Nanohertz gravitational waves from the baryon-dark matter coincidence
Alessia Musumeci, Jacopo Nava, Silvia Pascoli, Filippo Sala

TL;DR
This paper links nanohertz gravitational waves to a cosmological phase transition caused by baryon-dark matter asymmetry, proposing observable signals and experimental tests for this novel baryogenesis mechanism.
Contribution
It introduces a new baryogenesis model connecting dark matter asymmetry with a phase transition at 100 MeV, predicting observable gravitational waves and experimental signatures.
Findings
Phase transition at 100 MeV can produce detectable gravitational waves.
Dark matter self-interactions are near observational limits.
Model predicts lower maximum neutron star masses.
Abstract
The nanohertz gravitational waves (GW) observed by pulsar timing arrays may originate from a cosmological first-order phase transition (PT) at 100 MeV. Taking this possibility seriously motivates the question: why 100 MeV? We point out that a PT at exactly those scales is predicted by the generation of the baryon asymmetry from a dark asymmetry via resonant neutron-dark matter oscillations, and we prove that this PT can induce an observable GW signal compatibly with all experimental constraints. This proposal predicts dark matter self-interactions close to their observational upper limits and lowers the maximal expected mass of neutron stars. Independently of GW, this baryogenesis mechanism is tested by searches for missing-energy at the LHC and for neutron decays. We keep the model consistent with big-bang nucleosynthesis by adding heavy neutral leptons below 100 MeV, which…
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