Probing freeze-in dark matter using Bose-Einstein condensate in neutron star

TL;DR

This paper explores how Bose-Einstein condensates of bosonic dark matter inside neutron stars can significantly enhance annihilation rates, leading to observable heating effects detectable by telescopes like JWST.

Contribution

It introduces a novel scenario where condensate formation amplifies dark matter annihilation, providing new observational and theoretical insights into dark matter properties.

Findings

Annihilation rate can increase by 10^15 to 10^20 times due to condensate formation.

Neutron star heating from dark matter annihilation can be detected by JWST.

This scenario probes dark matter-nucleon interactions in the neutrino fog regime.

Abstract

Neutron star (NS) is one of the most promising astrophysical targets to probe non-gravitational interaction of dark matter (DM) with visible matter. Their compactness makes them an ideal object which can capture particle DM efficiently over its lifetime using the DM-nucleon scattering cross-section. If DM particles are bosonic, then the captured DM population may form a Bose-Einstein condensate at the center of the NS, increasing the DM density significantly. In this work, we study the phenomenology of such scenario with enhanced DM annihilation rate due to the increased density in a condensate. The enhanced DM annihilation makes the NS surface `hotter' than in the standard cooling scenario. We show that the annihilation rate is enhanced by a factor of $\mathcal{O}(10^{15}-10^{20})$ if DM forms a condensate, and DM with freeze-in value annihilation cross-section can heat up the NS to higher temperatures, bringing it within the reach of James Webb Space Telescope. It also allows us to probe DM-nucleon scattering cross section within the neutrino fog regime which will complement the terrestrial direct detection searches. Moreover, the enhanced annihilation from the condensate changes the lower limits on s-wave DM annihilation cross-section for capture-annihilation equilibrium and the formation of a black hole inside the NS. Finally, we show an example of a scalar DM model where such small annihilation and DM-nucleon scattering cross sections can generically arise.