English
Related papers

Related papers: Bimetric Relativity and the Opera Neutrino Experim…

200 papers

This is a brief note discussing the energy dependence of superluminal neutrino velocities recently claimed by OPERA [1,2]. The analysis is based on the data provided there on this issue, as well as on consistency with neutrino data from…

High Energy Physics - Phenomenology · Physics 2011-10-25 N. D. Hari Dass

The OPERA collaboration reported [1] an anomaly in the ratio of the speed of neutrinos to the speed of light of (v-c)/c =(2.48\pm0.28 (stat.) \pm 0.30 (sys.))\times10-5. I identify sources of systematic uncertainty that were not considered…

High Energy Physics - Experiment · Physics 2011-10-12 Juergen Knobloch

The result of the OPERA experiment revealed that the velocity of muon-neutrinos was larger than the speed of light. We argue that this apparent superluminal velocity can be interpreted as a weak value, which is a new concept recently…

High Energy Physics - Phenomenology · Physics 2011-10-11 Shogo Tanimura

In a recent study, Cohen and Glashow argue that superluminal neutrinos of the type recently reported by OPERA should be affected by anomalous Cherenkov-like processes. This causes them to loose much of their energy before reaching the OPERA…

High Energy Physics - Phenomenology · Physics 2015-05-30 Giovanni Amelino-Camelia , Laurent Freidel , Jerzy Kowalski-Glikman , Lee Smolin

In this paper, we consider the apparent superluminal speed of neutrinos in their travel from CERN to Gran Susso, as measured by the OPERA experiment, within the framework of the Extended Lorentz Transformation Model. The model is based on a…

General Physics · Physics 2012-02-28 S. Hamieh

We show that the superluminal speeds of the muon neutrinos observed in the OPERA experiment can be explained within a relativity theory with extra time like dimensions. In addition, such theory predicts, the existence of dark matter.

General Relativity and Quantum Cosmology · Physics 2011-10-24 Matej Pavšič

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

We pinpoint how a subatomic particle with non-zero mass may attain, in principle, velocities faster-than-light by travelling in helical motion in the limit of very large momentum. This is an educated guess by virtue of the MINOS and OPERA…

General Physics · Physics 2011-10-06 E. Canessa

Recent results from the OPERA experiment reported a neutrino beam traveling faster than light. The experiment measured the neutrino time of flight (TOF) over a baseline from the CERN to the Gran Sasso site. The neutrino beam arrives 60 ns…

General Physics · Physics 2015-06-03 Claudio Germana

Violation of Lorentz invariance (VLI) has been suggested as an explanation of the superluminal velocities of muon neutrinos reported by OPERA. In this note we show that the amount of VLI required to explain this result poses severe…

High Energy Physics - Phenomenology · Physics 2011-12-21 R. Cowsik , S. Nussinov , U. Sarkar

We give an explanation on the effect of superluminal neutrinos in the OPERA experiment and show that the SN 1987A data and the recent OPERA data do agree well by the use of common known physics. The data in addition can give a good number…

General Physics · Physics 2011-12-05 H. Genreith

The OPERA Collaboration reported evidence for muonic neutrinos traveling slightly faster than light in vacuum. While waiting further checks from the experimental community, here we aim at exploring some theoretical consequences of the…

High Energy Physics - Phenomenology · Physics 2015-05-30 Alessandro Drago , Isabella Masina , Giuseppe Pagliara , Raffaele Tripiccione

A physical metric is introduced as one that directly gives experimental data without further coordinate transformation. It will be shown that the geodesic equation for the Schwartzschild metric does not give the correct expression for the…

General Physics · Physics 2011-11-29 Yukio Tomozawa

First we call the attention that velocity defined by ratio between some intervals of space and time respectively is sometimes ambiguous, in the framework of quantum theory. Velocity in general is not possible to be well defined as some…

High Energy Physics - Phenomenology · Physics 2011-12-06 Shi-Yuan Li

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

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

In this letter, we show that superluminal neutrinos announced by OPERA could be explained by the existence of a monopole, which is left behind after the spontaneous symmetry breaking (SSB) phase transition of some scalar fields in the…

