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.
Collective Modes in a Superfluid Neutron Gas within the Quasiparticle Random-Phase Approximation
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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.