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In the context of theories where particles can have different limiting velocities, we review the running of particle speeds towards a common limiting velocity at low energy. Motivated by the recent OPERA experimental results, we describe a…

High Energy Physics - Phenomenology · Physics 2015-03-19 Mohamed M. Anber , John F. Donoghue

From a mathematical point of view velocities can be larger than c. It has been shown that Lorentz transformations are easily extended in Minkowski space to address velocities beyond the speed of light. Energy and momentum conservation fixes…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. Giani

OPERA is an experiment that aims at detecting the appearance of tau-neutrino in an almost pure mu-neutrino beam (the CNGS neutrino beam) through oscillation. OPERA is a hybrid detector that associates nuclear emulsions to electronic…

High Energy Physics - Experiment · Physics 2009-10-20 Tsutomu Fukuda

We found three mistakes in the article " The OPERA neutrino velocity result and the synchronisation of clocks" by Contaldi \cite{Contaldi}. First, the definition of the angle of the latitude in the geoid description leads to a prolate…

High Energy Physics - Phenomenology · Physics 2011-10-19 Olivier Besida

We discuss two experiments ICANOE and OPERA that have been proposed within the context of long-baseline and atmospheric neutrino experiments in Europe. The joint ICANOE/OPERA program aims at further improving our understanding of the effect…

High Energy Physics - Experiment · Physics 2009-10-31 Andre Rubbia

The superluminal propagation of neutrinos observed by the OPERA collaboration can be explained by an energy dependent potential for the neutrino beam in passage through the Earth.

General Physics · Physics 2011-10-19 Jerrold Franklin

We show that special relativity (SR) may be consistent with the OPERA measurements of the neutrino velocity provided the latter is corrected for the second order term in V^2/c^2 implied by the velocity, V, of the alpha particles from…

General Physics · Physics 2011-10-19 Jean-Paul Mbelek

An interpretation of the superluminal velocity observed by OPERA collaboration is given in terms wave packet distortion of ultrarelativistic massive neutrinos. Standard quantum-mechanical time evolution of physical states can explain the…

High Energy Physics - Phenomenology · Physics 2011-10-19 M. De Sanctis

We propose a test to compare the speed of muons and muon neutrinos produced in the same bundles in the atmosphere. By comparing the arrival times of primary muons and muons induced by neutrinos, experiments such as Super-Kamiokande, IceCube…

High Energy Physics - Experiment · Physics 2011-12-08 T. Montaruli , F. Ronga

The superluminal propagation of neutrinos observed by OPERA collaboration can be interpreted as neutrinos traveling in a pseudoscalar potential which may be generated by a medium. The OPERA differential arrival time data set a constraint on…

High Energy Physics - Phenomenology · Physics 2011-10-12 Sarira Sahu , Bing Zhang

Precise tests of Lorentz invariance in neutrinos can be performed using long baseline experiments such as MINOS and OPERA or neutrinos from astrophysical sources. The MINOS collaboration reported a measurement of the muonic neutrino…

High Energy Physics - Phenomenology · Physics 2015-05-30 Giacomo Cacciapaglia , Aldo Deandrea , Luca Panizzi

The OPERA experiment reached its main goal by proving the appearance of $\nu_{\tau}$ in the CNGS $\nu_{\mu} $ beam. A sample of five $\nu_{\tau}$ candidates was collected allowing to reject the null hypothesis at $5.1 \sigma$. The…

High Energy Physics - Experiment · Physics 2017-05-09 L. Patrizii

This paper reviews the current experimental program envisaged with the future CERN neutrino beam called CNGS. Two detectors, OPERA and ICARUS, are under preparation and should investigate the neutrino properties coming from the CNGS to shed…

High Energy Physics - Experiment · Physics 2009-11-07 D. Duchesneau

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 OPERA experiment aims at the direct confirmation of the leading oscillation mechanism in the atmospheric sector looking for the appearance of $\nu_{\tau}$ in an almost pure $\nu_{\mu}$ beam (the CERN CNGS beam). In five years of physics…

