'Physics performance' diaporamas de présentation

ALICE Performance

ALICE Performance. Physics motivation Experimental conditions Physics performance. LHC Energy. For A-A collisions: E cms = 5500 A GeV E lab = E cms 2 / (2 A m N ) = 1.6 ? 10 7 A GeV

584 views • 43 slides

ATLAS overview

Lecce. Andrea Ventura University of Salento & INFN Lecce on behalf of the ATLAS Collaboration. ATLAS overview. New Trends in High-Energy Physics Alushta , Crimea, Ukraine , September 5, 2011. The Large Hadron Collider.

470 views • 29 slides

ATLAS overview

Lecce. Andrea Ventura University of Salento & INFN Lecce on behalf of the ATLAS Collaboration. ATLAS overview. New Trends in High-Energy Physics Alushta , Crimea, Ukraine , September 5, 2011. The Large Hadron Collider.

291 views • 29 slides

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EURO ?

EURO ?. A High Intensity Neutrino Oscillation Facility in Europe. Introduction What EUROnu is doing Next step Input to the Strategy Review Future of EUROnu Conclusions. On behalf of the EUROnu Consortium. EUROnu. FP7 Design Study

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Physics and Performance Evaluation Group: Status and plans

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SiD A Linear Collider Detector

SiD A Linear Collider Detector. SLAC Users Organization Annual Meeting September 17, 2009 John Jaros. LC Physics Case is Compelling as Ever.

302 views • 20 slides

Vertex Trigger Workshop

Vertex Trigger Workshop. Saturday, 14th of November, 1998 The Vertex Trigger Detector Project M. Koratzinos (CERN). Outline of the talk. A personal and probably biased overview of the project by someone working on it for the past couple of years. Historical Overview Project components

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The Silicon Detector Concept

The Silicon Detector Concept. Taipei ACFA Meeting November 9, 2004 John Jaros. Calorimetry drives the Detector Design.

423 views • 18 slides

The Silicon Detector Concept

The Silicon Detector Concept. Taipei ACFA Meeting November 9, 2004 John Jaros. Calorimetry drives the Detector Design.

183 views • 18 slides

KM3NeT

KM3NeT. P.Kooijman Universities of Amsterdam & Utrecht for the consortium. KM3NeT Goals. Neutrino telescope for detecting cosmic neutrinos Dark Matter Annihilation (100-500 GeV ) Galactic sources (E -2 up to ~100 TeV ) Extragalactic sources (E -2 ) Gamma Ray Bursts (E -1 to E -2 )

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Physics and Performance Evaluation Group

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Sunanda Banerjee ( Saha Inst. Nucl . Phys., Kolkata, India)

IEEE Nuclear Science Symposium and Medical Imaging Conference Short Course The Geant4 Simulation Toolkit. Sunanda Banerjee ( Saha Inst. Nucl . Phys., Kolkata, India) Min Cheol Han ( Hanyang Univ., Seoul, Korea) Steffen Hauf (XFEL, Hamburg, Germany)

254 views • 14 slides

AGENDA (km3net2p3.fr)

AGENDA (http://km3net.in2p3.fr). Manage password: wp20710. Pending Issues. Physics Priority < 1 TeV: Dark matter 1-100 TeV: HESS sources, GRBs >1 PeV: Diffuse flux, GZK, AGN Evaluation of NEMO geometry Evaluate effect of energy measurement on sensitivity

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Summary of Parallel Session 3A : Hadronic Validation

Summary of Parallel Session 3A : Hadronic Validation . J. Yarba Fermilab 17th Geant4 Collaboration Workshop 9/14/2012. Topics. Validation Status Report and Work Plan Validation for LHE experiments Related discussions Physics Performance and Benchmarking of INCL++.

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Neutrino oscillation physics with the Neutrino Factory

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Computing in US ATLAS Trigger/DAQ

Computing in US ATLAS Trigger/DAQ. Physics Performance (Contributions to Physics TDR) trigger chapter - algorithms; see Trigger Performance top physics - Single top: MSU (Pineiro, Brock) top pair: Columbia (Parsons) Trigger Performance (Contributions to TPSR and TDR)

174 views • 3 slides