TL;DR
This paper reviews the general relativistic macroscopic description of superfluid neutron star interiors and presents new findings on oscillation modes influenced by superfluidity, including the discovery of a new class of modes.
Contribution
It introduces a comprehensive relativistic framework for superfluid neutron star interiors and reports novel oscillation modes caused by superfluid effects.
Findings
Identification of a new class of oscillation modes in superfluid neutron stars
Development of a general relativistic model for neutron star superfluidity
Insights into the impact of superfluidity on neutron star oscillations
Abstract
Neutron stars are believed to contain (neutron and proton) superfluids. I will give a summary of a macroscopic description of the interior of neutron stars, in a formulation which is general relativistic. I will also present recent results on the oscillations of neutron stars, with superfluidity explicitly taken into account, which leads in particular to the existence of a new class of modes.
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