanghai Jiao Tong University, Shanghai 200240 (China)
  3. Cyclotron Institute and Department of Physics and Astronomy, Texas A and M University, College Station, Texas 77843-3366 (United States)
  4. Department of Physics and Astronomy, Texas A and M University-Commerce, Commerce, Texas 75429-3011 (United States)

The isospin- and momentum-dependent MDI interaction, which has been extensively used in intermediate-energy heavy-ion reactions to study the properties of asymmetric nuclear matter, is extended to include the nucleon-hyperon and hyperon-hyperon interactions by assuming the same density, momentum, and isospin dependence as for the nucleon-nucleon interaction. The parameters in these interactions are determined from the empirical hyperon single-particle potentials in symmetric nuclear matter at saturation density. The extended MDI interaction is then used to study in the mean-field approximation the equation of state of hypernuclear matter and also the properties of hybrid stars by including the phase transition from hypernuclear matter to quark matter at high densities. In particular, the effects of attractive and repulsive SIGMAN interactions and different values of symmetry energies on the hybrid star properties are investigated.

OSTI ID:
21389073
Journal Information:
Physical Review. C, Nuclear Physics, Vol. 81, Issue 5; Other Information: DOI: 10.1103/PhysRevC.81.055803; (c) 2010 The American Physical Society; ISSN 0556-2813
Country of Publication:
United States
Language:
English