Searching for heavy millicharged particles from the atmosphere
If millicharged particles (MCPs) exist they can be created in the atmosphere when high energy cosmic rays collide with nuclei and could subsequently be detected at neutrino experiments. We extend previous work, which considered MCPs from decays of light mesons and proton bremsstrahlung, by including production from <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mi mathvariant="normal">ϒ</a:mi></a:math> meson decays and the Drell-Yan process. MCPs with masses below a GeV primarily arise from proton bremsstrahlung, while heavier MCPs predominantly originate from heavy meson decays and Drell-Yan. We analyze the resulting single scatter and multiple scatter signals at SuperK and JUNO. Searches for low energy coincident signals at JUNO will be sensitive to MCPs with millicharges up to an order of magnitude beyond current constraints for MCP masses between 2 and 10 GeV. Published by the American Physical Society 2024
Authors
- Ningqiang Song (ORCID: https://orcid.org/0000-0002-3590-2341)
- Edward P. Hardy
- Han Wu
Institutions
- University of Liverpool (GB)
- Queen's University (CA)
- University of Oxford (GB)
- Arthur B. McDonald-Canadian Astroparticle Physics Research Institute (CA)
- Institute of Theoretical Physics (CN)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2024-12-30
- DOI
- https://doi.org/10.1103/physrevd.110.115037
- Citations
- 6
- Primary Topic
- Astrophysics and Cosmic Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 3.96
Funders
- UK Research and Innovation
- Canada Foundation for Innovation
- National Natural Science Foundation of China
- Science and Technology Facilities Council