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Cosmic Ray Muons in Laboratories Deep Underground

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arxiv 2406.10339 v2 pith:BP7WHSKQ submitted 2024-06-14 hep-ph

classification hep-ph
keywords undergroundmuoncalculationsavailablecosmicdeepdifferentflux
verification ladder T0 review T1 audit T2 compute T3 formal
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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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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Characterisation of the Bedretto Underground Site for Fundamental Physics Experiments

    astro-ph.IM 2025-12 conditional novelty 6.0 of 10

    The Bedretto tunnel's ~4000 m.w.e. depth, low muon flux, and very low seismic/magnetic noise make it a strong candidate for a European deep-underground physics laboratory.

  2. A New Method for Measuring the Pion-Air Cross Section at Multi-TeV Energies Using Muon Bundle Properties in Deep Underground Detectors

    astro-ph.HE 2025-07 conditional novelty 5.0 of 10

    Simulations show that underground muon bundle counts could constrain the inelastic pion-air cross section to roughly 10-15% near 1-2 TeV.

  3. Mineral Detection of Neutrinos and Dark Matter 2025 Proceedings

    physics.ins-det 2025-08 unverdicted novelty 4.0 of 10

    A workshop proceedings presenting 20 status reports on mineral detectors as passive, long-exposure nuclear recoil detectors for dark matter, neutrinos, and cosmic rays.

  4. Community Report from the 2025 SNOLAB Future Projects Workshop

    hep-ex 2025-07 unverdicted novelty 1.0 of 10

    A community report summarizes proposed future experiments and infrastructure needs for SNOLAB over the next 15 years.

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