'Cngs beam' presentation slideshows

LVD and the CNGS beam M. Selvi for the LVD Collaboration INFN Bologna

LVD and the CNGS beam M. Selvi for the LVD Collaboration INFN Bologna. Outline. Run 1 summary Some inconsistency in the database Run 2 results MC simulation: m flux from the rock. L arge V olume D etector.

917 views • 80 slides

CNGS Operation

747 views • 61 slides

CNGS Operation

614 views • 61 slides

Status of LBL Neutrino Experiments

547 views • 42 slides

Thomas Patzak APC , University Paris Diderot Paris 7

569 views • 38 slides

Versus and

Versus and. Do neutrinos really travel faster than light?. History in the Making?. 1862: Maxwell found that there should be electromagnetic waves travelling at approximately the (known) speed of light

441 views • 33 slides

Introduction Experimental procedure Beam characteristics and systematic

“ q 13 ” at CNGS. D.Duchesneau LAPP, Annecy. Introduction Experimental procedure Beam characteristics and systematic OPERA and ICARUS performances Conclusion. GDR Neutrino Lyon, September 20 th 2005. Mesure de q 13. Pour les projets de Long Baseline:. Dans le vide.

436 views • 30 slides

The OPERA experiment at LNGS

413 views • 29 slides

Status of the OPERA Neutrino Oscillation Experiment

Status of the OPERA Neutrino Oscillation Experiment. Sergey Dmitrievsky Joint Institute for Nuclear Research, Dubna on behalf of the OPERA Collaboration. CRACOW EPIPHANY CONFERENCE. On Physics in Underground Laboratories and Its Connection with LHC. 5-8 January 2010, Cracow, Poland. Outline.

472 views • 28 slides

The OPERA long baseline neutrino experiment : status and first results.

427 views • 27 slides

CNGS Overview Konrad Elsener

375 views • 25 slides

The OPERA experiment O scillation P roject with E mulsion t R acking A pparatus

The OPERA experiment O scillation P roject with E mulsion t R acking A pparatus. Direct search for the ? ? ? ? ? oscillation by looking at the appearance of ? ? in a pure ? ? beam ? CNGS program ? OPERA detector and experimental strategy ? Physics potential

345 views • 24 slides

Status of the OPERA long-baseline neutrino experiment

Magali Besnier. PIC 07- Annecy. Status of the OPERA long-baseline neutrino experiment. June 27 th 2007. OPERA. 37 INSTITUTS, ~ 160 PHYSI CISTS. International Collaboration (Europe + Japan) IIHE (ULB-VUB), Brussels Sofia IHEP Beijing, Shandong IRB Zagreb

351 views • 20 slides

An experiment to measure q 13 with the CNGS beam off axis and

207 views • 20 slides

Towards a larger Liquid Argon Imaging Chamber: the MODULAr project A. Guglielmi (INFN-PD)

Towards a larger Liquid Argon Imaging Chamber: the MODULAr project A. Guglielmi (INFN-PD) 27-09-2010. Beyond ICARUS-T600.

243 views • 16 slides

Hypothesis : scenario, SPS beam sharing, CNGS cycle length, SPS maximum intensity

Analysis of the maximum potential proton flux to CNGS M. Meddahi and E. Shaposhnikova CERN AB-2007-013 (PAF). Hypothesis : scenario, SPS beam sharing, CNGS cycle length, SPS maximum intensity CNGS design values and limitations SPS limitations Estimated proton flux. 1.1- Scenarios.

255 views • 15 slides

Beam Loss, Protection and Transfer Lines Working Group

207 views • 11 slides

Abstract

103 views • 1 slides

Congresso del Dipartimento di Fisica Highlights in Physics 2005

142 views • 1 slides