Split SIMPs with Decays
Andrey Katz, Ennio Salvioni, Bibhushan Shakya

TL;DR
This paper presents a minimal SIMP dark matter model with a dark QCD sector, exploring mass splittings, stability, and decay of dark mesons, and demonstrates its viability against cosmological and experimental constraints.
Contribution
It introduces a novel SIMP cosmology with large mass splittings and long-lived unstable mesons, and discusses an ultraviolet completion within neutral naturalness.
Findings
SIMP mechanism effectively sets dark matter relic density with mass splittings.
Unstable dark mesons can decay without conflicting with CMB constraints.
The model's phenomenology is compatible with cosmological and terrestrial probes.
Abstract
We discuss a minimal realization of the strongly interacting massive particle (SIMP) framework. The model includes a dark copy of QCD with three colors and three light flavors. A massive dark photon, kinetically mixed with the Standard Model hypercharge, maintains kinetic equilibrium between the dark and visible sectors. One of the dark mesons is necessarily unstable but long-lived, with potential impact on CMB observables. We show that an approximate "isospin" symmetry acting on the down-type quarks is an essential ingredient of the model. This symmetry stabilizes the dark matter and allows to split sufficiently the masses of the other states to suppress strongly their relic abundances. We discuss for the first time the SIMP cosmology with sizable mass splittings between all meson multiplets. We demonstrate that the SIMP mechanism remains efficient in setting the dark matter relic…
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