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Spectrum of cosmic-ray nucleons and the atmospheric muon charge ratio

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arxiv 1111.6675 v2 pith:L6RZXDP7 submitted 2011-11-29 astro-ph.HE hep-ph

classification astro-ph.HEhep-ph
keywords spectrachargemeasurementsratioatmospherecosmic-raymuonneutrons
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Interpretation of measurements of the muon charge ratio in the TeV range depends on the spectra of protons and neutrons in the primary cosmic radiation and on the inclusive cross sections for production of $\pi^\pm$ and $K^\pm$ in the atmosphere. Recent measurements of the spectra of cosmic-ray nuclei are used here to estimate separately the energy spectra of protons and neutrons and hence to calculate the charge separated hadronic cascade in the atmosphere. From the corresponding production spectra of $\mu^+$ and $\mu^-$ the $\mu^+/\mu^-$ ratio is calculated and compared to recent measurements. The comparison leads to a determination of the relative contribution of kaons and pions. Implications for the spectra of $\nu_\mu$ and $\bar{\nu}_\mu$ are discussed.

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Cited by 3 Pith papers

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

  1. Using Cosmic Rays to Predict the Weather: Meteorological Data Assimilation of Atmospheric Muon Flux Data

    physics.ao-ph 2025-09 conditional novelty 7.0 of 10

    Simulated cosmic-ray muon counts, assimilated into an ensemble weather model, improve short-range forecasts of a tropical cyclone beyond what a single surface pressure measurement provides.

  2. Ultra-High-Energy Cosmic Ray Boosted Relic Neutrinos

    hep-ph 2026-06 unverdicted novelty 6.0 of 10

    Computes the diffuse UHECR-boosted CνB flux across elastic, coherent, incoherent, resonance, and deep-inelastic channels with mixed-composition UHECR models and derives upper limits on CνB overdensity from IceCube and...

  3. Beyond standard model particles in the atmospheric flux: a long-lived stau example

    hep-ph 2025-07 conditional novelty 5.0 of 10

    Atmospheric stau production from squark decays is computed with Z-moments; predicted IceCube-Gen2 event rates are tiny and LHC bounds are more restrictive.

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