This research proposes a comprehensive program to constrain dark matter spike evolution through neutron star tidal heating signatures, developing a theoretical framework and multi-messenger observational strategies.
Key findings
Develops a novel theoretical framework connecting DM spike density profiles to tidal heating rates.
Performs N-body simulations to quantify feedback between spike dynamics and orbital evolution.
Constructs gravitational wave templates incorporating tidal heating and DM spike effects.
Designs a multi-messenger observational campaign to constrain spike properties.
Derives constraints on DM microphysics from anomalous tidal heating observations.
Limitations & open questions
Assumes the validity of current dark matter models and the accuracy of N-body simulations.
Relies on the availability and sensitivity of future gravitational wave and multi-messenger detectors.