Probing superheavy dark matter with gravitational waves

TL;DR

This paper explores a superheavy dark matter model within an extended $B-L$ framework, proposing that gravitational wave detection from cosmic strings can test dark matter masses far beyond traditional limits.

Contribution

It introduces a novel superheavy dark matter scenario with co-annihilation effects, enabling masses above the Griest-Kamionkowski bound, and demonstrates testability via gravitational wave signals from cosmic strings.

Findings

Dark matter mass up to $10^{13}$ GeV is achievable.

Future gravitational wave detectors can probe dark matter in the $10^9$ to $10^{13}$ GeV range.

The scenario links superheavy dark matter to observable gravitational wave signatures.

Abstract

We study the superheavy dark matter (DM) scenario in an extended $B-L$ model, where one generation of right-handed neutrino $\nu_R$ is the DM candidate. If there is a new lighter sterile neutrino that co-annihilate with the DM candidate, then the annihilation rate is exponentially enhanced, allowing a DM mass much heavier than the Griest-Kamionkowski bound ($\sim10^5$ GeV). We demonstrate that a DM mass $M_{\nu_R}\gtrsim10^{13}$ GeV can be achieved. Although beyond the scale of any traditional DM searching strategy, this scenario is testable via gravitational waves (GWs) emitted by the cosmic strings from the $U(1)_{B-L}$ breaking. Quantitative calculations show that the DM mass $\mathcal{O}(10^9-10^{13}~{\rm GeV})$ can be probed by future GW detectors.