Neutron star cooling in seven of eight transient outbursts from LMXBs is matched by thermonuclear heating leakage via an updated nscool boundary condition without ad hoc shallow heating.
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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.
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On a re-examination of neutron star cooling in transient sources -- No shallow heating required?
Neutron star cooling in seven of eight transient outbursts from LMXBs is matched by thermonuclear heating leakage via an updated nscool boundary condition without ad hoc shallow heating.
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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.