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Atmospheric lepton fluxes at ultrahigh energies

Journal Article · · Journal of Cosmology and Astroparticle Physics
;  [1];  [2]
  1. CAFPE and Depto. de Física Teórica y del Cosmos, Universidad de Granada, 18071 Granada (Spain)
  2. INFN and Dipartimento di Fisica, Università di Roma Tre, 00146 Rome (Italy)
In order to estimate the possibility to observe exotic physics in a neutrino telescope, it is essential to first understand the flux of atmospheric neutrinos, muons and dimuons. We study the production of these leptons by high-energy cosmic rays. We identify three main sources of muons of energy E ≥ 10{sup 6} GeV: the weak decay of charm and bottom mesons and the electromagnetic decay of unflavored mesons. Contrary to the standard assumption, we find that η mesons, not the prompt decay of charm hadrons, are the dominant source of atmospheric muons at these energies. We show that, as a consequence, the ratio between the neutrino and muon fluxes is significantly reduced. For dimuons, which may be a background for long-lived staus produced near a neutrino telescope, we find that pairs of E ≈ 10{sup 7} GeV forming an angle above 10{sup −6} rad are produced through D (80%) or B (10%) meson decay and through Drell-Yan proceses (10%). The frequency of all these processes has been evaluated using the jet code PYTHIA.
OSTI ID:
22273253
Journal Information:
Journal of Cosmology and Astroparticle Physics, Journal Name: Journal of Cosmology and Astroparticle Physics Journal Issue: 09 Vol. 2009; ISSN 1475-7516
Country of Publication:
United States
Language:
English