Pairing properties and specific heat of the inner crust of a neutron star
arXiv:1412.8410 · doi:10.1103/PhysRevC.91.015809
Abstract
We investigate the pairing properties at finite temperature of the Wigner-Seitz cells in the inner crust of a neutron star obtained with the recent Brussels-Montreal Skyrme functional BSk21. In particular we analyze the phenomena of persistence and reentrance of pairing correlations and their impact on the specific heat in the low-density region of the inner crust.
Submitted to Phys. Rev. C
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- Superfluidity and Superconductivity in Neutron Stars
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- A new statistical method for the structure of the inner crust of neutron stars
- Properties of a quantum vortex in neutron matter
- Entrainment effects in neutron-proton mixtures within the nuclear-energy density functional theory. II. Finite temperatures and arbitrary currents
- Pairing effects in nuclear pasta phase within the relativistic Thomas-Fermi formalism