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Probing nuclear symmetry energy at high densities using pion, kaon, eta and photon productions in heavy-ion collisions
Zhi-Gang Xiao, Gao-Chan Yong, Lie-Wen Chen +4
The high-density behavior of nuclear symmetry energy is among the most uncertain properties of dense neutron-rich matter. Its accurate determination has significant ramifications i…
Breaking the EOS-Gravity Degeneracy with Masses and Pulsating Frequencies of Neutron Stars
Weikang Lin, Bao-An Li, Lie-Wen Chen +2
A thorough understanding of many astrophysical phenomena associated with compact objects requires reliable knowledge about both the equation of state (EOS)of super-dense nuclear ma…
Probing isospin- and momentum-dependent nuclear effective interactions in neutron-rich matter
Lie-Wen Chen, Che Ming Ko, Bao-An Li +2
The single-particle potentials 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 iso…
Probing the high-density behavior of symmetry energy with gravitational waves
F. J. Fattoyev, W. G. Newton, Bao-An Li
Gravitational wave (GW) astronomy opens up an entirely new window on the Universe to probe the equations of state (EOS) of neutron-rich matter. With the advent of next generation G…
Influence of neutron-skin thickness on ratio in Pb+Pb collisions
Gao-Feng Wei, Bao-An Li, Jun Xu +1
Within an isospin- and momentum-dependent transport model IBUU11 using as an input nucleon density profiles from Hartree-Fock calculations based on a modified Skyrme-like (MSL) mod…
Relationship between the symmetry energy and the single-nucleon potential in isospin-asymmetric nucleonic matter
Chang Xu, Bao-An Li, Lie-Wen Chen
In this contribution, we review the most important physics presented originally in our recent publications. Some new analyses, insights and perspectives are also provided. We showe…