Reshuffled Strongly Interacting Massive Particle Dark Matter
arXiv:2107.04375 · doi:10.1016/j.dark.2022.101061
Abstract
In this work, we reanalyze the multi-component strongly interacting massive particle (mSIMP) scenario using an effective operator approach. As in the single-component SIMP case, the total relic abundance of mSIMP dark matter (DM) is determined by the coupling strengths of processes achieved by a five-point effective operator. Intriguingly, we notice that there is an irreducible process induced by the corresponding five-point interaction in the dark sector, which would reshuffle the mass densities of SIMP DM after the chemical freeze-out. We dub this DM scenario as reshuffled SIMP (SIMP). Given this observation, we then numerically solve the coupled Boltzmann equations including the and processes to get the correct yields of SIMP DM. It turns out that the masses of SIMP DM must be nearly degenerate for them to contribute sizable abundances. On the other hand, we also introduce effective operators to bridge the dark sector and visible sector via a vector portal coupling. Notably, we find that the reshuffled mechanism in the SIMP scenario is sensitive to the size of the DM self-interacting cross section.
arXiv comment8 pages, 3 figures, 3 tables, the title changed. Matches the version published in Phys.Dark Univ
References in corpus (33)
- 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
- The SIMPlest Miracle
- 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
- Elastically Decoupling Dark Matter
- Scale invariant extension of the standard model with strongly interacting hidden sector
- SIMP Spectroscopy
- On the interpretation of dark matter self-interactions in Abell 3827
- The Scale of Dark QCD
- SIMPs through the axion portal
- Hidden sector monopole, vector dark matter and dark radiation with Higgs portal
- Co-SIMP Miracle
- Electroweak symmetry breaking and cold dark matter from strongly interacting hidden sector
- Cosmic abundances of SIMP dark matter
- The effect of quark interactions on dark matter kinetic decoupling and the mass of the smallest dark halos
- Resonant SIMP dark matter
- Vector SIMP dark matter with approximate custodial symmetry
- Dark Matter in Anomaly-Free Gauge Extensions
- Scalar and Fermion Two-component SIMP Dark Matter with an Accidental Symmetry
- Split SIMPs with Decays
- AdS/QCD approach to the scale-invariant extension of the standard model with a strongly interacting hidden sector
- Implications of Two-component Dark Matter Induced by Forbidden Channels and Thermal Freeze-out
- SIMPler realisation of Scalar Dark Matter
- Electroweak symmetry breaking and cold dark matter from hidden sector technicolor
- Hidden Monopole Dark Matter via Axion Portal and its Implications for Direct Detection Searches, Beam-Dump Experiments, and the Tension
- Cosmology and prospects for sub-MeV dark matter in electron recoil experiments
- Enhanced n-body annihilation of dark matter and its indirect signatures
- Thermodynamic Evolution of Secluded Vector Dark Matter: Conventional WIMPs and Nonconventional WIMPs
- Probing multicomponent FIMP scenarios with gamma-ray telescopes
- Numerical evaluation of a two loop diagram in the cutoff regularization
- Comment on "New Freezeout Mechanism for Strongly Interacting Dark Matter"