Revisiting Singlet Fermion Dark Matter with a Scalar Portal: Connecting Higgs Phenomenology and Strong Electroweak Phase Transition

TL;DR

This paper explores a minimal Standard Model extension with a singlet scalar and fermion dark matter, demonstrating that a strong electroweak phase transition and observable gravitational waves can occur without conflicting with collider and detection constraints.

Contribution

It introduces a novel scenario where the scalar does not acquire a VEV at zero temperature, decoupling Higgs mixing from the phase transition, and links collider, dark matter, and gravitational wave phenomenology.

Findings

Strong first-order electroweak phase transition achieved in selected parameter space.

Predicted gravitational wave signals could be detected by future space-based interferometers.

Model remains consistent with current collider and dark matter detection constraints.

Abstract

We investigate a minimal extension of the Standard Model with a real singlet scalar and a singlet Dirac fermion acting as dark matter. Unlike a conventional singlet scalar setup, we assume that the singlet scalar does not acquire a vacuum expectation value at zero temperature. This decouples the scalar mixing angle from the Higgs-portal quartic coupling responsible for the strong first-order electroweak phase transition, allowing it to coexist with current collider and direct-detection constraints. The Higgs-singlet mixing is generated independently through a trilinear portal interaction. We check theoretical consistency conditions, various LHC limits on heavy scalar resonances, dark matter relic abundance, and direct detection bounds to delineate the viable parameter space. We perform a detailed analysis of the electroweak phase transition and show that a strong first-order transition is realized for a selected set of benchmark points. We further compute the resulting stochastic gravitational wave spectra and find that several scenarios yield signals potentially observable at future space-based interferometers. Our results establish a unified and testable framework that connects collider phenomenology, first-order electroweak phase transition, and the resulting production of gravitational waves, along with the dark matter phenomenology, all within a simple renormalizable extension of the Standard Model.