Cosmic ray muons in laboratories deep underground
- 1. University of Alberta, Department of Physics, 4-181 CCIS, 116 St. and 85 Ave., Edmonton, AB T6G 2R3, Canada
- 2. Institute of Physics, Academia Sinica, Taipei City, 11529, Taiwan
- 3. University of Alberta, Department of Physics 4-181 CCIS, 116 St. and 85 Ave., Edmonton, AB T6G 2R3, Canada
Description
We provide comprehensive calculations of total muon fluxes, energy and angular spectra, and mean muon energies in deep underground laboratories—under flat overburdens and mountains and underwater—using our latest calculation code, mute v3. For precise modeling, we compiled rock densities and chemical compositions for various underground labs, as well as topographic map profiles of overburdens, and integrated them into our calculations. Our results show excellent agreement with available data for most underground sites when using the latest surface muon flux model, daemonflux. Moreover, since our calculations do not rely on underground measurements of muons or other secondaries, we can verify the consistency of measurements across different detectors at different sites. mute is an open-source, publicly available program, providing a solid framework for accurate muon flux predictions in various underground environments, essential for applications in cosmic ray physics and dark matter searches.
Files
10.1103_PhysRevD.110.063006.pdf
Files
(1.6 MB)
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Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.110.063006;
- arXiv
- arXiv:2406.10339;
- Crossref Funder ID
- 10.13039/501100010785; 10.13039/501100021202;
Publishing Information
- Journal Title
- Physical Review D
- Journal Volume
- 110
- Journal Issue
- 6
- Journal Page Range
- 18 pgs.
- ISSN
- 1089-4918
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S97: MATHEMATICAL METHODS AND COMPUTING;
- Descriptors DEI
- CHEMICAL COMPOSITION; COMPUTERIZED SIMULATION; COSMIC MUONS; COSMIC NUCLEI; COSMIC RAY DETECTION; COSMIC RAY FLUX; DENSITY; FLUX DENSITY; FORECASTING; MAPS; NONLUMINOUS MATTER; OVERBURDEN; ROCKS; SIMULATION; SOLIDS; UNDERGROUND
- Descriptors DEC
- COSMIC RADIATION; DETECTION; ELEMENTARY PARTICLES; FERMIONS; IONIZING RADIATIONS; LEPTONS; LEVELS; MATTER; MUONS; NUCLEI; PHYSICAL PROPERTIES; PRIMARY COSMIC RADIATION; RADIATION DETECTION; RADIATION FLUX; RADIATIONS; SECONDARY COSMIC RADIATION; SIMULATION
Optional Information
- Contract/Grant/Project number
- AS-CFII-112-103
- Notes
- Contact Email: Contact author: wwoodley@ualberta.ca; Contact Email: Contact author: anatoli@gate.sinica.edu.tw; Contact Email: Contact author: mariecci@ualberta.ca; Record automatically processed
- Funding organization
- Canada First Research Excellence Fund; Alliance de recherche numérique du Canada; Arthur B. McDonald Canadian Astroparticle Physics Research Institute; Academia Sinica Grid-Computing Center