Neutrinos and Ultra-High Energy Cosmic Rays. Dmitry Semikoz MPI, Munich & INR, Moscow in collaboration with F.Aharonian, O.Kalashev, V.Kuzmin, A.Neronov and G.Sigl. Overview:. Introduction Experimental detection of high energy neutrinos: Under/ground/water/ice Horizontal air showersBy tayte
<Xmax> measurements by fluorescence experiments. GZK-40. INR, Moscow. May 17, 2006. Konstantin Belov High Resolution Fly’s Eye (HiRes) Collaboration. Columbia University University of Adelaide University of New Mexico Rutgers University University of MontanaBy zorion
The cosmic-ray spectrum. From the knee to the ankle. Spectrometers ( D A = 1 resolution, good E resolution). Air showers. Calorimeters (less good resolution). Air-shower arrays on the ground to overcome low flux. Don’t see primaries directly. Direct measurements. Knee. Ankle.By chet
Tunka Experiment: Towards 1км 2 EAS Cherenkov Array at the Tunka Valley. N.Budnev 2 , D.Chernov 1 , O.Gress 2 , N.Kalmykov 1 , Е. Korosteleva 1 , V.Kozhin 1, L.Kuzmichev 1 , B.Lubsandorzhiev 3 , G.Navarra 5 ,By artie
Status of LHCf. Alessia Tricomi University of catania & INFN catania on behalf of the LHCf collaboration. Forward photon energy spectrum at √s = 7 TeV p-P collisions Prospects for new analyses Detector upgrade. CSN1 Napoli, July 5, 2011. Physics motivations.By dorian-freeman
Ashra Report: VHE Neutrino Detection. Koji Noda (ICRR, Univ. of Tokyo) for Ashra-1 collaboration DPF2006 Oct 31, 2006. Overview. Earth-skimming n t MC simulation Detector status Summary. 1. Earth-skimming n t. VHE neutrino candidates: AGN,GRB,GZK,,, Why Earth-skimming n t ?By mariamatthews
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