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Comparison of heavy-ion transport simulations: Collision integral in a box
Ying-Xun Zhang, Yong-Jia Wang, Maria Colonna +27
Simulations by transport codes are indispensable to extract valuable physics information from heavy ion collisions. In order to understand the origins of discrepancies between diff…
Deep crustal heating by neutrinos from the surface of accreting neutron stars
F. J. Fattoyev, Edward F. Brown, Andrew Cumming +4
We present a new mechanism for deep crustal heating in accreting neutron stars. Charged pions () are produced in nuclear collisions on the neutron star surface during active a…
Effects of retarded electrical fields on observables sensitive to the high-density behavior of nuclear symmetry energy in heavy-ion collisions at intermediate energies
Gao-Feng Wei, Bao-An Li, Gao-Chan Yong +3
Within the isospin- and momentum-dependent transport model IBUU11, we examine the relativistic retardation effects of electrical fields on the ratio and neutron-proto…
The interplay of short-range correlations and nuclear symmetry energy in hard photon productions from heavy-ion reactions at Fermi energies
Gao-Chan Yong, Bao-An Li
Within an isospin- and momentum-dependent transport model for nuclear reactions at intermediate energies, we investigate the interplay of the nucleon-nucleon short-range correlatio…
Simulating spin dynamics with spin-dependent cross sections in heavy-ion collisions
Yin Xia, Jun Xu, Bao-An Li +1
We have incorporated the spin-dependent nucleon-nucleon cross sections into a Boltzmann-Uehling-Uhlenbeck transport model for the first time, using the spin-singlet and spin-triple…
How tightly is nuclear symmetry energy constrained by unitary Fermi gas?
Nai-Bo Zhang, Bao-Jun Cai, Bao-An Li +2
We examine critically how tightly the density dependence of nuclear symmetry energy \esym is constrained by the universal equation of state (EOS) of the unitary Fermi gas $E_{\rm{U…