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Recent experiments have led to the production of neutrinos with transit times indicating the appearance of traveling faster than the speed of light. In this paper, we present a conceptual framework to understand how faster-than-light events…

General Physics · Physics 2012-03-15 Eric Sakk , Aradhya P. Kumar

It has been recently suggested by Dvali and Vikman that the superluminal neutrino phenomenology of the OPERA experiment may be due to an environmental feature of the Earth, naturally yielding a long-range fifth force of gravitational origin…

General Relativity and Quantum Cosmology · Physics 2015-03-19 Lorenzo Iorio

The OPERA experiment is based on a hybrid technology combining electronic detectors and nuclear emulsions. OPERA collected muon-neutrino interactions during the 2008 and 2009 physics runs of the CNGS neutrino beam, produced at CERN with an…

High Energy Physics - Experiment · Physics 2012-08-27 OPERA Collaboration

The RENO experiment recently reported the disappearance of reactor electron antineutrinos consistent with neutrino oscillations, with a significance of 4.9 standard deviations. The published ratio of observed to expected number of…

The claims that the GSI time anomaly is due to the mixing of neutrinos in the final state of the observed electron-capture processes are refuted. With the help of an analogy with a double-slit experiment, it is shown that the standard…

High Energy Physics - Phenomenology · Physics 2009-04-17 Carlo Giunti

We discuss different schemes of neutrino oscillations and the time-energy uncertainty relation. From the results of the K2K and MINOS accelerator experiments follows that neutrino oscillations are a non-stationary phenomenon and that the…

High Energy Physics - Phenomenology · Physics 2009-03-31 S. M. Bilenky , F. von Feilitzsch , W. Potzel

In this report a potential problem in the data analysis of the OPERA experiment is discussed: the main issue is that the quantity \partial t used in the maximum likelihood procedure is not a "true" parameter of the parent-distribution…

High Energy Physics - Experiment · Physics 2011-11-08 Pierluigi Frabetti , Leonid Chernenko

Probably not.

High Energy Physics - Phenomenology · Physics 2015-05-30 M. V. Berry , N. Brunner , S. Popescu , P. Shukla

In this work we consider a possible conceptual similarity between recent, amazing OPERA experiment of the superluminal propagation of neutrino and experiment of the gain-assisted superluminal light propagation realized about ten years ago.…

General Physics · Physics 2011-10-04 Vladan Pankovic

Neutrino oscillations in a core-collapse supernova may be responsible for the observed rapid motions of pulsars. Three-dimensional numerical calculations show that, in the absence of neutrino oscillations, the recoil velocities of neutron…

Astrophysics · Physics 2016-12-07 Alexander Kusenko

Oscillations in the electron-capture (EC) decay rate observed in storage-ring experiments are reconsidered in connection with the neutrino mass difference. Taking into account that - according to Relativity Theory - time is slowed down in…

High Energy Physics - Phenomenology · Physics 2015-01-21 Walter Potzel

Examining a catalogue of isolated galaxy pairs, a preferred orbital intervelocity of ~150 km/s was recently reported. This discovery is difficult to reconcile with the expectations from Newtonian numerical simulations of cosmological…

Astrophysics of Galaxies · Physics 2022-06-05 Riccardo Scarpa , Renato Falomo , Aldo Treves

The claim of a neutrino velocity different from the speed of the light, made in September 2001 by the Opera experiment, suggested the study of the time delays between TeV underground muons in the Gran Sasso laboratory using the old data of…

High Energy Physics - Experiment · Physics 2012-09-14 Francesco Ronga

We have estimated the number flux of of mu-neutrinos which are produced due to the hadronic interactions between the cosmic rays coming from a neutron star and the matter in a companion star. The event rate at 1 km^2 detectors of…

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

According to the theory of ether light propagates with constant speed c with respect to the absolute reference frame and with respect to any other reference frame the speed of light is covariant. According to the theory of special…

