Derives exact expressions for pressure and chemical potentials in the neutron star inner crust within Hartree-Fock and extended Thomas-Fermi frameworks, applicable to catalyzed and accreted matter, with examples using BSk24.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
nucl-th 2verdicts
UNVERDICTED 2representative citing papers
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.
citing papers explorer
-
Pressure and chemical potentials in the inner crust of a cold neutron star within Hartree-Fock and extended Thomas-Fermi methods
Derives exact expressions for pressure and chemical potentials in the neutron star inner crust within Hartree-Fock and extended Thomas-Fermi frameworks, applicable to catalyzed and accreted matter, with examples using BSk24.
-
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.