Self-consistent HFB calculations with Bloch boundary conditions show more than 90% of neutrons are superfluid in the inner crust crystal phase above 0.03 fm^{-3}, nearly independent of interaction and geometry details.
Low-energy collec- tive excitations in the neutron star inner crust
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
nucl-th 1years
2025 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Superfluid fraction in the crystal phase of the inner crust of neutron stars
Self-consistent HFB calculations with Bloch boundary conditions show more than 90% of neutrons are superfluid in the inner crust crystal phase above 0.03 fm^{-3}, nearly independent of interaction and geometry details.