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Related papers: OPERA first events from the CNGS neutrino beam

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The OPERA experiment has reported the detection of five $\nu_{\tau}$ candidates in the CNGS $\nu_{\mu}$ beam, allowing to reject the background-only hypothesis at the 5.1$\sigma$ level. Besides these events, on May 23$^{rd}$ 2011, OPERA…

High Energy Physics - Experiment · Physics 2016-05-12 Eduardo Medinaceli

The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio in the TeV energy region. We analyzed 403069 atmospheric muons corresponding to 113.4 days of livetime during the 2008…

High Energy Physics - Experiment · Physics 2010-03-10 OPERA Collaboration , N. Agafonova , A. Anokhina , S. Aoki , A. Ariga , T. Ariga , D. Autiero , A. Badertscher , A. Bagulya , A. Bertolin , M. Besnier , D. Bick , V. Boyarkin , C. Bozza , T. Brugière , R. Brugnera , G. Brunetti , S. Buontempo , A. Cazes , L. Chaussard , M. Chernyavsky , V. Chiarella , N. Chon-Sen , A. Chukanov , M. Cozzi , G. D'Amato , F. Dal Corso , N. D'Ambrosio , G. De Lellis , Y. D'eclais , M. De Serio , F. Di Capua , D. Di Ferdinando , A. Di Giovanni , N. Di Marco , S. Dmitrievski , M. Dracos , D. Duchesneau , S. Dusini , J. Ebert , O. Egorov , R. Enikeev , A. Ereditato , L. S. Esposito , J. Favier , G. Felici , T. Ferber , R. Fini , D. Frekers , T. Fukuda , C. Fukushima , V. I. Galkin , A. Garfagnini , G. Giacomelli , M. Giorgini , C. Goellnitz , J. Goldberg , D. Golubkov , L. Goncharova , Y. Gornushkin , G. Grella , F. Grianti , M. Guler , C. Gustavino , C. Hagner , K. Hamada , T. Hara , M. Hierholzer , K. Hoshino , M. Ieva , K. Jakovcic , C. Jollet , F. Juget , M. Kazuyama , S. H. Kim , M. Kimura , B. Klicek , J. Knuesel , K. Kodama , M. Komatsu , U. Kose , I. Kreslo , H. Kubota , C. Lazzaro , J. Lenkeit , A. Ljubicic , A. Longhin , G. Lutter , A. Malgin , G. Mandrioli , A. Marotta , J. Marteau , T. Matsuo , V. Matveev , N. Mauri , E. Medinaceli , F. Meisel , A. Meregaglia , P. Migliozzi , S. Mikado , S. Miyamoto , P. Monacelli , K. Morishima , U. Moser , M. T. Muciaccia , N. Naganawa , T. Naka , M. Nakamura , T. Nakano , D. Naumov , V. Nikitina , K. Niwa , Y. Nonoyama , S. Ogawa , A. Olchevski , C. Oldorf , G. Orlova , V. Osedlo , M. Paniccia , A. Paoloni , B. D. Park , I. G. Park , A. Pastore , L. Patrizii , E. Pennacchio , H. Pessard , V. Pilipenko , C. Pistillo , G. Policastro , N. Polukhina , M. Pozzato , K. Pretzl , P. Publichenko , F. Pupilli , R. Rescigno , T. Roganova , H. Rokujo , G. Romano , G. Rosa , I. Rostovtseva , A. Rubbia , A. Russo , V. Ryasny , O. Ryazhskaya , O. Sato , Y. Sato , A. Schembri , W. Schmidt Parzefall , H. Schroeder , L. Scotto Lavina , A. Sheshukov , H. Shibuya , S. Simone , M. Sioli , C. Sirignano , G. Sirri , J. S. Song , M. Spinetti , L. Stanco , N. Starkov , M. Stipcevic , T. Strauss , P. Strolin , S. Takahashi , M. Tenti , F. Terranova , I. Tezuka , V. Tioukov , P. Tolun , T. Tran , S. Tufanli , P. Vilain , M. Vladimirov , L. Votano , J. L. Vuilleumier , G. Wilquet , B. Wonsak , V. Yakushev , C. S. Yoon , T. Yoshioka , J. Yoshida , Y. Zaitsev , S. Zemskova , A. Zghiche , R. Zimmermann

We argue that the result quoted by the OPERA Collaboration cannot be interpreted as simply related to the muon neutrino moving at a superluminal velocity from the point of creation at CERN to the point of interaction at LNGS.

