Perturbative Unitarity of Strongly Interacting Massive Particle Models
arXiv:2210.01393 · doi:10.1007/JHEP02(2023)217
Abstract
Dark pion is a promising candidate for the strongly interacting massive particle dark matter. A large pion self-coupling tends to be required for correct relic abundance, and hence the partial-wave amplitudes can violate the perturbative unitarity even for the coupling within naïve perturbative regime. We improve the partial-wave amplitudes in order to satisfy the optical theorem. We demonstrate that the improvement is relevant only for semi-relativistic pions, and thus this does not affect the self-scattering cross section at the cosmic structures. We also discuss the impact of the improvement of the scattering process, and we find that there is an upper bound on at which the correct relic abundance is never achieved even at large due to the optical theorem.
arXiv comment17+26 pages, 5 figures, discussions improved, figures modified, version published in JHEP
References in corpus (57)
- Observational evidence for self-interacting cold dark matter
- Dark Matter Self-interactions and Small Scale Structure
- The SIMP Miracle
- Walking in the SU(N)
- The SIMPlest Miracle
- The inverse amplitude method in Chiral Perturbation Theory
- Dark Matter from new Technicolor Theories
- Generalized Dimensional Analysis
- Review of strongly-coupled composite dark matter models and lattice simulations
- Composite dark matter from a model with composite Higgs boson
- Hidden SU(N) Glueball Dark Matter
- Strong Interactive Massive Particles from a Strong Coupled Theory
- Aidnogenesis via Leptogenesis and Dark Sphalerons
- Technicolor Dark Matter
- Self-healing of unitarity in effective field theories and the onset of new physics
- Big Bang Darkleosynthesis
- Big Bang Synthesis of Nuclear Dark Matter
- Fundamental Composite Higgs Dynamics on the Lattice: SU(2) with Two Flavors
- Making Asymmetric Dark Matter Gold: Early Universe Synthesis of Nuggets
- Dynamical generation of the weak and Dark Matter scales from strong interactions
- Nuclear Structure of Bound States of Asymmetric Dark Matter
- Cosmic Signals from the Hidden Sector
- Non-Abelian Dark Forces and the Relic Densities of Dark Glueballs
- Dark Nuclei II: Nuclear Spectroscopy in Two-Colour QCD
- Dark Matter as a weakly coupled Dark Baryon
- Stealth Dark Matter: Dark scalar baryons through the Higgs portal
- Composite Goldstone Dark Matter: Experimental Predictions from the Lattice
- Cosmic abundances of SIMP dark matter
- Phenomenology of ELDER Dark Matter
- Thermal Squeezeout of Dark Matter
- Signatures of Large Composite Dark Matter States
- Direct Detection of Stealth Dark Matter through Electromagnetic Polarizability
- Precise WIMP Dark Matter Abundance and Standard Model Thermodynamics
- Astrophysical Signatures of Asymmetric Dark Matter Bound States
- A general theoretical description of N-body recombination
- Vector SIMP dark matter
- Meson-meson Scattering in QCD-like Theories
- Lattice calculation of composite dark matter form factors
- Dark Matter and Neutrino Mass from the Smallest Non-Abelian Chiral Dark Sector
- Dark Matter from Strong Dynamics: The Minimal Theory of Dark Baryons
- A Practical and Consistent Parametrization of Dark Matter Self-Interactions
- Analyticity, Crossing Symmetry and the Limits of Chiral Perturbation Theory
- Composite Asymmetric Dark Matter with a Dark Photon Portal
- Asymmetric Dark Matter and the hadronic spectra of hidden QCD
- Accidentally Asymmetric Dark Matter
- Production of dark-matter bound states in the early universe by three-body recombination
- Asymmetric Dark Matter May Not Be Light
- Signals of composite electroweak-neutral Dark Matter: LHC/Direct Detection interplay
- Split SIMPs with Decays
- Electroweak Corrections in Technicolor Reconsidered
- Glueballs in a Thermal Squeezeout Model
- Unitarity limits on thermal dark matter in (non-)standard cosmologies
- Partially Composite Dark Matter
- Bosonic-Seesaw Portal Dark Matter
- Asymmetric accidental composite dark matter
- Enhanced n-body annihilation of dark matter and its indirect signatures
- Stealth QCD-like Strong Interactions and the t-tbar Asymmetry