Forbidden Scalar Dark Matter and Dark Higgses

TL;DR

This paper investigates how a dark Higgs field influences the relic abundance of sub-GeV dark matter in forbidden dark matter models, revealing significant effects even with weak couplings and potential detectability in future experiments.

Contribution

It introduces the role of a dark Higgs in forbidden dark matter models, showing it can significantly impact relic abundance calculations and experimental constraints.

Findings

Dark Higgs can alter relic abundance by orders of magnitude.

Effects remain significant even with small dark matter-Higgs couplings.

Model points consistent with observed dark matter are mildly constrained but testable soon.

Abstract

As experimental searches for WIMP dark matter continue to yield null results, models beyond the WIMP paradigm have proliferated in order to elude ever improving observational constraints, among them that of sub-GeV dark matter mediated by a massive vector portal (a dark photon) associated with a new dark $U(1)$ gauge symmetry. It has been previously noted that for a significant range of the parameter space of this class of models, the annihilation of dark matter particles into a pair of dark photons can dominate the freeze-out process even when this process is kinematically forbidden for dark matter at rest -- this is known as the "forbidden dark matter" (FDM) regime. Prior studies of this regime, however, assume that any "dark Higgs" associated with breaking the dark $U(1)$ and imparting mass to the dark photon is decoupled from the dark matter and as such plays no role in the freeze-out process. In this paper, we explore the effects of a dark Higgs on sub-GeV dark matter phenomenology in this FDM regime by considering the simplest possible construction in which there exist non-trivial dark matter-dark Higgs couplings: a model with a single complex scalar DM candidate coupled directly to the dark Higgs field. We find that for a wide range of parameter space, the dark Higgs can alter the resulting relic abundance by many orders of magnitude, and that this effect can remain significant even for a small dark matter-dark Higgs coupling constant. Considering measurements from direct detection and measurements of the CMB, we further find that points in this model's parameter space which recreate the appropriate dark matter relic abundance suffer only mild constraints from other sources at present, but may become accessible in near-future direct detection experiments.