The effect of isoscalar-isovector coupling in infinite nuclear matter
arXiv:1211.5461 · doi:10.1088/0954-3899/40/8/085104
Abstract
Working on the framework of Relativistic Mean Field theory, we exposed the effect of nonlinear isoscalar-isovector coupling on G2 parameter set on the density dependence of nuclear symmetry energy in infinite nuclear matter. The observables like symmetric energy and few related coefficients are studied systematically. We presented the results of stiff symmetry energy at sub-saturation densities and a soft variation at normal densities. Correlation between the symmetric energy and the isoscalar-isovector coupling parameter fully demonstrated for wide range of density. The work further extended to the octet system and showed the effect of coupling over the equation of state.
6 pages, 5 figures
References in corpus (19)
- Shapiro delay measurement of a two solar mass neutron star
- Constraints on the symmetry energy and neutron skins from experiments and theory
- Neutron-Rich Nuclei in Heaven and Earth
- Skyrme Interaction and Nuclear Matter Constraints
- Nuclear symmetry energy probed by neutron skin thickness of nuclei
- Measurement of the Neutron Radius of 208Pb Through Parity-Violation in Electron Scattering
- Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment
- Constraints on the symmetry energy and on neutron skins from the pygmy resonances in 68Ni and 132Sn
- Hyperons and massive neutron stars: the role of hyperon potentials
- Connecting Neutron Star Observations to Three-Body Forces in Neutron Matter and to the Nuclear Symmetry Energy
- Extended-soft-core Baryon-Baryon Model II. Hyperon-Nucleon Interaction
- Nuclear symmetry energy and its density slope at normal density extracted from global nucleon optical potentials
- Giant Quadrupole Resonances in 208Pb, the nuclear symmetry energy and the neutron skin thickness
- The long journey from the giant-monopole resonance to the nuclear-matter incompressibility
- Exploring the extended density-dependent Skyrme effective forces for normal and isospin-rich nuclei to neutron stars
- Generic Constraints on the Relativistic Mean-Field and Skyrme-Hartree-Fock Models from the Pure Neutron Matter Equation of State
- Phase transition and properties of compact star
- Hadron production in non linear relativistic mean field models
- Effects of hyperons on the nuclear equation of state in a Dirac-Brueckner-Hartree-Fock model
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- The effect of self interacting isoscalar-vector meson on finite nuclei and infinite nuclear matter
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