Probing Very High Energy Prompt Muon and Neutrino fluxes and the cosmic ray knee via Underground Muons

Abstract

We calculate event rate and demonstrate the observational feasibility of very high energy muons (1-1000 TeV) in a large mass underground detector operating as a pair-meter. This energy range corresponds to surface muon energies of $\sim$(5 TeV - 5000 TeV) and primary cosmic ray energies of $\sim$ (50 TeV - 5 $\times 10^4$ TeV). Such measurements would significantly assist in an improved understanding of the prompt contribution to ${\nu }_e,{\nu }_{\mu }$ and $\mu$ fluxes in present and future ultra-high energy neutrino detectors. In addition, they would shed light on the origin of the observed 'knee' in the cosmic ray spectrum.

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References in corpus (24)

• Origin and Propagation of Extremely High Energy Cosmic Rays
• Ultrahigh-Energy Neutrino Interactions
• Neutrino Interactions at Ultrahigh Energies
• Particle Physics with High Energy Neutrinos
• High-energy Neutrino Astronomy: The Cosmic Ray Connection
• Energy determination in the Akeno Giant Air Shower Array experiment
• Detection and imaging of atmospheric radio flashes from cosmic ray air showers
• Measurement of the Flux of Ultrahigh Energy Cosmic Rays from Monocular Observations by the High Resolution Fly's Eye Experiment
• Atmospheric Muon Flux at Sea Level, Underground, and Underwater
• Charm Production and High Energy Atmospheric Muon and Neutrino Fluxes
• Lepton Fluxes from Atmospheric Charm
• The primary cosmic ray composition between 10**15 and 10**16 eV from Extensive Air Showers electromagnetic and TeV muon data
• Photonuclear interaction of high energy muons and tau-leptons
• Shower Power: Isolating the Prompt Atmospheric Neutrino Flux Using Electron Neutrinos
• Cosmic Rays and Large Extra Dimensions
• On the shape of the UHE cosmic ray spectrum
• Ultra-High Energy Neutrinos: A Review of Theoretical and Phenomenological Issues
• Prompt atmospheric neutrinos and muons: dependence on the gluon distribution function
• Prompt atmospheric neutrinos and muons: NLO vs LO QCD predictions
• Upper Limit on the Prompt Muon Flux Derived from the LVD Underground Experiment
• Prompt muon contribution to the flux underwater
• Measuring the prompt atmospheric neutrino flux with down-going muons in neutrino telescopes
• Rigidity dependent knee and cosmic ray induced high energy neutrino fluxes
• Ultra High Energy Neutrino Astronomy

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• IC at IC: IceCube can constrain the intrinsic charm of the proton
• Cross sections and energy loss for lepton pair production in muon transport
• A method for detection of muon induced electromagnetic showers with the ANTARES detector