Elementary excitations in homogeneous superfluid neutron star matter: role of the neutron-proton coupling

TL;DR

This paper investigates the elementary excitations in superfluid neutron star matter, emphasizing the neutron-proton coupling effects on spectral functions and collective modes within a superfluid framework.

Contribution

It introduces a generalized Random Phase Approximation formalism that accounts for superfluidity and neutron-proton interactions in neutron star matter.

Findings

Protons influence neutron spectral functions via nuclear interactions.

Proton spectral function exhibits a pseudo-Goldstone mode below 2Δ.

Neutron spectral function shows a collective sound mode at higher densities.

Abstract

The thermal evolution of Neutron Stars is affected by the elementary excitations that characterize the stellar matter. In particular, the low-energy excitations, with a spectrum linear in momentum, can play a major role in the emission and propagation of neutrinos. In this paper, we focus on the elementary modes in the region of proton superfluidity, where the neutron component is expected to have a very small or zero pairing gap. We study the overall spectral functions of protons, neutrons and electrons on the basis of the Coulomb and nuclear interactions. This study is performed in the framework of the Random Phase Approximation, generalized in order to describe the response of a superfluid system. The formalism we use ensures that the Generalized Ward's Identities are satisfied. Despite their relative small fraction, the protons turn out to modify the neutron spectral function as a consequence of the nuclear neutron-proton interaction. This effect is particularly evident at the lower density, just below the crust for a density close to the saturation value, while at increasing density the neutrons and the protons are mainly decoupled. The proton spectral function is characterized by a pseudo-Goldstone mode below $ 2\Delta $, twice the pairing gap, and a pair-breaking mode above $ 2\Delta $. The latter merges in the sound mode of the normal phase at higher momenta. The neutron spectral function develops a collective sound mode only at the higher density. The electrons have a strong screening effect on the proton-proton interaction at the lower momenta, and decouple from the protons at higher momenta.