Interband response enhances the neutron superfluid fraction in the crystalline crust, yielding effective ion masses close to the mass of quantum mechanically bound nucleons for realistic pairing gaps.
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astro-ph.HE 2years
2026 2verdicts
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Bayesian modeling with informed priors reduces uncertainties in neutron-star crust shear properties, predicting torsional mode frequencies of 20-50 Hz compatible with observations.
citing papers explorer
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Superfluid fraction and effective ion mass in the crystalline crust of a neutron star: role of interband response
Interband response enhances the neutron superfluid fraction in the crystalline crust, yielding effective ion masses close to the mass of quantum mechanically bound nucleons for realistic pairing gaps.
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Bayesian analysis of the shear modulus in the neutron-star crust
Bayesian modeling with informed priors reduces uncertainties in neutron-star crust shear properties, predicting torsional mode frequencies of 20-50 Hz compatible with observations.