'10 tev' diaporamas de présentation

Alexandre Kisselev Institute for High Energy Physics Protvino, Russia

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Valya Khoze ( IPPP Durham University ) with Matt Dolan, Joerg Jaeckel , Chris Wymant

What do we expect from SUSY. Valya Khoze ( IPPP Durham University ) with Matt Dolan, Joerg Jaeckel , Chris Wymant. Introduction: soft SUSY-breaking terms and flavour universality Gauge Mediation and the status of pure Gauge Mediation 3 types of experimental constraints

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Gamma-ray absorption by cosmic radiation fields

blazar. GRB. Gamma-ray absorption by cosmic radiation fields. Susumu Inoue (Kyoto University). with (more than) a little help from my friends. Fermi. z~60-6. CTA. outline. 1. probe of high-z UV background. SI, R. Salvaterra, T. R. Choudhury, A. Ferrara,

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Gamma-ray absorption by cosmic radiation fields

blazar. GRB. Gamma-ray absorption by cosmic radiation fields. Susumu Inoue (Kyoto University). with (more than) a little help from my friends. Fermi. z~60-6. CTA. outline. 1. probe of high-z UV background. SI, R. Salvaterra, T. R. Choudhury, A. Ferrara,

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ATLAS Trigger Strategies and Early Physics Perspectives

ATLAS Trigger Strategies and Early Physics Perspectives. Thomas J. LeCompte High Energy Physics Division Argonne National Laboratory. LBNL Workshop May 2009. My Goals For This Talk.

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Future Colliders Why do we need them? And which one do we need?

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4-f Contact Interactions

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Prospects for New Physics at the LHC

atlas. Prospects for New Physics at the LHC. Ayana T Arce APS/AAPT Meeting February 13, 2010. Outline. New physics at the LHC Looking for new physics with ATLAS and CMS The art of the search Possible discoveries using leptons, jets and lifetimes Outlook. New physics (to us).

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Getting to Early Physics

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Discussion with LHCC Referees November 18, 2008

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Higgs in CMS

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Tibet Air Shower Array plus M uon D etector Array for the 100 TeV Gamma-Ray Wide Sky Survey

Tibet Air Shower Array plus M uon D etector Array for the 100 TeV Gamma-Ray Wide Sky Survey. K. Kawata For the Tibet AS g Collaboration ICRR, University of Tokyo. Locating PeV Cosmic-Ray Accelerators: Future Detectors in Multi-TeV Gamma-Ray Astronomy Adelaide 6 - 8 December 2006.

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Event Selection

Event Selection. Analysis without b- tag , ~10 pb -1. Trigger paths for 1 e31 : HLT_Mu9, HLT_Ele15_SW_L1R ( HLT8E29 not yet available in our ttbar PAT- tuples ) Dilepton selection : Highest pt lepton pair with opposite charge

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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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MPI Kernphysik, Heidelberg Humboldt Univ. Berlin Ruhr-Univ. Bochum Univ. Hamburg

Ground-Based Gamma Ray Astronomy at Energies > 10 TeV (H.E.S.S. et al. & beyond......) Gavin Rowell (MPIK Heidelberg). MPI Kernphysik, Heidelberg Humboldt Univ. Berlin Ruhr-Univ. Bochum Univ. Hamburg Landessternwarte Heidelberg Univ. Kiel Ecole Polytechnique, Palaiseau

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10 TeV vs 14 TeV 10 31 14.4.0

10 TeV vs 14 TeV 10 31 14.4.0. 10 TeV statistics based on only 500k min bias events; 3M event sample in progress. Note curious increase in dimuons at 10 TeV: this seems consistent across all trigger levels. L2 Rates 10 TeV vs 14 TeV 14.4.0.

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