High Energy Physics - Experiment · Physics 2011-09-27 Jacek Ciborowski , Jakub Rembielinski

The possibility to improve the CERN to Gran Sasso neutrino beam performances for theta_{13} searches is investigated. We show that by an appropriate optimization of the target and focusing optics of the present CNGS design, we can increase…

High Energy Physics - Phenomenology · Physics 2009-11-07 A. Rubbia , P. Sala

Most recently, the measurement of the neutrino velocity with the OPERA detector in the CNGS beam shows unexpected indication, that the muon neutrino velocity, $v_{\nu}$, exceeds the velocity of light in the vacuum, $c$, which is obviously…

High Energy Physics - Phenomenology · Physics 2012-03-27 Nan Qin , Bo-Qiang Ma

We study how much the unique ability of the OPERA experiment to directly detect \nu_\tau can help in probing new, non-standard contact interactions of the third family of neutrinos. We perform a combined analysis of future, high-statistics…

High Energy Physics - Phenomenology · Physics 2008-11-26 Andreu Esteban-Pretel , Patrick Huber , Jose W. F. Valle

The OPERA neutrino oscillation experiment foresees the construction of two magnetized iron spectrometers located after the lead-nuclear emulsion targets. The magnet is made up of two vertical walls of rectangular cross section connected by…

The OPERA experiment was designed to search for $\nu_{\mu} \rightarrow \nu_{\tau}$ oscillations in appearance mode through the direct observation of tau neutrinos in the CNGS neutrino beam. In this paper, we report a study of the…

High Energy Physics - Experiment · Physics 2017-06-27 OPERA Collaboration

The project of a large underground experiment (NOE) devoted to long baseline neutrino oscillation measurement is presented

High Energy Physics - Experiment · Physics 2019-08-14 E. Scapparone

Energy spectra, intensity and composition of the CERN to Gran Sasso CNGS neutrino beam for nu_mu-->nu_tau and nu_mu-->nu_e oscillation searches are presented. The associated beam systematics, which is the major ingredient for the…

High Energy Physics - Phenomenology · Physics 2009-11-11 A. Ferrari , A. Guglielmi , P. R. Sala

We consider a possibility that the recent OPERA results on neutrinos' superluminality could be caused by a local effect of a new gauge field sourced by the earth. If neutrinos couple to this gauge field via a gauge-invariant but…

High Energy Physics - Phenomenology · Physics 2015-05-30 Ichiro Oda , Hajime Taira

Two simple exercises are solved, which educators can use to awake interest of their students in subtleties of the CERN Neutrino beam to Grand Sasso (CNGS) experiment. The first one is about the statistical error of the average departure…

Popular Physics · Physics 2011-10-14 Bernd A. Berg , Peter Hoeflich

We consider the possibility that the superluminal neutrino propagation reported by the OPERA collaboration originates from a violation of CPT. On this basis we compare our actual knowledge concerning the CPT theorem to the nuclear reaction…

High Energy Physics - Phenomenology · Physics 2011-10-20 Benjamin Koch

We report an updated result from the ICARUS experiment on the search for {\nu}{\mu} ->{\nu}e anomalies with the CNGS beam, produced at CERN with an average energy of 20 GeV and travelling 730 km to the Gran Sasso Laboratory. The present…

The OPERA experiment searching for nu(mu)- nu(tau) oscillations in the CERN to Gran Sasso nu(mu) beam, has detected so far three candidates of nu(tau) charged current interactions. All three events are attributed by the authors to the…

High Energy Physics - Experiment · Physics 2014-03-07 P. F. Loverre

The present paper highlights the data analysis status of the OPERA experiment. The experiment was designed to perform the neutrino interactions analysis on event-by-event basis, and optimized to search for $\nu_{\mu} \rightarrow \nu_{\tau}$…

High Energy Physics - Experiment · Physics 2017-08-23 T. A. Dzhatdoev , V. L. Troshina

The feasibility of a European next-generation very massive neutrino observatory in seven potential candidate sites located at distances from CERN ranging from 130 km to 2300 km, is being considered within the LAGUNA design study. The study…

High Energy Physics - Phenomenology · Physics 2010-03-10 A. Rubbia

The debate on OPERA focused on two extremes: either "OPERA is wrong" or our formulation of the laws of physics needs a major overhaul. I here argue that some effort should be directed toward manifestations of laws that are already known,…

High Energy Physics - Phenomenology · Physics 2012-02-01 Giovanni Amelino-Camelia

We present an optimization procedure for neutrino beams which could be produced at CERN and aimed to a set of seven possible underground sites in Europe with distances ranging from 130 km to 2300 km. Studies on the feasibility of a next…

Instrumentation and Detectors · Physics 2012-06-20 A. Longhin
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