'Muon energy' presentation slideshows

What we do know about cosmic rays at energies above 10 15 eV?

4 th Round Table, December 16 - 17, 2011. What we do know about cosmic rays at energies above 10 15 eV?. A.A.Petrukhin. National Research Nuclear University MEPhI, Russia. Contents. 1. Introduction. 2. How these CR are investigated. 3. Results and questions.

558 views • 49 slides

On the behalf of the ACORDE Collaboration

ACORDE and Cosmic Rays Physics at LHC S. Kartal University of Istanbul -Turkey C.E. Pagliarone Univeristy of Cassino & INFN Pisa. On the behalf of the ACORDE Collaboration. Outline. Motivations ACORDE (the A LICE CO smic R ays D etector) Physics Goals

595 views • 46 slides

QE kinematics

QE kinematics. 1. Introduction 2. MiniBooNE pahse space study 3. T2K phase space study 4. Conclusion. Teppei Katori Queen Mary University of London Valencia Neutrino Interaction T2K meeting ( V ANISh ) University of Valencia, Valencia, Spain, Apr. 3, 2014. 1. Introduction

456 views • 37 slides

Muon-induced neutrons: how deep should we go to get rid of them?

Muon-induced neutrons: how deep should we go to get rid of them?. V. A. Kudryavtsev. Department of Physics and Astronomy University of Sheffield. Outline. Introduction: what are muon-induced neutrons and why are they dangerous for sensitive experiments? Simulations of muons.

408 views • 33 slides

Physics Laboratory

Physics Laboratory. School of Science and Technology. Hellenic Open University. HOU contribution to KM3NeT TDR (WP2). A. G. Tsirigotis. EESFYE - Demokritos , 22 May 200 9. In the framework of the KM3NeT Design Study. The HOU software chain. Underwater Neutrino Detector

320 views • 31 slides

Overview

Overview. Astrophysical Neutrinos & Searching for a Diffuse Flux of Muon Neutrinos Muon Energy Estimation 22 String Diffuse Analysis Results Outlook for 40 Strings Questions & Discussion. Neutrinos as Cosmic Messengers. Neutrinos help answer many questions in astrophysics:.

443 views • 29 slides

Physics Laboratory

Physics Laboratory. School of Science and Technology. Hellenic Open University. Progress report of the HOU contribution to TDR (WP2). A. G. Tsirigotis. WP2 - Demokritos , 31 March 200 9. In the framework of the KM3NeT Design Study. The HOU software chain. Underwater Detector

351 views • 27 slides

Physics Laboratory

Physics Laboratory. School of Science and Technology. Hellenic Open University. Progress report of the HOU contribution to TDR (WP2). A. G. Tsirigotis. WP2 - Demokritos , 31 March 200 9. In the framework of the KM3NeT Design Study. The HOU software chain. Underwater Detector

283 views • 27 slides

Muon Energy reconstruction in IceCube and neutrino flux measurement

Muon Energy reconstruction in IceCube and neutrino flux measurement. Dmitry Chirkin, University of Wisconsin at Madison, U.S.A., MANTS meeting, fall 2009. Muon Energy reconstruction in IceCube. parameterization of light pattern created by a muon fitting of event data to this light pattern

364 views • 23 slides

Muon Energy reconstruction in IceCube and neutrino flux measurement

Muon Energy reconstruction in IceCube and neutrino flux measurement. Dmitry Chirkin, University of Wisconsin at Madison, U.S.A., MANTS meeting, fall 2009. Muon Energy reconstruction in IceCube. parameterization of light pattern created by a muon fitting of event data to this light pattern

233 views • 23 slides

SCIPP Summer Outreach Project

SCIPP Summer Outreach Project. July 2005. Topics. Cosmic Ray Detectors Detector Testing Muon Lifetime Experiment Count Rate Analysis Exponential Decay. Cosmic Ray Detectors. CCRT from SLAC BERKELEY from LBNL WALTA from FNAL New Power Supply and Housing Detector Testing

336 views • 22 slides

M. Spurio, G. Carminati, A. Margiotta University of Bologna and INFN

MU ons from PA rametric formulas: a fast Ge nerator of atmospheric m for neutrino telescopes ( MUPAGE ). M. Spurio, G. Carminati, A. Margiotta University of Bologna and INFN. VLVnT08 - Toulon 22-24 April 2008. Atmospheric muons in a VLV n T.

424 views • 21 slides

Physics Laboratory

Physics Laboratory. School of Science and Technology. Hellenic Open University. HOU Reconstruction & Simulation (HOURS): A complete simulation and reconstruction package for Very Large Volume underwater neutrino Telescopes. A.Leisos, A. G. Tsirigotis , S.E.Tzamarias.

366 views • 20 slides

Search for L epton F lavor V iolation in the m + N -> t + N conversion (preliminary)

Search for L epton F lavor V iolation in the m + N -> t + N conversion (preliminary). S.N. Gninenko INR, Moscow. SPSC meeting, Villars, September 22-28, 2004. Outline. Introduction m +N-> t +N conversion Choice of signature Experimental setup

265 views • 20 slides

PERFORMANCE OF THE MACRO LIMITED STREAMER TUBES IN DRIFT MODE FOR MEASUREMENTS OF MUON ENERGY

7 International Conference on. th. ADVANCED TECHNOLOGY AND PARTICLE PHYSICS. Villa Olmo, Como, 15-19/10/2001. PERFORMANCE OF THE MACRO LIMITED STREAMER TUBES IN DRIFT MODE FOR MEASUREMENTS OF MUON ENERGY. M. Giorgini for the MACRO Collaboration.

339 views • 19 slides

Energy Reconstruction Algorithms for the ANTARES Neutrino Telescope

366 views • 18 slides

Physics Laboratory

238 views • 16 slides

Search for exotic contributions to Atmospheric Neutrino Oscillations

259 views • 16 slides

Determination of muon hit position for the KIMS experiment

Determination of muon hit position for the KIMS experiment. JingJun Zhu. Tsinghua University &. KIMS collaboration. 2003 Oct. 24th KPS meeting. KIMS experiment.

383 views • 15 slides

Muon induced electromagnetic shower reconstruction in the ANTARES neutrino telescope

ICRC2011, 32ND INTERNATIONAL COSMIC RAY CONFERENCE, BEIJING 2011. Muon induced electromagnetic shower reconstruction in the ANTARES neutrino telescope.

91 views • 1 slides