'Mc simulation' presentation slideshows

COMPASS Present issues and near future

COMPASS Present issues and near future. On the strange quark PDFs The COMPASS programme for GPDs Stephane Platchkov IRFU*/Department of Nuclear Physics, CEA Saclay *Institute for Research on the Fundamental laws of the Universe. COMPASS: experimental setup (for a muon beam). 50 m.

541 views • 42 slides

ZEUS Status Report

E. Tassi Calabria Univ. , INFN and Hamburg Univ. ZEUS Status Report. 68 th DESY PRC Meeting 5-6 November 2009. OUTLINE Combined H1 and ZEUS Analyses ZEUS Physics Highlights Concluding Remarks. The combination of H1 and ZEUS data.

564 views • 36 slides

Backgrounds/Interference, etc: Lessons from RICE expt, OR: Everything We Did Wrong

Backgrounds/Interference, etc: Lessons from RICE expt, OR: Everything We Did Wrong.

359 views • 28 slides

PHENIX Capabilities for Studying the QCD Critical Point

389 views • 27 slides

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471 views • 27 slides

Distributed Computing for Crystallography

STFC. Distributed Computing for Crystallography. experiences and opportunities Dr. Kenneth Shankland & Tom Griffin ISIS Facility CCLRC Rutherford Appleton Laboratory. Expensive State of the art Good results Dedicated. Cheaper Can easily expand Dedicated. Cluster. Supercomputer.

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Small Angle Neutron Scattering (SANS) A DANSE Subproject

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A High Speed TRNG Based on SRAM for Resource Constrained Devices Chunhu Zhang and Yu Yao

A High Speed TRNG Based on SRAM for Resource Constrained Devices Chunhu Zhang and Yu Yao Dec 1st, 2009. Motivation. Foundation of Hardware Secuirty Mifare Classic RFID was cracked RNG is fundamental to cryptographic applications. Background. Traditional ways to generate RNG

425 views • 22 slides

Elastic pp Scattering at RHIC

Elastic pp Scattering at RHIC. STAR. Mainly : Elastic pp scattering program at RHIC Data analysis for the 2009 run Results (A N , r 5 , A NN & A SS ). Kin Yip For STAR Collaboration Brookhaven National Lab . Sept. 7, 2011, Alushta , Crimea, Ukraine. RHIC-Spin Accelerator Complex.

408 views • 19 slides

Searching for electron-positron annihilation line from Galactic compact objects with IBIS

Searching for electron-positron annihilation line from Galactic compact objects with IBIS. G. De C esare, INAF-IASF, Rome. Outlines. Positrons in the Galaxy: first detection in 1970 Positrons in the Galaxy: 511 keV emission from 1E 1740.7-2942 in 1990 The Galactic positrons origin

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LECTURE 26: PARTICLE FILTERS

LECTURE 26: PARTICLE FILTERS. Objectives: Bayes Rule (Again!) Sequential Bayesian Estimation Monte Carlo Methods State Space Formulations Kalman Filters Bayesian Particle Filters

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Double beta decays of 100 Mo and Molybdenum Observatory Of Neutrinos(MOON)

Double beta decays of 100 Mo and Molybdenum Observatory Of Neutrinos(MOON). Introduction Neutrino studied by 100 Mo ELEGANT V and Oto Cosmo Observatory Molybdenum Observatory Of Neutrinos (MOON) Concluding Remarks. Collaborators(Japan-USA).

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UTB SOI for LER/RDF

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A Model of the Chemical Kinetics Exhibited by a Telechelic Polymer

A Model of the Chemical Kinetics Exhibited by a Telechelic Polymer. Mark Wilson . Acknowledgements: Dr. Arlette Baljon Department of Physics, San Diego State University Dr. Avinoam Rabinovitch Department of Physics, Ben Gurion University of the Negev, Israel Joris Billen

263 views • 15 slides

Backup Slides

Backup Slides. David Doll. Beyond SM theories. Mark Wise paper. BBU starting point and expansion. Look at 2.24 and 2.26 to see difference between kinetic and pole scheme in hep -ph/0607316. Former Analysis extended. Novosibirsk function: Argus function:. Source Babar doc. where:.

670 views • 15 slides

CERN and HelixNebula , the Science Cloud

256 views • 13 slides

338 views • 13 slides

VELO ADC vs Charge Calibration

VELO ADC vs Charge Calibration . Jianchun Wang April 16, 2008. This is an update to the presentation at April 11 st VELO Group Meeting. A new scan data of larger charge range has been taken. Further more detailed studies. Introduction.

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ALFA GeoModel implementation and simulation status

648 views • 6 slides

FEM Results

Y. Z. X. X, transverse direction Y, normal direction Z, axially direction. FEM Results. 5 500 38. Y. Z. X. X, transverse direction Y, normal direction Z, axially direction. Stave deflections. X direction pixel width = 50 microns sigma = 50/sqrt(12) = 14.4 microns

195 views • 2 slides