Three-dimensional band-structure calculations in the BCS approximation within HFB theory find that only 8% of free neutrons participate in superflow at baryon density 0.03 fm^{-3}, independent of the pairing gap.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2representative citing papers
Molecular dynamics simulations produce a new equation of state P(n_B, T) for warm neutron star outer crusts with tabulated data and neural network parametrization on Zenodo.
citing papers explorer
-
Superfluid fraction in the crystalline crust of a neutron star: role of BCS pairing
Three-dimensional band-structure calculations in the BCS approximation within HFB theory find that only 8% of free neutrons participate in superflow at baryon density 0.03 fm^{-3}, independent of the pairing gap.
-
Equation of State for warm Neutron Star outer crusts
Molecular dynamics simulations produce a new equation of state P(n_B, T) for warm neutron star outer crusts with tabulated data and neural network parametrization on Zenodo.