'Herwig' diaporamas de présentation

HERWIG

Herwig++. HERWIG. Peter Richardson IPPP, Durham University. Summary. Introduction HERWIG 6.5 Herwig++ Parton Shower Underlying Event Hard Radiation and NLO BSM Physics Hadronization Hadron and Tau Decays Conclusions. A Monte Carlo Event. Hard Perturbative scattering:

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Lecture 1 Time Scales, Temperature-density Scalings, Critical Masses

Lecture 1 Time Scales, Temperature-density Scalings, Critical Masses. I. Preliminaries. The life of any star is a continual struggle between gravity, seeking to reduce the star to a point, and pressure, which supports the star. Stars are gravitationally confined thermonuclear reactions.

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Recent Experimental QCD Results

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BSM Physics in Herwig++

BSM Physics in Herwig++. M. Baehr, S. Gieseke, M. Gigg , D. Grellscheid, K. Hamilton, S. Latunde-Dada, S. Plaetzer, PR , M.H. Seymour, A. Sherstnev, B.R. Webber. Peter Richardson IPPP, Durham University and CERN Theory Group. A. Siodmok J. Tully. Outline. Introduction Philosophy

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HERWIG vs. HERWIG++ - SUSY: SU3 comparison -

HERWIG vs. HERWIG++ - SUSY: SU3 comparison -. ATLAS MC Generator Meeting Physics and Performance Week: 26-29 August 2008. Claire Gwenlan (Oxford) , Zhonghua Qin (DESY) Andy Buckley (Durham), Alessandro Tricoli (RAL). with many thanks to Peter Richardson for helpful discussion!!!.

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Fortran HERWIG Status Report and Validation in Athena rel. 14

Fortran HERWIG Status Report and Validation in Athena rel. 14. By Jon Butterworth (UCL) Claire Gwenlan (Oxford) Alessandro Tricoli (RAL). ATLAS MC Generator Meeting, 11 th December 2008. Latest Tags Herwig_i-00-03-15 ? CVS tag HEAD Herwig_i-00-03-13 ? 14.4.0.1 release.

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High P T Inclusive Jets Study

1. High P T Inclusive Jets Study. Manuk Zubin Mehta , Prof. Manjit kaur Panjab University, Chandigarh India CMS Meeting March , 2009. 2. Introduction: Inclusive Jets

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Yields from single AGB stars

Yields from single AGB stars. Amanda Karakas Research School of Astronomy & Astrophysics Mt Stromlo Observatory. Introduction. The asymptotic giant branch (AGB) is the final nuclear burning phase before stars become PN The composition of PN are determined (in part) by AGB nucleosynthesis

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Monte Carlo tuning using ATLAS data

Monte Carlo tuning using ATLAS data. Davide Costanzo (on behalf of the ATLAS collaboration). Monte Carlo simulation process. The Monte Carlo simulation of the ATLAS detector is used in most ATLAS papers/results. Event generators:

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Quark and Gluon Jet Fragmentation Differences

Quark and Gluon Jet Fragmentation Differences. Andrey Korytov. Abstracts covered in this talk 5-0081 Fragmentation differences of quark and gluon jets at the Tevatron (CDF) 5-0437 Charged particle multiplicities in 3-jet events and two-gluon systems (DELPHI). CDF. k T =1 GeV/c.

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Event Generation with HERWIG

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Monte Carlo Simulation of Neutrino Induced EAS

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Photon(s)+X Group: HERWIG vs. MadGraph

Photon(s)+X Group: HERWIG vs. MadGraph. Osamu Jinnouchi (Tokyo Tech), Fernando Monticelli (La Plate), Bruce Schumm (SCIPP), Harnan Wahlberg (La Plata) Incidental slides for the discussion of whether the Photon+X group should be asked to migrate to MadGraph for 2016 analyses.

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Pythia and Herwig settings

Pythia and Herwig settings. Kt 2 = PARP(64)(1-z)Q 2 L QCD = PARP (61). ISR setting Tune-A: PARP(67)=4 Pt(Z) tunning: PARP(64)=0.2 by Willis (Herwig: 1.0) Top/diboson MC production in 4.9.1 Tune-A: PARP(67)=4 Pt(Z) tunning: PARP(64)= 1.0 W/Z production MC production in 4.9.1

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driven by high energy injection from nuclear burning

Hydrodynamics processes in stars: Investigating the physics of the nuclear production site of the elements. He-shell flash convection in giant stars: production of carbon, oxygen, F, Mg, Na, and heavy elements like barium.

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NT CVD : Development and Validation of new Diagnostic, Preventive and Therapeutic Tools for the Prevention of Cardiovasc

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