'Pion production' diaporamas de présentation

Gamma-Rays, Cosmic Rays And Neutrinos. Introduction to the observational situation Introduction to the propagation of cosmic rays and electromagnetic cascades Applications to diffuse and point source fluxes of gamma-rays and neutrinos

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Modelling neutrino cross sections

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Jonathan Link Columbia University Fermilab Wine & Cheese November 18 th 2005

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What can we learn from the GZK feature?

What can we learn from the GZK feature?. Angela V. Olinto Astronomy & Astrophysics Kavli Institute Cosmol.Phys. Enrico Fermi Institute University of Chicago. Huge Amounts!. If the GZK feature is accurately measured... we can learn the 1. composition of the primaries

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Propagation of ultra-high energy cosmic rays in the Universe

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Photohadronic processes and neutrinos

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The High-Power Target Experiment

The High-Power Target Experiment . MUTAC Meeting BNL April 28, 2004. Neutrino Factory Targetry Concept. Capture low P T pions in a high-field solenoid Use Hg jet tilted with respect to solenoid axis Use Hg pool as beam dump.

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SciBooNE, A Neutrino Cross Section Measurement Experiment at Fermilab

SciBooNE, A Neutrino Cross Section Measurement Experiment at Fermilab. 1. Motivation 2. SciBooNE detector 3. Cross section measurements 4. Conclusion. Teppei Katori for the SciBooNE collaboration Massachusetts Institute of Technology

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H A R P A Hadron Production Experiment at the Proton Synchrotron at CERN

H A R P A Hadron Production Experiment at the Proton Synchrotron at CERN. Motivation for the HARP experiment The HARP Detector MiniBooNE and HARP. HARP Motivation (general). Measure absolute inclusive cross-sections for Hadron production with a range of

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Ultra-High Energy Neutrino Fluxes

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Angular Distribution of Gamma-rays from Up-to-date p-p Interactions

Angular Distribution of Gamma-rays from Up-to-date p-p Interactions. GLAST Science Lunch Talk Aug 3, 2006 Niklas Karlsson SLAC / KTH niklas@slac.stanford.edu. Outline. Recap p-p interaction model parameterization of gamma-ray spectra Angular distribution of gamma-rays - simulations

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Low Energy Muon Cooling : Frictional Cooling

Low Energy Muon Cooling : Frictional Cooling. Studies at Columbia University &Nevis Labs Raphael Galea Allen Caldwell Stefan Schlenstedt (DESY/Zeuten) Halina Abramowitz(Tel Aviv University). Summer Students: Christos Georgiou Daniel Greenwald Yujin Ning Inna Shpiro Will Serber.

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New developments in FLUKA

New developments in FLUKA. Paola Sala INFN Milano On behalf of the FLUKA collaboration ? 50 members from several institutions around the world Varenna , June 14 th 2012. http ://www.fluka.org. A glimpse of latest developments and applications.

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Extra Spectral Components due to Hadronic Cascade

Extra Spectral Components due to Hadronic Cascade. Katsuaki Asano (Tokyo Inst. Tech.). Collaboration with S.Inoue, P.Meszaros K.Murase, T.Terasawa. GRB 090510; Spectra. Band+ Extra PL. Extra Component in 090902B. Models.

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Analytic/Numerical Beam Simulation Model_B

Analytic/Numerical Beam Simulation Model_B. Beam simulation that incorporates the main characteristics of the beam using numerical and analytic methods Main motivation is to have a beam tool that is easily understood and can be used to compare to and validate the GEANT3 and GEANT4 simulations

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Polarized p-A and Inclusive Lambda Polarization experiments at the AGS

Polarized p-A and Inclusive Lambda Polarization experiments at the AGS. Yousef I. Makdisi Brookhaven National Laboratory. Outline. Asymmetry in Inclusive Pion Production at the AGS Issues with intended production from a carbon target The experimental set up and results

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Pion Production / Capture

Pion Production / Capture. M. Yoshida (Osaka Univ.) COMET/Mu2e Joint Workshop Jan. 23, 2009, LBNL. Pions at Target. Forward. MARS simulation Count pions at target surface Compare momentum distribution for Tungsten, Gold, Copper and Graphite Heavy material has softer distributions.

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MARS vs HARP

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