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.
Proximity effect of pair correlation in the inner crust of neutron stars
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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.