학술논문

Linear Sigma Dark Matter
Document Type
Working Paper
Source
JHEP09(2022)041
Subject
High Energy Physics - Phenomenology
Astrophysics - Cosmology and Nongalactic Astrophysics
Language
Abstract
We present a model of self-interacting dark matter based on QCD-like theories and inspired by the proximity of $a_0(980\pm 20)$ to the $K\bar{K}(990)$ threshold. Dark matter is comprised of dark pions which self-scatter via the $\sigma$ resonance close to the $\pi\pi$ threshold. While the linear sigma model serves as a qualitative guide, a fully unitary description of the scattering in the strongly coupled regime is given by effective range theory. The introduction of a kinetically mixed dark photon allows the dark pion to either freeze-out or -in. We study the viable parameter space which explains the observed relic abundance while evading all current constraints. Searches for dark matter self interactions at different scales, (in)direct detection signals, and (in)visibly-decaying dark photons will test this model in the near future.
Comment: 30 pages, 13 figures; v2: minor revisions to match published version