Analytical relations between nuclear symmetry energy and single-nucleon potentials in isospin asymmetric nuclear matter
arXiv:1004.4403 · doi:10.1016/j.nuclphysa.2011.06.027
Abstract
Using the Hugenholtz-Van Hove theorem, we derive general expressions for the quadratic and quartic symmetry energies in terms of single-nucleon potentials in isospin asymmetric nuclear matter. These analytical relations are useful for gaining deeper insights into the microscopic origins of the uncertainties in our knowledge on nuclear symmetry energies especially at supra-saturation densities. As examples, the formalism is applied to two model single-nucleon potentials that are widely used in transport model simulations of heavy-ion reactions.
23 pages with 6 figures
References in corpus (12)
- Nuclear symmetry energy probed by neutron skin thickness of nuclei
- Higher-order effects on the incompressibility of isospin asymmetric nuclear matter
- Nuclear symmetry energy and its density slope at normal density extracted from global nucleon optical potentials
- Symmetry energy of dilute warm nuclear matter
- Locating the inner edge of neutron star crust using terrestrial nuclear laboratory data
- Probing the Nuclear Symmetry Energy with Heavy Ion Collisions
- Isospin emission and flows at high baryon density: a test of the symmetry potential
- The High-Density Symmetry Energy and Direct Urca
- Why is the nuclear symmetry energy so uncertain at supra-saturation densities?
- An improved single particle potential for transport model simulations of nuclear reactions induced by rare isotope beams
- Nuclear symmetry potential in the relativistic impulse approximation
- Effective 3-Body Interaction for Mean-Field and Density-Functional Theory
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- Higher-order symmetry energy and neutron star core-crust transition with Gogny forces
- Single-nucleon potential decomposition of the nuclear symmetry energy
- Isospin splitting of nucleon effective mass from giant resonances in Pb
- Probing isospin- and momentum-dependent nuclear effective interactions in neutron-rich matter
- Probing nuclear symmetry energy at high densities using pion, kaon, eta and photon productions in heavy-ion collisions
- Extracting the nuclear symmetry potential and energy from neutron-nucleus scattering data
- Revisit of the neutron/proton ratio puzzle in intermediate-energy heavy-ion collisions
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- Neutron-proton effective mass splitting in neutron-rich matter and its impacts on nuclear reactions
- Neutron-proton effective mass splitting in neutron-rich matter
- Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars
- Probing Nuclear Symmetry Energy and its Imprints on Properties of Nuclei, Nuclear Reactions, Neutron Stars and Gravitational Waves
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- Isospin dependent global neutron-nucleus optical model potential
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- Anomalous quartic term in the expansion of the symmetry energy
- Equation of State of Neutron-Rich Matter in -Dimensions
- Neutron matter within QCD sum rules
- Correlated structure of nuclear symmetry energy from covariant nucleon self-energy
- Origins and Impacts of High-Density Symmetry Energy
- Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
- Basic quantities of the Equation of State in isospin asymmetric nuclear matter