https://doi.org/10.1140/epjc/s10052-024-12660-6
Regular Article - Theoretical Physics
Precision predictions for dark matter with DM@NLO in the MSSM
1
PRISMA+ Cluster of Excellence and Mainz Institute for Theoretical Physics, FB 08 - Physics, Mathematics and Computer Science, Johannes Gutenberg University Mainz, 55099, Mainz, Germany
2
LAPTh, Université Savoie Mont Blanc, CNRS, 74000, Annecy, France
3
Institut für Theoretische Physik, Universität Münster, Wilhelm-Klemm-Straße 9, 48149, Münster, Germany
e
luca.wiggering@uni-muenster.de
Received:
12
January
2024
Accepted:
10
March
2024
Published online:
1
April
2024
We present DM@NLO, a Fortran 77 based program with a C++ interface dedicated to precision calculations of dark matter (DM) (co)annihilation cross-sections and elastic dark matter-nucleon scattering amplitudes in the minimal supersymmetric (SUSY) Standard Model (MSSM) at next-to-leading order (NLO) in perturbative (SUSY) QCD. If the annihilating initial particles carry an electric or colour charge, the Sommerfeld enhanced cross section is included as well and can be matched to the NLO cross section. We review these calculations including technical details relevant for using the code. We illustrate their impact by applying DM@NLO to an example scenario in the constrained MSSM.
© The Author(s) 2024
Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
Funded by SCOAP3.