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  • Open Access

Gravitational wave production and baryogenesis in a simple left-right model

Arnab Dasgupta1,*, Matthew Knauss2,†, and Marc Sher2,‡

  • 1Pittsburgh Particle Physics, Astrophysics, and Cosmology Center, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15206, USA
  • 2High Energy Theory Group, Department of Physics, William & Mary, Williamsburg, Virginia 23187, USA

  • *Contact author: arnabdasgupta@pitt.edu
  • †Contact author: mhknauss@wm.edu
  • ‡Contact author: mtsher@wm.edu

Phys. Rev. D 112, 055034 – Published 24 September, 2025

DOI: https://doi.org/10.1103/x9v8-b1j4

Abstract

The left-right model with the simplest Higgs structure has a SU(2)L doublet HL, a SU(2)R doublet HR, and a singlet σ that couples to the doublets as σ(|HL|2−|HR|2). The left-right symmetry has HL↔HR and σ↔−σ. We study gravitational wave production and baryogenesis in the electroweak phase transitions in the model. For two benchmark points, σ first gets a vev, followed by HR and then HL. An interesting feature is that the vev of HL is initially much higher than its zero temperature value, leading to a more strongly first-order transition and higher frequency gravitational waves. An unusual benchmark point has the σ vev at zero when the electroweak symmetry breaks. This results in both HL and HR vevs being equal and in the multi-TeV range. At a lower temperature, the σ vev turns on, breaking the left-right symmetry and HL drops to its standard model value. Since the electroweak symmetry is broken at the multi-TeV scale, the frequency of gravitational waves will be much higher than usual. Baryogenesis is also discussed.

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