'10 17 ev' presentation slideshows

10 17 ev - PowerPoint PPT Presentation


Neutrinos and Ultra-High Energy Cosmic Rays

Neutrinos and Ultra-High Energy Cosmic Rays

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 showers

By tayte
(160 views)

Konstantin Belov High Resolution Fly’s Eye (HiRes) Collaboration

Konstantin Belov High Resolution Fly’s Eye (HiRes) Collaboration

<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 Montana

By zorion
(82 views)

The cosmic-ray spectrum

The cosmic-ray spectrum

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
(130 views)

Tunka Experiment: Towards 1км 2 EAS Cherenkov Array at the Tunka Valley

Tunka Experiment: Towards 1км 2 EAS Cherenkov Array at the Tunka Valley

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
(114 views)

Status of LHCf

Status of LHCf

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
(116 views)

Ashra Report: VHE Neutrino Detection

Ashra Report: VHE Neutrino Detection

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
(0 views)


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