Electroweak baryogenesis and gravitational waves from a real scalar singlet
Ville Vaskonen
TL;DR
This work analyzes a minimal SM extension with a real scalar singlet that enables a strong first-order electroweak phase transition and introduces CP violation through a dimension-6 operator modifying the top-quark mass. By solving transport equations for baryogenesis and computing the associated gravitational-wave spectrum from the phase transition, the authors reveal a robust correlation: larger new-physics scales Λ yield stronger gravitational waves while still achieving the observed baryon asymmetry. They demonstrate that future space-based detectors like LISA and BBO can probe the parameter space, including regions with high Λ, linking cosmological baryogenesis to observable gravitational waves. The study also highlights the role of two-step phase-transition dynamics and wall-velocity effects in shaping both η_B and the GW signal, offering conservative predictions and avenues for more detailed future work on bubble-wall dynamics.
Abstract
We consider a real scalar singlet field which provides a strong first-order electroweak phase transition via its coupling to the Higgs boson, and gives a $CP$ violating contribution on the top quark mass via a dimension-6 operator. We study the correlation between the baryon-to-entropy ratio produced by electroweak baryogenesis, and the gravitational wave signal from the electroweak phase transition. We show that future gravitational wave experiments can test, in particular, the region of the model parameter space where the observed baryon-to-entropy ratio can be obtained even if the new physics scale, which is explicit in the dimension-6 operator, is high.
