Bound-state formation, dissociation and decays of darkonium with potential non-relativistic Yukawa theory for scalar and pseudoscalar mediators
arXiv:2112.10145 · doi:10.1007/JHEP03(2022)172
Abstract
Dark matter models with light mediators featuring sizable interactions among dark particles enjoy an increasing attention in the model building community due to the elegance with which they can potentially explain the scaling relations governing galactic halos and clusters of galaxies. In the present work we continue our study of such models using non-relativistic and potential non-relativistic effective field theories (NREFTs and pNREFTs) and explore the properties of a Yukawa-type model with scalar and pseudoscalar interactions between a low-energetic scalar mediator and heavy dark matter fermions. In particular, we make first steps towards the formulation of such theories at finite temperature by providing the thermal bound-state formation rate and the thermal break-up of bound states from the self-energies of the dark-pair fields, that interact with the thermal environment. We estimate numerically bound-state effects on the dark matter energy density, that provide up to a correction depending on the relative size of the model couplings.
47 pages, 11 figures, journal version, references added
References in corpus (27)
- Secluded WIMP Dark Matter
- Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-5
- Cosmology and Astrophysics of Minimal Dark Matter
- The non-gravitational interactions of dark matter in colliding galaxy clusters
- Static quark-antiquark pairs at finite temperature
- Bound-state formation for thermal relic dark matter and unitarity
- Dark Nuclei I: Cosmology and Indirect Detection
- Dark-matter bound states from Feynman diagrams
- Non-relativistic bound states at finite temperature (I): the hydrogen atom
- Standard Model with a real singlet scalar and inflation
- Effects of QCD bound states on dark matter relic abundance
- Non-relativistic bound states at finite temperature (II): the muonic hydrogen
- Non-Abelian Electric Field Correlator at NLO for Dark Matter Relic Abundance and Quarkonium Transport
- On thermal corrections to near-threshold annihilation
- Re-derived overclosure bound for the inert doublet model
- Bound-state effects on dark matter coannihilation: Pushing the boundaries of conversion-driven freeze-out
- Freeze-in produced dark matter in the ultra-relativistic regime
- Higgs-mediated bound states in dark-matter models
- Dark matter bound state formation via emission of a charged scalar
- Effective Field Theories for Heavy Quarkonium
- Saha equilibrium for metastable bound states and dark matter freeze-out
- Muonic vs electronic dark forces: a complete EFT treatment for atomic spectroscopy
- Non-relativistic and potential non-relativistic effective field theories for scalar mediators
- Studies of a thermally averaged p-wave Sommerfeld factor
- Bound states of WIMP dark matter in Higgs-portal models. Part I. Cross-sections and transition rates
- Impact of bound states on non-thermal dark matter production
- Bound states of WIMP dark matter in Higgs-portal models. Part II. Thermal decoupling
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- Strong electroweak phase transition in -channel simplified dark matter models
- Excited bound states and their role in dark matter production
- Non-perturbative effects for dark sectors with QCD portals
- Final bound-state formation effect on dark matter annihilation
- Effective Field Theories for Dark Matter Pairs in the Early Universe