General Physics · Physics 2010-03-12 Daniele Sasso

We discuss the prospects for improved upper limits on neutrino masses that may be provided by a core-collapse supernova explosion in our galaxy, if it exhibits time variations in the neutrino emissions on the scale of a few milliseconds as…

High Energy Physics - Phenomenology · Physics 2013-05-30 John Ellis , Hans-Thomas Janka , Nikolaos E. Mavromatos , Alexander S. Sakharov , Edward K. G. Sarkisyan

While the OPERA experimental scrutiny is ongoing in the community, in the present article we construct a toy model of {\it extended Lorentz code} (ELC) of the uniform motion, which will be a well established consistent and unique…

General Physics · Physics 2013-03-07 G. Ter-Kazarian

We performed a detailed analysis and the Monte Carlo simulation of the neutron lifetime experiment [S. Arzumanov et al., Phys. Lett. B 483 (2000) 15] because of the strong disagreement by 5.6 standard deviations between the results of this…

Nuclear Experiment · Physics 2014-11-21 A. K. Fomin , A. P. Serebrov

OPERA collaboration has reported evidence of superluminal phenomenon for neutrinos. One of the possible ways to explain the superluminality is to have Lorentz symmetry violated. It has been shown that dispersion relations put forwards has…

High Energy Physics - Phenomenology · Physics 2015-06-03 Gang Guo , Xiao-Gang He

Lorentz invariance is a fundamental symmetry of spacetime and foundational to modern physics. One of its most important consequences is the constancy of the speed of light. This invariance, together with the geometry of spacetime, implies…

