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Phase transitions and gravitational waves in a non-Abelian vector dark matter scenario

Nico Benincasa1,*, Luigi Delle Rose2,3,†, Luca Panizzi2,3,‡, Maimoona Razzaq2,3,§, and Savio Urzetta2,∥

  • *Contact author: nico.benincasa@kbfi.ee
  • †Contact author: luigi.dellerose@unical.it
  • ‡Contact author: luca.panizzi@unical.it
  • §Contact author: maimoona.razzaq@unical.it
  • ∥Contact author: sav.urze98@gmail.com

Phys. Rev. D 112, 095004 – Published 7 November, 2025

DOI: https://doi.org/10.1103/xd9f-bq4p

Abstract

We study a scenario where the Standard Model is extended by a SU(2) gauge group in the dark sector. The three associated dark gauge bosons are stabilized via a custodial symmetry triggered by an additional dark SU(2) scalar doublet, thus making them viable dark-matter candidates. After considering the most recent constraints for this model, we analyze the phase transition dynamics and compute the power spectrum of the resulting stochastic gravitational-wave background. Finally, we find regions of the parameter space yielding the observed dark-matter relic density while also leading to a strong enough phase transition with an associated gravitational-wave signal reaching the sensitivity of a future space-based gravitational-wave detector, such as LISA, DECIGO, BBO, TianQin, or Taiji.

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