Isospin Symmetry Breaking Effects on the Properties of Asymmetrical Nuclear Matter and -Stable Matter
arXiv:nucl-th/0307103 · doi:10.1023/B:IJTP.0000028872.40417.47
Abstract
We have studied the influences of isospin symmetry breaking of nucleon-nucleon interaction on the various properties of asymmetrical nuclear matter and -stable matter. For asymmetrical nuclear matter, it is found that by including this isospin symmetry breaking, the changes of bulk properties increase by increasing both density and asymmetry parameter. However, these effects on the total energy and equation of state of -stable matter are ignorable. For asymmetrical nuclear matter, the validity of the empirical parabolic law in the isospin symmetry breaking case is shown. It is observed that the isospin symmetry breaking of nucleon-nucleon interaction affects the -equilibrium conditions in -stable matter.
9 figures, International Journal of Theoretical Physics, 43 (2004) in press
References in corpus (1)
Cited by in corpus (10)
- Modified TOV in gravity's rainbow: properties of neutron stars and dynamical stability conditions
- Neutron stars structure in the context of massive gravity
- Dilatonic Equation of Hydrostatic Equilibrium and Neutron Star Structure
- Computation of Neutron Star Structure Using Modern Equation of State
- Neutron stars in Einstein- gravity: the cosmological constant effects
- Spin polarized liquid 3He
- Lowest Order Constrained Variational calculation for Polarized Liquid 3He at Finite Temperature
- LOCV calculations for polarized liquid with the spin-dependent correlation
- Effects of medium-induced meson mixing on the equation of state in isospin-asymmetric nuclear matter
- The impact of charge symmetry and charge independence breaking on the properties of neutrons and protons in isospin-asymmetric nuclear matter