High Energy Astrophysical Phenomena · Physics 2025-02-26 KM3NeT Collaboration , O. Adriani , S. Aiello , A. Albert , A. R. Alhebsi , M. Alshamsi , S. Alves Garre , A. Ambrosone , F. Ameli , M. Andre , L. Aphecetche , M. Ardid , S. Ardid , C. Argüelles , J. Aublin , F. Badaracco , L. Bailly-Salins , Z. Bardačová , A. Bariego-Quintana , Y. Becherini , M. Bendahman , F. Benfenati Gualandi , M. Benhassi , M. Bennani , D. M. Benoit , E. Berbee , E. Berti , V. Bertin , P. Betti , S. Biagi , M. Boettcher , D. Bonanno , S. Bottai , A. B. Bouasla , J. Boumaaza , M. Bouta , M. Bouwhuis , C. Bozza , R. M. Bozza , H. Brânzaş , F. Bretaudeau , M. Breuhaus , R. Bruijn , J. Brunner , R. Bruno , E. Buis , R. Buompane , J. Busto , B. Caiffi , D. Calvo , A. Capone , F. Carenini , V. Carretero , T. Cartraud , P. Castaldi , V. Cecchini , S. Celli , L. Cerisy , M. Chabab , A. Chen , S. Cherubini , T. Chiarusi , M. Circella , R. Clark , R. Cocimano , J. A. B. Coelho , A. Coleiro , A. Condorelli , R. Coniglione , P. Coyle , A. Creusot , G. Cuttone , R. Dallier , A. De Benedittis , G. De Wasseige , V. Decoene , P. Deguire , I. Del Rosso , L. S. Di Mauro , I. Di Palma , A. F. Díaz , D. Diego-Tortosa , C. Distefano , A. Domi , C. Donzaud , D. Dornic , E. Drakopoulou , D. Drouhin , J. -G. Ducoin , P. Duverne , R. Dvornický , T. Eberl , E. Eckerová , A. Eddymaoui , T. van Eeden , M. Eff , D. van Eijk , I. El Bojaddaini , S. El Hedri , S. El Mentawi , V. Ellajosyula , A. Enzenhöfer , G. Ferrara , M. D. Filipović , F. Filippini , D. Franciotti , L. A. Fusco , S. Gagliardini , T. Gal , J. García Méndez , A. Garcia Soto , C. Gatius Oliver , N. Geißelbrecht , E. Genton , H. Ghaddari , L. Gialanella , B. K. Gibson , E. Giorgio , I. Goos , P. Goswami , S. R. Gozzini , R. Gracia , C. Guidi , B. Guillon , M. Gutiérrez , C. Haack , H. van Haren , A. Heijboer , L. Hennig , J. J. Hernández-Rey , A. Idrissi , W. Idrissi Ibnsalih , G. Illuminati , O. Janik , D. Joly , M. de Jong , P. de Jong , B. J. Jung , P. Kalaczyński , N. Kamp , J. Keegans , V. Kikvadze , G. Kistauri , C. Kopper , A. Kouchner , Y. Y. Kovalev , L. Krupa , V. Kueviakoe , V. Kulikovskiy , R. Kvatadze , M. Labalme , R. Lahmann , M. Lamoureux , G. Larosa , C. Lastoria , J. Lazar , A. Lazo , S. Le Stum , G. Lehaut , V. Lemaître , E. Leonora , N. Lessing , G. Levi , M. Lindsey Clark , F. Longhitano , F. Magnani , J. Majumdar , L. Malerba , F. Mamedov , A. Manfreda , A. Manousakis , M. Marconi , A. Margiotta , A. Marinelli , C. Markou , L. Martin , M. Mastrodicasa , S. Mastroianni , J. Mauro , K. C. K. Mehta , A. Meskar , G. Miele , P. Migliozzi , E. Migneco , M. L. Mitsou , C. M. Mollo , L. Morales-Gallegos , N. Mori , A. Moussa , I. Mozun Mateo , R. Muller , M. R. Musone , M. Musumeci , S. Navas , A. Nayerhoda , C. A. Nicolau , B. Nkosi , B. Ó Fearraigh , V. Oliviero , A. Orlando , E. Oukacha , L. Pacini , D. Paesani , J. Palacios González , G. Papalashvili , P. Papini , V. Parisi , A. Parmar , E. J. Pastor Gomez , C. Pastore , A. M. Păun , G. E. Păvălaş , S. Peña Martínez , M. Perrin-Terrin , V. Pestel , R. Pestes , M. Petropavlova , P. Piattelli , A. Plavin , C. Poirè , V. Popa , T. Pradier , J. Prado , S. Pulvirenti , C. A. Quiroz-Rangel , N. Randazzo , A. Ratnani , S. Razzaque , I. C. Rea , D. Real , G. Riccobene , J. Robinson , A. Romanov , E. Ros , A. Šaina , F. Salesa Greus , D. F. E. Samtleben , A. Sánchez Losa , S. Sanfilippo , M. Sanguineti , D. Santonocito , P. Sapienza , M. Scaringella , M. Scarnera , J. Schnabel , J. Schumann , H. M. Schutte , J. Seneca , N. Sennan , P. A. Sevle Myhr , I. Sgura , R. Shanidze , A. Sharma , Y. Shitov , F. Šimkovic , A. Simonelli , A. Sinopoulou , B. Spisso , M. Spurio , O. Starodubtsev , D. Stavropoulos , I. Štekl , D. Stocco , M. Taiuti , G. Takadze , Y. Tayalati , H. Thiersen , S. Thoudam , I. Tosta e Melo , B. Trocmé , V. Tsourapis , E. Tzamariudaki , A. Ukleja , A. Vacheret , V. Valsecchi , V. Van Elewyck , G. Vannoye , E. Vannuccini , G. Vasileiadis , F. Vazquez de Sola , A. Veutro , S. Viola , D. Vivolo , A. van Vliet , A. Y. Wen , E. de Wolf , I. Lhenry-Yvon , S. Zavatarelli , A. Zegarelli , D. Zito , J. D. Zornoza , J. Zúñiga , N. Zywucka
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