Microscopic DFT+QRPA calculation shows the effective coupling constant between nuclear clusters and superfluid phonons in the neutron-star inner crust is substantially smaller than hydrodynamical estimates due to suppression of the phonon amplitude inside and around the clusters.
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Hybrid star model with core quark pasta pinning superfluid vortices produces glitch amplitudes ΔΩ/Ω of order 10^{-6} matching Vela-like pulsar observations.
A review of spin effects, superfluidity, and magnetic fields in neutron matter and their influence on neutron-star structure, superfluid phases, and rotational dynamics.
citing papers explorer
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Interaction between nuclear clusters and superfluid phonons in the neutron-star inner crust
Microscopic DFT+QRPA calculation shows the effective coupling constant between nuclear clusters and superfluid phonons in the neutron-star inner crust is substantially smaller than hydrodynamical estimates due to suppression of the phonon amplitude inside and around the clusters.
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Modeling large glitches with core superfluidity in a Hybrid star
Hybrid star model with core quark pasta pinning superfluid vortices produces glitch amplitudes ΔΩ/Ω of order 10^{-6} matching Vela-like pulsar observations.
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Spin effects in superfluidity, neutron matter and neutron stars
A review of spin effects, superfluidity, and magnetic fields in neutron matter and their influence on neutron-star structure, superfluid phases, and rotational dynamics.