'Pion production' presentation slideshows

Pion production - PowerPoint PPT Presentation


Low Energy Muon Cooling : Frictional Cooling

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.

By martha
(204 views)

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

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

By leyna
(180 views)

What can we learn from the GZK feature?

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

By adem
(101 views)

The High-Power Target Experiment

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.

By sage
(115 views)

MARS vs HARP

MARS vs HARP

Goran Skoro . MARS vs HARP. GOAL (general): Comparison between experimental data and Monte Carlo calculations on pion production in proton – tantalum interactions will help to tune all the Neutrino Factory related calculations based on MARS predictions (capture, re-absorbtion, stress, etc.).

By arielle
(152 views)

SciBooNE, A Neutrino Cross Section Measurement Experiment at Fermilab

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

By tosca
(139 views)

New developments in FLUKA

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.

By frayne
(138 views)

Photohadronic processes and neutrinos

Photohadronic processes and neutrinos

Photohadronic processes and neutrinos. Summer school “High energy astrophysics” August 22-26, 2011 Weesenstein , Germany Walter Winter Universität Würzburg. TexPoint fonts used in EMF: A A A A A A A A. Contents. Lecture 1 (non-technical) Introduction, motivation

By regina
(66 views)

G ü nter Sigl Astroparticule et Cosmologie, Université Paris 7

G ü nter Sigl Astroparticule et Cosmologie, Université Paris 7

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

By oral
(126 views)

Ultra-High Energy Neutrino Fluxes

Ultra-High Energy Neutrino Fluxes

Ultra-High Energy Neutrino Fluxes. Neutrinos: A general connection to cosmic rays Neutrino fluxes in top-down models The Z-burst Summary. G ü nter Sigl GReCO, Institut d’Astrophysique de Paris, CNRS http://www.iap.fr/users/sigl/homepage.html.

By novia
(144 views)

Propagation of ultra-high energy cosmic rays in the Universe

Propagation of ultra-high energy cosmic rays in the Universe

Propagation of ultra-high energy cosmic rays in the Universe. Martin Lemoine Institut d’Astrophysique de Paris CNRS, Université Pierre & Marie Curie. Introduction. Ultra-high energy cosmic rays (UHECR) units: 1 EeV ´ 10 18 eV » 1 particle/km 2 /century above 10 20 eV. 2/41.

By aldon
(190 views)

Modelling neutrino cross sections

Modelling neutrino cross sections

Modelling neutrino cross sections. Jan T. Sobczyk Institute of Theoretical Physics, University of Wrocław (in collaboration with A. Ankowski, K. Graczyk, C. Juszczak, J. Nowak). Plan of the talk: Overview, „decomposition” of the total cross section.

By aria
(109 views)

Bochao Liu Xi’an Jiaotong University Collaborators: V.Baru, J.Haidenbauer and C.Hanhart

Bochao Liu Xi’an Jiaotong University Collaborators: V.Baru, J.Haidenbauer and C.Hanhart

Bochao Liu Xi’an Jiaotong University Collaborators: V.Baru, J.Haidenbauer and C.Hanhart.

By dobry
(99 views)

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

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

By rodd
(137 views)

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

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

Meson Production Results from E910 and Their Relevance to MiniBooNE. Jonathan Link Columbia University Fermilab Wine & Cheese November 18 th 2005. MiniBooNE. E910. Talk Outline. Motivation: What MiniBooNE needs What’s been done in the past Brookhaven E910 About the experiment

By kim
(207 views)

General facts and the experimental situation Acceleration (“bottom-up” scenario)

General facts and the experimental situation Acceleration (“bottom-up” scenario)

Cosmological Aspects of Ultra-High Energy Cosmic Rays. General facts and the experimental situation Acceleration (“bottom-up” scenario) The role of cosmic magnetic fields Neutrinos: Connection to cosmic rays and detection “New physics”. G ü nter Sigl

By quynh
(78 views)

Pion Production / Capture

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.

By morley
(190 views)

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

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

By marcus
(76 views)

Extra Spectral Components due to Hadronic Cascade

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.

By sumi
(78 views)

Analytic/Numerical Beam Simulation Model_B

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

By keiran
(148 views)

View Pion production PowerPoint (PPT) presentations online in SlideServe. SlideServe has a very huge collection of Pion production PowerPoint presentations. You can view or download Pion production presentations for your school assignment or business presentation. Browse for the presentations on every topic that you want.