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WIMP and SIMP Dark Matter from the Spontaneous Breaking of a Global Group

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it
abstract

We propose and study a scalar extension of the Standard Model which respects a $\mathbb{Z}_3$ symmetry remnant of the spontaneous breaking of a global $U(1)_\text{DM}$ symmetry. Consequently, this model has a natural dark matter candidate and a Goldstone boson in the physical spectrum. In addition, the Higgs boson properties are changed with respect to the Standard Model due to the mixing with a new particle. We explore regions in the parameter space taking into account bounds from the measured Higgs properties, dark matter direct detection as well as measurements of the effective number of neutrino species before recombination. The dark matter relic density is determined by three classes of processes: the usual self-annihilation, semi-annihilation and purely dark matter $3 \to 2$ processes. The latter has been subject of recent interest leading to the so-called `Strongly Interacting Massive Particle' (SIMP) scenario. We show under which conditions our model can lead to a concrete realization of such scenario and study the possibility that the dark matter self-interactions could address the small scale structure problems. In particular, we find that in order for the SIMP scenario to work, the dark matter mass must be in the range $7-115$ MeV, with the global symmetry energy breaking scale in the TeV range.

citation-role summary

background 1 method 1

citation-polarity summary

years

2026 2 2019 1

representative citing papers

Tachyonic gravitational dark matter production after inflation

astro-ph.CO · 2026-01-12 · accept · novelty 7.0

Tachyonic instabilities from post-inflation curvature reorganization via quadratic Gauss-Bonnet coupling produce the observed dark matter relic density across wide mass and scale ranges, backed by lattice simulations and a fitting function.

Axion-Like Electrophilic Portal for Pion Dark Matter

hep-ph · 2026-02-02 · unverdicted · novelty 5.0

A minimal electrophilic ALP portal for SIMP pion dark matter widens the allowed parameter space, making an ALP mass of order 10 MeV viable and consistent with the X17 anomaly.

citing papers explorer

Showing 3 of 3 citing papers.

  • Tachyonic gravitational dark matter production after inflation astro-ph.CO · 2026-01-12 · accept · none · ref 132 · internal anchor

    Tachyonic instabilities from post-inflation curvature reorganization via quadratic Gauss-Bonnet coupling produce the observed dark matter relic density across wide mass and scale ranges, backed by lattice simulations and a fitting function.

  • Axion-Like Electrophilic Portal for Pion Dark Matter hep-ph · 2026-02-02 · unverdicted · none · ref 6 · internal anchor

    A minimal electrophilic ALP portal for SIMP pion dark matter widens the allowed parameter space, making an ALP mass of order 10 MeV viable and consistent with the X17 anomaly.

  • Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos hep-ph · 2019-07-09 · unverdicted · none · ref 170 · internal anchor

    The thesis presents a new 3-to-2 freezeout mechanism, bound-state effects on searches, a new axion interferometric search, reionization assessments, 21-cm constraints, and the DarkHistory code for ionization and thermal histories.