Sommerfeld-corrected relic abundance of wino dark matter with NLO electroweak potentials
arXiv:2009.00640 · doi:10.1007/JHEP02(2021)020
Abstract
Extending previous work, we calculate the electroweak potentials for all co-annihilation channels of wino dark matter at the one-loop order and obtain the wino relic abundance including the Sommerfeld effect at the next-to-leading order (NLO).
48 pages, LaTeX
References in corpus (9)
- A Theory of Dark Matter
- Cosmology and Astrophysics of Minimal Dark Matter
- Non-perturbative Effect on Thermal Relic Abundance of Dark Matter
- Relic densities including Sommerfeld enhancements in the MSSM
- Heavy Dark Matter Annihilation from Effective Field Theory
- Prospects for dark matter searches in the pMSSM
- Prospects for Heavy WIMP Dark Matter with CTA: the Wino and Higgsino
- Soft Collinear Effective Theory for Heavy WIMP Annihilation
- The last refuge of mixed wino-Higgsino dark matter
Cited by in corpus (11)
- New physics explanations of in light of the FNAL muon measurement
- Non-Abelian Electric Field Correlator at NLO for Dark Matter Relic Abundance and Quarkonium Transport
- Non-relativistic and potential non-relativistic effective field theories for scalar mediators
- Matching resummed endpoint and continuum -ray spectra from dark-matter annihilation
- Sommerfeld-enhanced dark matter searches with dwarf spheroidal galaxies
- The Muon Magnetic Moment and Physics Beyond the Standard Model
- The hMSSM with a Light Gaugino/Higgsino Sector: Implications for Collider and Astroparticle Physics
- Neutrino forces and the Sommerfeld enhancement
- Minimal Nambu-Goldstone Higgs Model in Supersymmetric SU(5) Revisited
- NLO electroweak potentials for minimal dark matter and beyond
- Gamma-ray line from electroweakly interacting non-abelian spin-1 dark matter