Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

AUGER COLLABORATION, B. WUNDHEILER

PHYSICAL REVIEW D - PARTICLE AND FILDS

AMER PHYSICAL SOC

Año: 2009 p. 1020011 - 10200115

0556-2821

Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse flux of tau neutrinos in the cosmic radiation. Earth-skimming nu_tau may interact in the Earth’s crust and produce a tau lepton by means of charged-current interactions. The tau lepton may emerge from the Earth and decay in theatmosphere to produce a nearly horizontal shower with a typical signature, a persistent electromagnetic component even at very large atmospheric depths. The search procedure to select events induced by tau decays against the background of normal showers induced by cosmic rays is described. The method used to compute the exposure for a detector continuously growing with time is detailed. Systematic un-certainties in the exposure from the detector, the analysis, and the involved physics are discussed. No tau neutrino candidates have been found. For neutrinos in the energy range 2x10^17 eV < E_nu < 2x10^19 eV, assuming a diffuse spectrum of the form E_nu^-2 , data collected between 1 January 2004 and 30 April 2008 yield a 90% confidence-level upper limit of E_nu^-2 dN_nu_tau/dE_nu < 9x10^-8 GeVcm^-2 s^-1sr^-1.