Probing isospin- and momentum-dependent nuclear effective interactions in neutron-rich matter

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作者
Lie-Wen Chen
Che Ming Ko
Bao-An Li
Chang Xu
Jun Xu
机构
[1] Shanghai Jiao Tong University,Department of Physics and Astronomy and Shanghai Key Laboratory for Particle Physics and Cosmology
[2] National Laboratory of Heavy Ion Accelerator,Center of Theoretical Nuclear Physics
[3] Texas A & M University,Cyclotron Institute and Department of Physics and Astronomy
[4] Texas A & M University-Commerce,Department of Physics and Astronomy
[5] Xi’an Jiao Tong University,Department of Applied Physics
[6] Nanjing University,Department of Physics
[7] Chinese Academy of Sciences,Shanghai Institute of Applied Physics
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Neutron Star; Nuclear Matter; Symmetry Energy; Momentum Dependence; Symmetry Potential;
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摘要
The single-particle potential for nucleons and hyperons in neutron-rich matter generally depends on the density and isospin asymmetry of the medium as well as the momentum and isospin of the particle. It further depends on the temperature of the matter if the latter is in thermal equilibrium. We review here the extension of a Gogny-type isospin- and momentum-dependent interactions in several aspects made in recent years and their applications in studying intermediate-energy heavy-ion collisions, thermal properties of asymmetric nuclear matter and properties of neutron stars. The importance of the isospin and momentum dependence of the single-particle potential, especially the momentum dependence of the isovector potential, is clearly revealed throughout these studies.
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