M. Dracos
Centre national de la recherche scientifique
Network
Latest external collaboration on country level. Dive into details by clicking on the dots.
Publication
Featured researches published by M. Dracos.
Journal of High Energy Physics | 2012
T. Adam; D. Autiero; T. Brugière; F. Brunet; G. Brunetti; A. Cazes; L. Chaussard; Y. Déclais; P. del Amo Sanchez; M. Dracos; D. Duchesneau; J. Favier; C. Girerd; C. Guerin; C. Jollet; J. Marteau; A. Meregaglia; E. Pennacchio; H. Pessard; T. Tran; A. Zghiche; L. Scotto Lavina
A bstractThe OPERA neutrino experiment at the underground Gran Sasso Laboratory has measured the velocity of neutrinos from the CERN CNGS beam over a baseline of about 730 km. The measurement is based on data taken by OPERA in the years 2009, 2010 and 2011. Dedicated upgrades of the CNGS timing system and of the OPERA detector, as well as a high precision geodesy campaign for the measurement of the neutrino baseline, allowed reaching comparable systematic and statistical accuracies.An arrival time of CNGS muon neutrinos with respect to the one computed assuming the speed of light in vacuum of
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2007
T. Adam; E. Baussan; K. Borer; Jean-Eric Campagne; N. Chon-Sen; C. De La Taille; N. Dick; M. Dracos; G. Gaudiot; T. Goeltzenlichter; Y. Gornushkin; J.-N. Grapton; J.L. Guyonnet; M. Hess; R. Igersheim; J. Janicsko Csathy; C. Jollet; F. Juget; H. Kocher; A. Krasnoperov; Z. Krumstein; Gisele Martin-Chassard; U. Moser; A.A. Nozdrin; A. Olchevski; S.Y. Porokhovoi; L. Raux; A. Sadovski; J. Schuler; H.U. Schütz
left( {6.5pm 7.4left( {mathrm{stat}.} right)_{-8.0}^{+8.3}left( {mathrm{sys}.} right)} right)mathrm{ns}
Physics of Atomic Nuclei | 2004
M. Dracos
was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light
Archive | 2012
A. Stahl; P. del Amo Sanchez; D. Duchesneau; H. Pessard; F. Cadoux; B. Andrieu; B. Popov; C. Giganti; J.M. Levy; J. Dumarchez; M. Buizza-Avanzini; Aivlé Cabrera; J. Dawson; D. Franco; D. Kryn; M. Obolensky; T. Patzak; A. Tonazzo; O. Bésida; A. Delbart; S. Emery; V. Galymov; E. Mazzucato; G. Vasseur; M. Zito; E. Baussan; M. Dracos; C. Jollet; A. Meregaglia; E. Vallazza
{{{left( {upsilon -c} right)}} left/ {c} right.}=left( {2.7pm 3.1left( {mathrm{stat}.} right)_{-3.3}^{+3.4}left( {mathrm{sys}.} right)} right)times {10^{-6 }}
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2007
E. Baussan; K. Borer; Jean Eric Campagne; Nathalie Chon-Sen; M. Dracos; Y. Gornushkin; J.L. Guyonnet; J. Janicsko Csathy; C. Jollet; Frédéric Juget; Alexei Krasnoperov; Z. Krumstein; U. Moser; A.A. Nozdrin; A. Olchevski; A. Sadovski; P. Vilain; T. Wälchli; G. Wilquet
. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5u2009μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level.