Year: 2025
Type: article
Abstract: A bstract Long-range attractive interactions between dark matter particles can significantly enhance their annihilation, particularly at low velocities. This “Sommerfeld enhancement” is typically computed by evaluating the deformation of the two-particle wavefunction due to the long-range potential, while ignoring the physics associated with the annihilation, and then scaling the appropriate annihilation matrix elements by factors that depend on the wavefunction in the limit where the particles approach zero relative separation. It has long been recognized that this approach is a valid approximation only in the limit where the annihilation rate is small, and breaks down in the regime where the enhanced annihilation rate approaches the unitarity bound, in which case ignoring the impact of the annihilation physics on the two-particle wavefunction cannot be justified and leads to apparent violations of unitarity. In the case where the physics relevant to annihilation occurs at a parametrically shorter distance scale (higher energy scale) compared with the long-range potential, we provide a simple prescription for correcting the Sommerfeld enhancement for the effects of the short-range physics, valid for all partial waves and for systems where multiple states are coupled by the long-range potential.
Source: Journal of High Energy Physics
Authors: Aditya Parikh, Ryosuke Sato, Tracy R. Slatyer
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: diamond
Funders: National Science Foundation, U.S. Department of Energy, Simons Foundation, Aspen Center for Physics, Office of Science, Department of Physics, Harvard University, Japan Society for the Promotion of Science, Mainz Institute for Theoretical Physics, Johannes Gutenberg University Mainz, Kavli Institute for Theoretical Physics, University of California, Santa Barbara, High Energy Physics
Awards: G1006625179, G2539474701, G2595738051, G2695919875, THEORETICAL HIGH ENERGY PHYSICS, G3398237449, G3895747351, Theoretical Physics, G4360986921, G4437173897, G4689434848, Dynamics of Axion in the Early Universe, G5825571352, THEORETICAL HIGH ENERGY PHYSICS, G638484911, G6794394390, Kavli Institute for Theoretical Physics, Programs on Critical Problems in Physics, Astrophysics and Biophysics at the Aspen Center for Physics, G97843138
OpenAlex ID: W4416960068