High Energy Physics - Experiment · Physics 2019-08-13 Fabio Pupilli

Motivated by the tentative observation of superluminal neutrinos by the OPERA experiment, we present a model of active-sterile neutrino oscillations in which sterile neutrinos are superluminal and active neutrinos appear superluminal by…

High Energy Physics - Phenomenology · Physics 2012-01-17 D. Marfatia , H. Päs , S. Pakvasa , T. J. Weiler

In recent experiments conducted by the OPERA collaboration, researchers claimed the observation of neutrinos propagating faster than the light speed in vacuum. If correct, their results raise several issues concerning the special theory of…

High Energy Physics - Phenomenology · Physics 2011-12-15 C. A. Dartora , G. G. Cabrera

Quantum trajectories are used to study OPERA findings regarding superluminal neutrinos. As the applicable stationary quantum Klein-Gordon equation is real, real quantum reduced actions and subsequent real quantum trajectories follow. The…

General Physics · Physics 2016-11-25 Edward R. Floyd

The OPERA experiment was designed to search for $\nu_{\mu} \rightarrow \nu_{\tau}$ oscillations in appearance mode, i.e. by detecting the $\tau$-leptons produced in charged current $\nu_{\tau}$ interactions. The experiment took data from…

High Energy Physics - Experiment · Physics 2016-08-08 OPERA Collaboration , N. Agafonova , A. Aleksandrov , A. Anokhina , S. Aoki , A. Ariga , T. Ariga , D. Bender , A. Bertolin , I. Bodnarchuk , C. Bozza , R. Brugnera , A. Buonaura , S. Buontempo , B. Büttner , M. Chernyavsky , A. Chukanov , L. Consiglio , N. D'Ambrosio , G. De Lellis , M. De Serio , P. Del Amo Sanchez , A. Di Crescenzo , D. Di Ferdinando , N. Di Marco , S. Dmitrievski , M. Dracos , D. Duchesneau , S. Dusini , T. Dzhatdoev , J. Ebert , A. Ereditato , R. A. Fini , F. Fornari , T. Fukuda , G. Galati , A. Garfagnini , J. Goldberg , Y. Gornushkin , G. Grella , A. M. Guler , C. Gustavino , C. Hagner , T. Hara , H. Hayakawa , A. Hollnagel , B. Hosseini , K. Ishiguro , K. Jakovcic , C. Jollet , C. Kamiscioglu , M. Kamiscioglu , J. H. Kim , S. H. Kim , N. Kitagawa , B. Klicek , K. Kodama , M. Komatsu , U. Kose , I. Kreslo , F. Laudisio , A. Lauria , A. Ljubicic , A. Longhin , P. F. Loverre , A. Malgin , M. Malenica , G. Mandrioli , T. Matsuo , T. Matsushita , V. Matveev , N. Mauri , E. Medinaceli , A. Meregaglia , S. Mikado , M. Miyanishi , F. Mizutani , P. Monacelli , M. C. Montesi , K. Morishima , M. T. Muciaccia , N. Naganawa , T. Naka , M. Nakamura , T. Nakano , Y. Nakatsuka , K. Niwa , S. Ogawa , A. Olchevsky , T. Omura , K. Ozaki , A. Paoloni , L. Paparella , B. D. Park , I. G. Park , L. Pasqualini , A. Pastore , L. Patrizii , H. Pessard , C. Pistillo , D. Podgrudkov , N. Polukhina , M. Pozzato , F. Pupilli , M. Roda , T. Roganova , H. Rokujo , G. Rosa , O. Ryazhskaya , O. Sato , A. Schembri , W. Schmidt-Parzefall , I. Shakirianova , T. Shchedrina , A. Sheshukov , H. Shibuya , T. Shiraishi , G. Shoziyoev , S. Simone , M. Sioli , C. Sirignano , G. Sirri , A. Sotnikov , M. Spinetti , L. Stanco , N. Starkov , S. M. Stellacci , M. Stipcevic , P. Strolin , S. Takahashi , M. Tenti , F. Terranova , V. Tioukov , S. Tufanli , P. Vilain , M. Vladymyrov , L. Votano , J. L. Vuilleumier , G. Wilquet , B. Wonsak , C. S. Yoon , S. Zemskova
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