24–28 Aug 2026
Leiden University
Europe/Zurich timezone

Nanohertz Gravitational Waves from the Baryon-Dark Matter coincidence

Not scheduled
20m
Gorlaeus gebouw (Leiden University)

Gorlaeus gebouw

Leiden University

Einsteinweg 55, 2333 CC Leiden
Talk Gravitational Waves

Speaker

Jacopo Nava (Vrije Universiteit Brussels)

Description

The nanohertz gravitational-wave (GW) signal observed by pulsar timing arrays may originate from a cosmological first-order phase transition (FOPT) at temperatures of order 100 MeV. This coincidence raises a fundamental question: why this scale? We show that such a PT naturally arises in scenarios where the baryon asymmetry is generated from a dark asymmetry via resonant neutron-dark matter (DM) oscillations.

We demonstrate that the same PT can produce a GW signal compatible with NANOGrav observations while satisfying all current experimental and cosmological constraints. The framework predicts DM self-interactions close to observational bounds and a reduced maximum mass for neutron stars. It also offers complementary probes through missing-energy searches at the LHC and neutron decay experiments.

Consistency with big-bang nucleosynthesis is ensured by introducing O (10-100) MeV scale heavy neutral leptons, which simultaneously account for neutrino masses and provide additional experimental signatures.

Authors

Alessia Musumeci (Technical University of Munich) Filippo Sala Jacopo Nava (Vrije Universiteit Brussels) Silvia Pascoli (Universita Di Bologna (IT))

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