Wino dark matter annihilation through the radiative formation of bound states

TL;DR

This paper develops a zero-range effective field theory to analyze wino dark matter annihilation, especially near critical masses where Sommerfeld enhancements and bound state formations significantly increase annihilation rates.

Contribution

It introduces a zero-range effective field theory framework to describe wino interactions and calculates bound state formation rates via radiative processes.

Findings

Zero-range EFT accurately models near-threshold wino interactions.

Bound state formation rates are computed through soft photon emission.

Enhanced annihilation rates are linked to resonance conditions.

Abstract

The most dramatic "Sommerfeld enhancements" of neutral-wino-pair annihilation occur when the wino mass is tuned to near critical values where there is a zero-energy S-wave resonance at the neutral-wino-pair threshold. If the wino mass is larger than the critical value, the resonance is a wino-pair bound state. If the wino mass is near a critical value, low-energy winos can be described by a zero-range effective field theory in which the winos interact nonperturbatively through a contact interaction. The parameters of the zero-range effective field theory can be determined by matching wino scattering amplitudes calculated by solving the Schr\"odinger equation for a nonrelativistic effective field theory in which the winos interact through a potential due to the exchange of electroweak gauge bosons. The utility of the zero-range effective field theory is illustrated by calculating the rate for formation of an S-wave bound state in the collision of two neutral winos through the emission of two soft photons.