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Related papers: Third road to the OPERA: a tunnel after all?

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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

OPERA (Oscillation Project with Emulsion tRacking Apparatus)is an international collaboration between Europe and Asia, aiming to give the first direct proof of tau neutrino appearance in a pure muon neutrino beam, in order to validate the…

High Energy Physics - Experiment · Physics 2008-10-15 Dominique Duchesneau

Modified neutrino dispersion relations, which still obey the relativity principle, can have both a superluminal (muon-type) neutrino and a luminal (electron-type) neutrino, as long as neutrino-mass effects can be neglected. The idea is to…

High Energy Physics - Phenomenology · Physics 2012-01-24 F. R. Klinkhamer

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 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

The OPERA experiment, exposed to the CERN to Gran Sasso $\nu_\mu$ beam, collected data from 2008 to 2012. Four oscillated $\nu_\tau$ Charged Current interaction candidates have been detected in appearance mode, which are consistent with…

High Energy Physics - Experiment · Physics 2017-03-15 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 , T. Fukuda , G. Galati , A. Garfagnini , J. Goldberg , Y. Gornushkin , G. Grella , A. M. Guler , C. Gustavino , C. Hagner , T. Hara , 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 , A. Lauria , A. Ljubicic , A. Longhin , A. Malgin , M. Malenica , G. Mandrioli , T. Matsuo , V. Matveev , N. Mauri , E. Medinaceli , A. Meregaglia , S. Mikado , P. Monacelli , M. C. Montesi , K. Morishima , M. T. Muciaccia , N. Naganawa , T. Naka , M. Nakamura , T. Nakano , Y. Nakatsuka , K. Niwa , S. Ogawa , T. Omura , K. Ozaki , A. Paoloni , L. Paparella , B. D. Park , I. G. Park , L. Pasqualini , A. Pastore , L. Patrizii , H. Pessard , D. Podgrudkov , N. Polukhina , M. Pozzato , F. Pupilli , M. Roda , T. Roganova , H. Rokujo , G. Rosa , O. Ryazhskaya , O. Sato , A. Schembri , I. Shakirianova , T. Shchedrina , A. Sheshukov , H. Shibuya , T. Shiraishi , G. Shoziyoev , S. Simone , M. Sioli , C. Sirignano , G. Sirri , 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

The difference in light's travel time from CERN to GPS to Gran Sasso, on the one hand, and light going the direct route in vacuum (mimicked by neutrinos), on the other hand, is analyzed with a modified Robertson test theory of the Lorentz…

General Physics · Physics 2011-11-11 Jose G. Vargas

Tunneling of a particle through a potential barrier remains one of the most remarkable quantum phenomena. Owing to advances in laser technology, electric fields comparable to those electrons experience in atoms are readily generated and…

We suggest a possible interpretation of the recent observation by the OPERA collaboration of superluminal propagation of neutrinos. We show that it is in principle possible that the group velocity of neutrinos exceeds the speed of light…

High Energy Physics - Phenomenology · Physics 2011-10-13 Antonio Mecozzi , Marco Bellini

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

We digress on the implications of recent claims of superluminal neutrino propagation. No matter how we turn it around such behaviour is very odd and sits uncomfortably even within "far-fetched" theories. In the context of non-linear…

High Energy Physics - Phenomenology · Physics 2011-10-07 Joao Magueijo

We argue that the recent measurement of the neutrino velocity to be higher than the velocity of light could be due to violation of Lorentz invariance by the muon neutrinos. This result need not undermine special-relativistic foundational…

High Energy Physics - Phenomenology · Physics 2011-10-07 Robert B. Mann , Utpal Sarkar

According to the measurement of muon-neutrino experiment done by the OPERA collaboration, the speed of high-energy neutrino exceeds that of light in vacuum by 25ppm. Assuming that this result is correct, a possible resolution of the dilemma…

