Enhancing dark matter annihilation rates with dark bremsstrahlung

Nicole F. Bell, Yi Cai, James B. Dent, Rebecca K. Leane, and Thomas J. Weiler
Phys. Rev. D 96, 023011 – Published 26 July 2017

Abstract

Many dark matter interaction types lead to annihilation processes which suffer from p-wave suppression or helicity suppression, rendering them subdominant to unsuppressed s-wave processes. We demonstrate that the natural inclusion of dark initial state radiation can open an unsuppressed s-wave annihilation channel and, thus, provide the dominant dark matter annihilation process for particular interaction types. We illustrate this effect with the bremsstrahlung of a dark spin-0 or dark spin-1 particle from fermionic dark matter, χ¯χf¯fϕ or f¯fZ. The dark initial state radiation process, despite having a 3-body final state, proceeds at the same order in the new physics scale Λ as the annihilation to the 2-body final state χ¯χf¯f. This opens an unsuppressed s wave at lower order in Λ than the well-studied lifting of helicity suppression via Standard Model final state radiation or virtual internal bremsstrahlung. This dark bremsstrahlung process should influence LHC and indirect detection searches for dark matter.

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  • Received 22 May 2017

DOI:https://doi.org/10.1103/PhysRevD.96.023011

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Nicole F. Bell1,*, Yi Cai1,†, James B. Dent2,‡, Rebecca K. Leane1,§, and Thomas J. Weiler3,∥

  • 1ARC Centre of Excellence for Particle Physics at the Terascale School of Physics, The University of Melbourne, Victoria 3010, Australia
  • 2Department of Physics, University of Louisiana at Lafayette, Lafayette, Louisiana 70504-4210, USA
  • 3Department of Physics and Astronomy, Vanderbilt University, Nashville, Tennessee 37235, USA

  • *n.bell@unimelb.edu.au
  • yi.cai@unimelb.edu.au
  • jbdent@louisiana.edu
  • §rebecca.leane@gmail.com
  • tom.weiler@vanderbilt.edu

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Issue

Vol. 96, Iss. 2 — 15 July 2017

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