Temperature and momentum dependence of single-particle properties in hot asymmetric nuclear matter
arXiv:0801.2717 · doi:10.1103/PhysRevC.78.054323
Abstract
We have studied the effects of momentum dependent interactions on the single-particle properties of hot asymmetric nuclear matter. In particular, the single-particle potential of protons and neutrons as well as the symmetry potential have been studied within a self-consistent model using a momentum dependent effective interaction. In addition, the isospin splitting of the effective mass has been derived from the above model. In each case temperature effects have been included and analyzed. The role of the specific parametrization of the effective interaction used in the present work has been investigated. It has been concluded that the behavior of the symmetry potential depends strongly on the parametrization of the interaction part of the energy density and the momentum dependence of the regulator function. The effects of the parametrization have been found to be less pronounced on the isospin mass splitting.
arXiv comment22 pages, 14 figures
References in corpus (43)
- Determination of the Equation of State of Dense Matter
- Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
- Composition and Structure of Protoneutron Stars
- Reaction Dynamics with Exotic Beams
- Isospin Physics in Heavy-Ion Collisions at Intermediate Energies
- Determination of the stiffness of the nuclear symmetry energy from isospin diffusion
- Phase Transitions in Warm, Asymmetric Nuclear Matter
- Asymmetric Nuclear Matter from Extended Brueckner-Hartree-Fock Approach
- Nucleon-nucleon cross sections in neutron-rich matter and isospin transport in heavy-ion reactions at intermediate energies
- Probing the High Density Behaviour of Nuclear Symmetry Energy with High Energy Heavy-Ion Collisions
- Momentum dependence of symmetry potential in asymmetric nuclear matter for transport model calculations
- Equation of state of asymmetric nuclear matter and collisions of neutron-rich nuclei
- Density dependence of the symmetry energy and the nuclear equation of state: A Dynamical and Statistical model perspective
- Determination of the Mean-Field Momentum-Dependence using Elliptic Flow
- Effective Nucleon Masses in Symmetric and Asymmetric Nuclear Matter
- Effects of momentum-dependent symmetry potential on heavy-ion collisions induced by neutron-rich nuclei
- Isovector splitting of nucleon effective masses, ab-initio benchmarks and extended stability criteria for Skyrme energy functionals
- The Relativistic Dirac-Brueckner Approach to Asymmetric Nuclear Matter
- Isospin-dependent properties of asymmetric nuclear matter in relativistic mean-field models
- Momentum dependence of the symmetry potential and nuclear reactions induced by neutron-rich nuclei at RIA
- Modelization of the EOS
- Isospin splitting of the nucleon mean field
- Momentum, Density, and Isospin dependence of the Symmetric and Asymmetric Nuclear Matter Properties
- Density Dependence of the Symmetry energy and the Equation of State of Isospin Asymmetric Nuclear Matter
- Constraining the neutron-proton effective mass splitting in neutron-rich matter
- Transport properties of isospin effective mass splitting
- Low-momentum interactions with smooth cutoffs
- Fast nucleon emission as a probe of the isospin momentum dependence
- Temperature effects on the nuclear symmetry energy and symmetry free energy with an isospin and momentum dependent interaction
- The Liquid-Gas Phase Transitions in a Multicomponent Nuclear System with Coulomb and Surface Effects
- Symmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures
- Hot Nuclear Matter Equation of State with a Three-body Force
- Kaon Condensates, Nuclear Symmetry Energy and Cooling of Neutron Stars
- Predicting the single-proton/neutron potentials in asymmetric nuclear matter
- Effects of isospin and momentum dependent interactions on thermal properties of asymmetric nuclear matter
- Effects of isospin and momentum dependent interactions on liquid-gas phase transition in hot asymmetric nuclear matter
- Thermal effects on nuclear symmetry energy with a momentum-dependent effective interaction
- Evolution of the symmetry energy of hot neutron-rich matter formed in heavy-ion reactions
- High-energy behavior of the nuclear symmetry potential in asymmetric nuclear matter
- Nuclear symmetry potential in the relativistic impulse approximation
- Temperature dependence of single-particle properties in nuclear matter
- Warm Asymmetric Nuclear Matter and Proto-Neutron Star
- Nuclear Chemical and Mechanical Instability and the Liquid-Gas Phase Transition in Nuclei
Cited by in corpus (9)
- The Microscopic Approach to Nuclear Matter and Neutron Star Matter
- Effects of the equation of state on the bulk properties of maximally-rotating neutron stars
- Thermodynamical Description of Hot, Rapidly Rotating Neutron Stars, Protoneutron Stars, and Neutron Star Merger Remnants
- Neutron-proton effective mass splitting and thermal evolution in neutron rich matter
- Equation of state for -stable hot nuclear matter
- Neutron Stars and Gravitational Waves: the Key Role of Nuclear Equation of State
- Temperature-dependence of single-particle properties in isospin-symmetric and -asymmetric matter within the Dirac-Brueckner-Hartree-Fock model
- Equation of state for dense supernova matter
- Temperature effects on the neutron matter equation of state obtained from chiral effective field theory