A multi-component SIMP model with
arXiv:2103.05956 · doi:10.1007/JHEP09(2021)028
Abstract
Multi-component dark matter scenarios are studied in the model with dark gauge symmetry that is broken into its product subgroup á la Krauss-Wilczek mechanism. In this setup, there exist two types of dark matter fields, and , distinguished by different charges. The real and imaginary parts of the -charged field, and , get different masses from the symmetry breaking. The field , which is another dark matter candidate due to the unbroken symmetry, belongs to the Strongly Interacting Massive Particle (SIMP)-type dark matter. Both and may contribute to 's annihilation processes, opening a new class of SIMP models with a local dark gauge symmetry. Depending on the mass difference between and , we have either two-component or three-component dark matter scenarios. In particular two- or three-component SIMP scenarios can be realised not only for small mass difference between and , but also for large mass hierarchy between them, which is a new and unique feature of the present model. We consider both theoretical and experimental constraints, and present four case studies of the multi-component dark matter scenarios.
v1: 25 pages; v2: 27 pages, references updated, analysis improved; v3: 31 pages, version accepted for publication in JHEP
References in corpus (19)
- Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-5
- New Limits on Hidden Photons from Past Electron Beam Dumps
- Scale invariant extension of the standard model with strongly interacting hidden sector
- Refined Bounds on MeV-scale Thermal Dark Sectors from BBN and the CMB
- Dark Matter from a Classically Scale-Invariant
- WIMP and SIMP Dark Matter from the Spontaneous Breaking of a Global Group
- Galactic center -ray excess in hidden sector DM models with dark gauge symmetries: local symmetry as an example
- MDM: A Model for Sterile Neutrino and Dark Matter Reconciles Cosmological and Neutrino Oscillation Data after BICEP2
- Residual Non-Abelian Dark Matter and Dark Radiation
- Inelastic Dark Matter Electron Scattering and the XENON1T Excess
- Vector SIMP dark matter
- Combined search for light dark matter with electron and muon beams at NA64
- Supersymmetric U(1)B x U(1)L model with leptophilic and leptophobic cold dark matters
- Light Dark Matter through Assisted Annihilation
- On thermal production of self-interacting dark matter
- The 3.5 keV X-ray line signature from annihilating and decaying dark matter in Weinberg model
- Implications of Two-component Dark Matter Induced by Forbidden Channels and Thermal Freeze-out
- Electroweak symmetry breaking and cold dark matter from hidden sector technicolor
- Complex Scalar Dark Matter in G2HDM
Cited by in corpus (13)
- A Two-Component Dark Matter Model and its Associated Gravitational Waves
- Scalar and Fermion Two-component SIMP Dark Matter with an Accidental Symmetry
- Two-component scalar and fermionic dark matter candidates in a generic U model
- Fermion and scalar two-component dark matter from a symmetry
- A two-component vector WIMP -- fermion FIMP dark matter model with an extended seesaw mechanism
- The model of three-component scalar dark matter
- Distinguishing two dark matter component particles at colliders
- Multi-component Dark Sectors: Symmetries, Asymmetries and Conversions
- An Asymmetric SIMP Dark Matter Model
- Scalar Dark Matter with Strong Positron Fluxes
- and strongly interacting dark matter with collider implications
- -charged Dark Matter in three-Higgs-doublet models
- The Influence of Lepton Portal on the WIMP-pFIMP framework