Abundance distribution of heavy nuclides up to a subnuclear density and the equation of state for gravitationally collapsing stars

摘要: With the use of empirical equations for binding and internal energies heavy nuclides with density dependence, abundance distribution neutron-excess which appear up to some subnuclear along collapsing trajectory a stellar core is calculated an assumption β-equilibrium condition. Free nucleons are simply assumed be non-interacting, degenerate fermions. Using thus derived, quantities affecting hydrodynamics core, such as average mass number fraction nuclides, free neutrons, electrons per baryon, excitation energy nucleus, entropy, pressure adiabatic index system then calculated. It found that we can obtain fairly reliable values these physical by introducing only magic near-magic in calculation, results hardly affected difference semi-empirical nuclear formula derive unknown grand partition function nuclides.