Published September 4, 2024 | Version v1
Journal article Open

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.

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10.1103_PhysRevD.110.063006.pdf

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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

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