Relativistic mean-field calculations with asymmetric finite differences find that neutron-star inner-crust binding energies decrease with larger symmetry-energy slope L and larger nucleon effective mass, while quantum shell effects produce oscillatory densities and alter neutron properties.
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Skyrme-HF calculations of beta+ and EC half-lives in 290Fl, 293Mc, 294Lv, 295Ts indicate alpha decay is the dominant mode.
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Relativistic mean-field study of the neutron star inner crust using the asymmetric finite difference method
Relativistic mean-field calculations with asymmetric finite differences find that neutron-star inner-crust binding energies decrease with larger symmetry-energy slope L and larger nucleon effective mass, while quantum shell effects produce oscillatory densities and alter neutron properties.
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Microscopic calculations of weak decays in superheavy nuclei
Skyrme-HF calculations of beta+ and EC half-lives in 290Fl, 293Mc, 294Lv, 295Ts indicate alpha decay is the dominant mode.