A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …

Abstract According to the Hugenholtz–Van Hove theorem, nuclear symmetry energy E sym
(ρ) and its slope L (ρ) at an arbitrary density ρ are determined by the nucleon isovector …

Resorting to a neural network approach we refined several representative and sophisticated
global nuclear mass models within the latest atomic mass evaluation (AME2012). In the …

The global nuclear mass based on the macroscopic–microscopic model was studied by
applying a newly designed multi-task learning artificial neural network (MTL-ANN). First, the …

We present an upgraded review of our microscopic investigation on the single-particle
properties and the EOS of isospin asymmetric nuclear matter within the framework of the …

Abstract Atomic Mass Evaluation (AME2016) has replenished the latest nuclear binding
energy data. Other physical observables, such as the separated energies, decay energies …

By using point-coupling versions of finite-range nuclear relativistic mean-field models
containing cubic and quartic self-interactions in the scalar field σ, a nonrelativistic limit is …

We extract the mass-dependent symmetry energy coefficients a sym (A) with the nuclear
mass differences reducing the uncertainties as far as possible. The estimated a sym (A) of …

An improved macroscopic–microscopic nuclear mass formula is presented in which shell
and pairing effects are simultaneously evaluated by a procedure similar to Strutinsky …

The nuclear symmetry energy coefficients of finite nuclei are extracted by using the
differences between the masses of isobaric nuclei. Based on the masses of more than 2400 …