High Energy Physics - Phenomenology · Physics 2011-10-10 Peng Wang , Houwen Wu , Haitang Yang

In the bimetric scalar-tensor gravitational theory there are two frames associated with the two metrics {\hat g}_{\mu\nu} and g_{\mu\nu}, which are linked by the gradients of a scalar field \phi. The choice of a comoving frame for the…

General Relativity and Quantum Cosmology · Physics 2014-11-17 J. W. Moffat

The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the $\nu_\mu \to \nu_\tau$ channel, via the detection of the $\tau$-leptons created in charged current…

High Energy Physics - Experiment · Physics 2013-08-13 OPERA Collaboration , N. Agafonova , A. Aleksandrov , A. Anokhina , S. Aoki , A. Ariga , T. Ariga , T. Asada , D. Autiero , A. Badertscher , A. Ben Dhahbi , D. Bender , A. Bertolin , C. Bozza , R. Brugnera , G. Brunetti , B. Buettner , S. Buontempo , L. Chaussard , M. Chernyavskiy , V. Chiarella , A. Chukanov , L. Consiglio , N. D'Ambrosio , P. Del Amo Sanchez , G. De Lellis , M. De Serio , A. Di Crescenzo , D. Di Ferdinando , N. Di Marco , S. Dmitrievski , M. Dracos , D. Duchesneau , S. Dusini , J. Ebert , A. Ereditato , J. Favier , T. Ferber , R. A. Fini , T. Fukuda , A. Garfagnini , G. Giacomelli , C. Goellnitz , J. Goldberg , Y. Gornushkin , G. Grella , F. Grianti , A. M. Guler , C. Gustavino , C. Hagner , K. Hakamata , T. Hara , T. Hayakawa , M. Hierholzer , A. Hollnagel , B. Hosseini , H. Ishida , K. Ishiguro , M. Ishikawa , K. Jakovcic , C. Jollet , C. Kamiscioglu , M. Kamiscioglu , T. Katsuragawa , H. Kawahara , J. Kawada , J. H. Kim , S. H. Kim , M. Kimura , N. Kitagawa , B. Klicek , K. Kodama , M. Komatsu , U. Kose , I. Kreslo , A. Lauria , J. Lenkeit , A. Ljubicic , A. Longhin , P. Loverre , A. Malgin , G. Mandrioli , J. Marteau , T. Matsuo , V. Matveev , N. Mauri , E. Medinaceli , A. Meregaglia , P. Migliozzi , S. Mikado , A. Minotti , M. Miyanishi , E. Miyashita , P. Monacelli , M. C. Montesi , K. Morishima , M. T. Muciaccia , N. Naganawa , T. Naka , M. Nakamura , T. Nakano , Y. Nakatsuka , K. Niwa , S. Ogawa , N. Okateva , A. Olshevsky , T. Omura , K. Ozaki , A. Paoloni , B. D. Park , I. G. Park , A. Pastore , L. Patrizii , E. Pennacchio , H. Pessard , C. Pistillo , D. Podgrudkov , N. Polukhina , M. Pozzato , K. Pretzl , F. Pupilli , R. Rescigno , M. Roda , T. Roganova , H. Rokujo , G. Rosa , I. Rostovtseva , A. Rubbia , A. Russo , O. Ryazhskaya , O. Sato , Y. Sato , A. Schembri , W. Schmidt-Parzefall , I. Shakiryanova , T. Schcedrina , 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 , T. Strauss , P. Strolin , K. Suzuki , S. Takahashi , M. Tenti , F. Terranova , V. Tioukov , P. Tolun , S. Tufanli , P. Vilain , M. Vladimirov , L. Votano , J. L. Vuilleumier , G. Wilquet , B. Wonsak , C. S. Yoon , J. Yoshida , M. Yoshimoto , Y. Zaitsev , S. Zemskova , A. Zghiche

The LVD time stability allows to establish a time-shift in the OPERA experiment, thus providing the first proof against Superluminal neutrinos, using the horizontal muons of the "Teramo Anomaly". This proof is particularly interesting since…

High Energy Physics - Experiment · Physics 2015-06-05 Antonino Zichichi