High Energy Physics - Phenomenology · Physics 2012-01-17 Noboru Nakanishi

The decay of neutrino mass eigenstates leads to a change of the conversion and survival probability of neutrino flavor eigenstates. Remarkably, we find that the neutrino decay provides an enhancement of the expected tau appearance signal…

High Energy Physics - Phenomenology · Physics 2016-06-22 Giulia Pagliaroli , Natalia Di Marco , Massimo Mannarelli

The OPERA experiment was designed to study $\nu_\mu\to\nu_\tau$ oscillations in appearance mode in the CNGS neutrino beam. In this letter we report the final analysis of the full data sample collected between 2008 and 2012, corresponding to…

High Energy Physics - Experiment · Physics 2018-05-30 OPERA Collaboration , N. Agafonova , A. Alexandrov , A. Anokhina , S. Aoki , A. Ariga , T. Ariga , A. Bertolin , C. Bozza , R. Brugnera , A. Buonaura , S. Buontempo , M. Chernyavskiy , 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. Dmitrievsky , M. Dracos , D. Duchesneau , S. Dusini , T. Dzhatdoev , J. Ebert , A. Ereditato , J. Favier , R. A. Fini , F. Fornari , T. Fukuda , G. Galati , A. Garfagnini , V. Gentile , J. Goldberg , Y. Gornushkin , S. Gorbunov , G. Grella , A. M. Guler , C. Gustavino , C. Hagner , T. Hara , T. Hayakawa , A. Hollnagel , K. Ishiguro , A. Iuliano , K. Jakovcic , C. Jollet , C. Kamiscioglu , M. Kamiscioglu , S. H. Kim , N. Kitagawa , B. Klicek , K. Kodama , M. Komatsu , U. Kose , I. Kreslo , F. Laudisio , A. Lauria , A. Ljubicic , A. Longhin , P. Loverre , A. Malgin , M. Malenica , G. Mandrioli , T. Matsuo , 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 , K. Niwa , N. Okateva , A. Olchevsky , S. Ogawa , K. Ozaki , A. Paoloni , L. Paparella , B. D. 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 , A. Sadovsky , O. Sato , A. Schembri , I. Shakiryanova , T. Shchedrina , H. Shibuya , E. Shibayama , T. Shiraishi , S. Simone , 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 , A. Ustyuzhanin , S. Vasina , P. Vilain , E. Voevodina , L. Votano , J. L. Vuilleumier , G. Wilquet , B. Wonsak , C. S. Yoon

We argue that with the current experimental setup of the OPERA neutrino experiment no `bit' of information faster than light was or could be sent, and therefore no violation of Lorentz symmetry and/or causality was observed.

High Energy Physics - Phenomenology · Physics 2011-10-19 F. Giacosa , P. Kovacs , S. Lottini

Recent time-of-flight measurements on muon neutrinos in the OPERA neutrino oscillation experiment have found anomalously short times compared to the light travel-times, corresponding to a superluminal velocity, $v-1=2.37\pm0.32\times…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 P. C. W. Davies , Ian G. Moss

This talk opens the CosPA2011 session on OPERA's superluminal neutrino claim. I summarize relevant observations and constraints from OPERA, MINOS, ICARUS, KamLAND, IceCube and LEP as well as observations of SN1987A. I selectively review…

High Energy Physics - Phenomenology · Physics 2012-11-20 Jarah Evslin

Modification of special theory of relativity is proposed to describe the propagation of signals with superluminal velocity. Modified kinematics and Lorentz transformations of Maxwell's equations are described. A possible experiment on…

General Physics · Physics 2011-10-14 V. I. Klyukhin

In the First Part of this paper [that was submitted for pub. in 1991 and appeared in print in Phys. Reports 214 (1992) 339] we critically review the main theoretical definitions and calculations of the sub-barrier tunnelling and reflection…

Condensed Matter · Physics 2007-09-17 Vladislav S. Olkhovsky , Erasmo Recami