Scalar and Fermion Two-component SIMP Dark Matter with an Accidental Symmetry
arXiv:2201.06856 · doi:10.1007/JHEP03(2022)005
Abstract
In this paper, we construct for the first time a two-component strongly interacting massive particles (SIMP) dark matter (DM) model, where a complex scalar and a vector-like fermion play the role of the SIMP DM candidates. These two particles are stable due to an accidental symmetry after the breaking of a gauge symmetry. By introducing one extra complex scalar as a mediator between the SIMP particles, this model can have processes that determine the DM relic density. On the other hand, the SIMP DM particles can maintain kinetic equilibrium with the thermal bath until the DM freeze-out temperature via the gauge couplings. Most importantly, we find an unavoidable two-loop induced process tightly connecting to the process that would redistribute the SIMP DM number densities after the chemical freeze-out of DM. Moreover, this redistribution would significantly modify the predictions of the self-interacting cross section of DM compared with other SIMP models. It is crucial to include the two-loop induced annihilations to obtain the correct DM phenomenology.
30 pages, 10 figures, 3 tables, and 2 appendices; references added, minor corrections, and match to published version
References in corpus (41)
- Secluded WIMP Dark Matter
- Dark Matter Self-interactions and Small Scale Structure
- Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56
- Weak lensing mass reconstruction of the interacting cluster 1E0657-558: Direct evidence for the existence of dark matter
- The SIMP Miracle
- Astrophysical Signatures of Secluded Dark Matter
- Beyond Collisionless Dark Matter: Particle Physics Dynamics for Dark Matter Halo Structure
- The SIMPlest Miracle
- Dark matter production in the early Universe: beyond the thermal WIMP paradigm
- Why Baryons Matter: The Kinematics of Dwarf Spheroidal Satellites
- Towards a precision calculation of in the Standard Model II: Neutrino decoupling in the presence of flavour oscillations and finite-temperature QED
- A precision calculation of relic neutrino decoupling
- A Lower Bound on the Mass of Cold Thermal Dark Matter from Planck
- How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves
- Primordial gravitational waves, precisely: The role of thermodynamics in the Standard Model
- The behaviour of dark matter associated with 4 bright cluster galaxies in the 10kpc core of Abell 3827
- SIMP Spectroscopy
- Neutrino decoupling beyond the Standard Model: CMB constraints on the Dark Matter mass with a fast and precise evaluation
- On the interpretation of dark matter self-interactions in Abell 3827
- SIMPs through the axion portal
- Global Constraints on Effective Dark Matter Interactions: Relic Density, Direct Detection, Indirect Detection, and Collider
- Hidden sector monopole, vector dark matter and dark radiation with Higgs portal
- Determining Dark Matter-Electron Scattering Rates from the Dielectric Function
- Co-SIMP Miracle
- Cosmic abundances of SIMP dark matter
- The Higgs Portal to Cosmology
- Velocity Dependence from Resonant Self-Interacting Dark Matter
- The effect of quark interactions on dark matter kinetic decoupling and the mass of the smallest dark halos
- Resonant SIMP dark matter
- On thermal production of self-interacting dark matter
- Dark Matter Daily Modulation With Anisotropic Organic Crystals
- Vector SIMP dark matter with approximate custodial symmetry
- Split SIMPs with Decays
- A Radiative Neutrino Mass Model with SIMP Dark Matter
- Implications of Two-component Dark Matter Induced by Forbidden Channels and Thermal Freeze-out
- A multi-component SIMP model with
- SIMPler realisation of Scalar Dark Matter
- Hidden Monopole Dark Matter via Axion Portal and its Implications for Direct Detection Searches, Beam-Dump Experiments, and the Tension
- Enhanced n-body annihilation of dark matter and its indirect signatures
- Cosmology and prospects for sub-MeV dark matter in electron recoil experiments
- Probing multicomponent FIMP scenarios with gamma-ray telescopes
Cited by in corpus (13)
- A Two-Component Dark Matter Model and its Associated Gravitational Waves
- A two-component vector WIMP -- fermion FIMP dark matter model with an extended seesaw mechanism
- The model of three-component scalar dark matter
- An Asymmetric SIMP Dark Matter Model
- Gravitational wave effects and phenomenology of a two-component dark matter model
- Prospecting bipartite Dark Matter through Gravitational Waves
- The centers of discrete groups as stabilizers of Dark Matter
- -charged Dark Matter in three-Higgs-doublet models
- Gravitational wave signatures of first-order phase transition in two-component dark matter model
- Bouncing Dark Matter
- Reshuffled Strongly Interacting Massive Particle Dark Matter
- Spin Trio: a dark matter scenario
- Light Thermal Self-Interacting Dark Matter in the Shadow of Non-Standard Cosmology