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6 papers · 2 filters
The Neutron Star Crust: Nuclear Physics Input
Andrew W. Steiner
A fully self-consistent model of the neutron star inner crust based upon models of the nucleonic equation of state at zero temperature is constructed. The results nearly match thos…
Rotation-driven prolate-to-oblate shape phase transition in 190W: A projected shell model study
Yang Sun, Philip M. Walker, Fu-Rong Xu +1
A shape phase transition is demonstrated to occur in 190W by applying the Projected Shell Model, which goes beyond the usual mean-field approximation. Rotation alignment of neutron…
Effects of nuclear molecular configurations on the astrophysical S-factor for O + O
A. Diaz-Torres, L. R. Gasques, M. Wiescher
The impact of nuclear molecular configurations on the astrophysical S-factor for O + O is investigated within the realistic two-center shell model based on Woods-Saxo…
The influence of cluster emission and the symmetry energy on neutron-proton spectral double ratios
Y. X. Zhang, P. Danielewicz, M. Famiano +3
Emissions of free neutrons and protons from the central collisions of 124Sn+124Sn and 112Sn+112Sn reactions are simulated using the Improved Quantum Molecular Dynamics model with t…
Constraining properties of neutron stars with heavy-ion reactions in terrestrial laboratories
Bao-An Li, Lie-Wen Chen, Che Ming Ko +3
Heavy-ion reactions provide a unique means to investigate the equation of state (EOS) of neutron-rich nuclear matter, especially the density dependence of the nuclear symmetry ener…
Enhancement of and low excitation of the second 0 state near N=40 in Ge isotopes
M. Hasegawa, T. Mizusaki, K. Kaneko +1
The long-standing problem of dramatic structure change near N=40 in Ge isotopes is investigated by means of large-scale shell model calculation. The analysis of simulated calculati…