English

The One-Loop Correction to Heavy Dark Matter Annihilation

High Energy Physics - Phenomenology 2019-10-25 v2 Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena

Abstract

We calculate the one-loop corrections to TeV scale dark matter annihilation in a model where the dark matter is described by an SU(2)L_L triplet of Majorana fermions, such as the wino. We use this framework to determine the high and low-scale MS-bar matching coefficients at both the dark matter and weak boson mass scales at one loop. Part of this calculation has previously been performed in the literature numerically; we find our analytic result differs from the earlier work and discuss potential origins of this disagreement. Our result is used to extend the dark matter annihilation rate to NLL' (NLL+O(α2\alpha_2) corrections) which enables a precise determination of indirect detection signatures in present and upcoming experiments.

Keywords

Cite

@article{arxiv.1612.04814,
  title  = {The One-Loop Correction to Heavy Dark Matter Annihilation},
  author = {Grigory Ovanesyan and Nicholas L. Rodd and Tracy R. Slatyer and Iain W. Stewart},
  journal= {arXiv preprint arXiv:1612.04814},
  year   = {2019}
}

Comments

27 pages, 5 figures. Corrected counter-term contributions, fixing an issue first noted in 1805.07367. Impact on final results in plots is imperceptible, leaving the conclusions and numerical analysis unchanged

R2 v1 2026-06-22T17:24:02.610Z