Heavy Dark Matter Annihilation from Effective Field Theory
arXiv:1409.8294 · doi:10.1103/PhysRevLett.114.211302
Abstract
We formulate an effective field theory description for SU(2) triplet fermionic dark matter by combining nonrelativistic dark matter with gauge bosons in the soft-collinear effective theory. For a given dark matter mass, the annihilation cross section to line photons is obtained with 5% precision by simultaneously including Sommerfeld enhancement and the resummation of electroweak Sudakov logarithms at next-to-next-to-leading logarithmic order. Using these results, we present more accurate and precise predictions for the gamma-ray line signal from annihilation, updating both existing constraints and the reach of future experiments.
5 pages, 2 figures
References in corpus (7)
- A Theory of Dark Matter
- Cosmology and Astrophysics of Minimal Dark Matter
- Drell-Yan production at small q_T, transverse parton distributions and the collinear anomaly
- The Zero-Bin and Mode Factorization in Quantum Field Theory
- Search for photon line-like signatures from Dark Matter annihilations with H.E.S.S
- Wino-like Minimal Dark Matter and future colliders
- Soft Collinear Effective Theory for Heavy WIMP Annihilation
Cited by in corpus (10)
- WIMPs at the Galactic Center
- Soft Collinear Effective Theory for Heavy WIMP Annihilation
- Dark Matter in lines: Galactic Center vs dwarf galaxies
- Shining Primordial Black Holes
- QCD Effects on Direct Detection of Wino Dark Matter
- The Sommerfeld Enhancement in the Scotogenic Model with Large Electroweak Scalar Multiplets
- Coupling Unification and Dark Matter in a Standard Model Extension with Adjoint Majorana Fermions
- Non-relativistic pair annihilation of nearly mass degenerate neutralinos and charginos III. Computation of the Sommerfeld enhancements
- NLO electroweak potentials for minimal dark matter and beyond
- Gamma-ray line from electroweakly interacting non-abelian spin-1 dark matter