English
Related papers

Related papers: Bimetric Relativity and the Opera Neutrino Experim…

200 papers

Solar, atmospheric, and reactor neutrino experiments have confirmed neutrino oscillations, implying that neutrinos have non-zero mass, but without pinning down their absolute masses. While it is established that the effect of neutrinos on…

Astrophysics · Physics 2010-12-09 Oystein Elgaroy , Ofer Lahav

The study of the neutrinoless double beta ($0 \beta\beta$) decay mode can provide us with important information on the neutrino properties, particularly on the electron neutrino absolute mass. In this work we revise the present constraints…

Nuclear Theory · Physics 2016-11-25 Sabin Stoica , Andrei Neacsu

Einstein's theory of special relativity(SR) and the principle of causality imply that the speed of any moving object can not exceed that of light in a vacuum($c$).However,there were many attempts in literature discussing the particle moving…

High Energy Physics - Phenomenology · Physics 2007-05-23 Guang-jiong Ni

The landmark discovery that neutrinos have mass and can change type (or "flavor") as they propagate -- a process called neutrino oscillation -- has opened up a rich array of theoretical and experimental questions being actively pursued…

High Energy Physics - Experiment · Physics 2025-10-28 NOvA , T2K Collaborations , : , K. Abe , S. Abe , S. Abubakar , M. A. Acero , B. Acharya , P. Adamson , H. Adhkary , R. Akutsu , H. Alarakia-Charles , Y. I. Alj Hakim , S. Alonso Monsalve , N. Anfimov , L. Anthony , A. Antoshkin , S. Aoki , K. A. Apte , T. Arai , T. Arihara , S. Arimoto , E. Arrieta-Diaz , Y. Ashida , L. Asquith , E. T. Atkin , A. Aurisano , D. Azevedo , N. Babu , A. Back , N. Balashov , P. Baldi , B. A. Bambah , E. F. Bannister , V. Baranov , G. J. Barker , G. Barr , A. Barros , D. Barrow , A. Bat , P. Bates , L. Bathe-Peters , M. Batkiewicz-Kwasniak , N. Baudis , K. Bays , V. Berardi , L. Berns , R. Bernstein , T. J. C. Bezerra , V. Bhatnagar , S. Bhattacharjee , B. Bhuyan , J. Bian , A. Blanchet , A. Blondel , P. M. M. Boistier , S. Bolognesi , A. C. Booth , S. Bordoni , R. Bowles , S. B. Boyd , B. Brahma , C. Bromberg , C. Bronner , A. Bubak , N. Buchanan , M. Buizza Avanzini , A. Butkevich , J. A. Caballero , F. Cadoux , N. F. Calabria , S. Calvez , S. Cao , S. Cap , D. Carabadjac , J. M. Carceller , T. J. Carroll , S. L. Cartwright , M. P. Casado , M. G. Catanesi , E. Catano-Mur , J. P. Cesar , J. Chakrani , A. Chalumeau , D. Cherdack , R. Chirco , B. C. Choudhary , A. Christensen , A. Chvirova , M. F. Cicala , T. E. Coan , J. Coleman , G. Collazuol , T. Contreras , A. Cooleybeck , F. Cormier , D. Coveyou , A. A. L. Craplet , L. Cremonesi , A. Cudd , D. D'ago , C. Dalmazzone , T. Daret , P. Dasgupta , G. S. Davies , C. Davis , Yu. I. Davydov , P. de Perio , G. De Rosa , T. Dealtry , C. Densham , A. Dergacheva , P. F. Derwent , R. Dharmapal Banerjee , F. Di Lodovico , G. Diaz Lopez , P. Ding , Z. Djurcic , K. Dobbs , S. Dolan , M. Dolce , D. Douqa , T. A. Doyle , O. Drapier , D. Dueñas Tonguino , K. E. Duffy , E. C. Dukes , J. Dumarchez , P. Dunne , A. Dye , K. Dygnarowicz , A. Eguchi , R. Ehrlich , J. Elias , S. Emery-Schrenk , G. Erofeev , A. Ershova , G. Eurin , E. Ewart , D. Fedorova , S. Fedotov , M. Feltre , L. Feng , D. Ferlewicz , P. Filip , A. J. Finch , M. D. Fitton , C. Forza , M. J. Frank , M. Friend , Y. Fujii , Y. Fukuda , Y. Furui , H. R. Gallagher , J. García-Marcos , A. C. Germer , L. Giannessi , C. Giganti , M. Girgus , A. Giri , V. Glagolev , R. A. Gomes , M. Gonin , R. González Jiménez , J. González Rosa , E. A. G. Goodman , M. C. Goodman , K. Gorshanov , P. Govindaraj , M. Grassi , R. Group , M. Guigue , F. Y. Guo , A. Habig , D. R. Hadley , F. Hakl , S. Han , D. A. Harris , R. J. Harris , J. Hartnell , T. Hasegawa , C. M. Hasnip , S. Hassani , N. C. Hastings , R. Hatcher , Y. Hayato , J. M. Hays , M. He , I. Heitkamp , K. Heller , D. Henaff , V Hewes , A. Himmel , Y. Hino , J. Holeczek , A. Holin , T. Holvey , N. T. Hong Van , T. Honjo , M. C. F. Hooft , T. Horoho , K. Hosokawa , J. Hu , A. K. Ichikawa , K. Ieki , M. Ikeda , T. Ishida , M. Ishitsuka , A. Ivanova , A. Izmaylov , N. Jachowicz , B. Jargowsky , S. J. Jenkins , C. Jesús-Valls , J. Y. Ji , M. Jia , J. J. Jiang , T. P. Jones , P. Jonsson , S. Joshi , C. K. Jung , M. Kabirnezhad , A. C. Kaboth , I. Kakorin , H. Kakuno , A. Kalitkina , J. Kameda , D. M. Kaplan , S. Karpova , V. S. Kasturi , Y. Kataoka , T. Katori , Y. Kawamura , M. Kawaue , E. Kearns , M. Khabibullin , A. Khanam , A. Khotjantsev , T. Kikawa , S. King , B. Kirezli , V. Kiseeva , J. Kisiel , J. Kleykamp , O. Klimov , A. Klustová , L. Kneale , H. Kobayashi , L. Koch , S. Kodama , L. W. Koerner , L. Kolupaeva , M. Kolupanova , A. Konaka , L. L. Kormos , Y. Koshio , K. Kowalik , R. Kralik , Y. Kudenko , Y. Kudo , A. Kumar , A. Kumar Jha , R. Kurjata , V. Kurochka , C. D. Kuruppu , V. Kus , T. Kutter , L. Labarga , M. Lachat , K. Lachner , T. Lackey , J. Lagoda , S. M. Lakshmi , M. Lamers James , K. Lang , A. Langella , D. H. Langridge , J. -F. Laporte , P. Lasorak , D. Last , N. Latham , M. Laveder , L. Lavitola , M. Lawe , D. Leon Silverio , J. Lesmeister , S. Levorato , S. V. Lewis , B. Li , W. Li , C. Lin , A. Lister , R. P. Litchfield , J. Liu , S. L. Liu , J. A. Lock , A. Longhin , A. Lopez Moreno , X. Lu , L. Ludovici , T. Lux , L. N. Machado , M. MacMahon , L. Magaletti , S. Magill , K. Mahn , K. K. Mahtani , M. Mandal , S. Manly , W. A. Mann , M. T. Manoharan , M. Manrique Plata , A. D. Marino , M. L. Marshak , D. G. R. Martin , L. Martinez , D. A. Martinez Caicedo , M. Martinez-Casales , M. Martini , T. Matsubara , R. Matsumoto , V. Matveev , C. Mauger , K. Mavrokoridis , N. McCauley , K. S. McFarland , C. McGrew , J. McKean , A. Mefodiev , G. D. Megias , B. Mehta , L. Mellet , M. D. Messier , C. Metelko , H. Meyer , M. Mezzetto , T. Miao , S. Miki , V. Mikola , E. W. Miller , W. H. Miller , A. Minamino , S. Mine , O. Mineev , J. Mirabito , S. R. Mishra , M. Miura , R. Mohanta , A. Moren , S. Moriyama , S. Moriyama , A. Morozova , P. Morrison , W. Mu , L. Mualem , Th. A. Mueller , M. Muether , K. Mulder , D. Munford , A. Muñoz , L. Munteanu , D. Myers , Y. Nagai , T. Nakadaira , K. Nakagiri , M. Nakahata , Y. Nakajima , K. D. Nakamura , Y. Nakano , T. Nakaya , S. Nakayama , K. Nakayoshi , D. Naples , C. E. R. Naseby , S. Nelleri , J. K. Nelson , D. T. Nguyen , V. Q. Nguyen , R. Nichol , K. Niewczas , E. Niner , S. Nishimori , Y. Nishimura , Y. Noguchi , A. Norman , A. Norrick , T. Nosek , F. Nova , J. C. Nugent , H. Oh , R. Okazaki , H. M. O'Keeffe , W. Okinaga , K. Okumura , T. Okusawa , A. Olshevskiy , T. Olson , N. Onda , N. Ospina , L. Osu , L. O'Sullivan , Y. Oyama , M. Ozkaynak , A. Pal , J. Paley , L. Panda , V. Paolone , J. Pasternak , R. B. Patterson , G. Pawloski , D. Payne , T. Peacock , R. Petti , M. Pfaff , L. Pickering , R. K. Plunkett , B. Popov , J. C. C. Porter , A. J. Portocarrero Yrey , M. Posiadala-Zezula , Y. S. Prabhu , L. R. Prais , H. Prasad , F. Pupilli , B. Quilain , P. T. Quyen , E. Radicioni , B. Radics , A. Rafique , V. Raj , M. Rajaoalisoa , M. A. Ramirez , R. Ramsden , B. Ramson , P. N. Ratoff , B. Rebel , M. Reh , G. Reina , C. Riccio , D. W. Riley , E. Robles , E. Rondio , S. Roth , N. Roy , P. Roy , A. Rubbia , L. Russo , A. Rychter , W. Saenz , K. Sakashita , S. Samani , O. Samoylov , M. C. Sanchez , F. Sánchez , S. Sánchez Falero , E. M. Sandford , Y. Sato , T. Schefke , C. M. Schloesser , K. Scholberg , M. Scott , Y. Seiya , T. Sekiguchi , H. Sekiya , T. Sekiya , D. Seppala , D. Sgalaberna , A. Shaikhiev , P. Shanahan , P. Sharma , A. Sheshukov , M. Shiozawa , Y. Shiraishi , Shivam , A. Shmakov , W. Shorrock , S. Shukla , A. Shvartsman , I. Singh , P. Singh , V. Singh , S. Singh Chhibra , D. K. Singha , N. Skrobova , K. Skwarczynski , A. Smith , J. Smolik , M. Smy , D. Smyczek , P. Snopok , J. T. Sobczyk , H. Sobel , F. J. P. Soler , N. Solomey , A. Sousa , K. Soustruznik , A. J. Speers , R. Spina , A. Srivastava , P. Stowell , M. Strait , Y. Stroke , I. A. Suslov , L. Suter , A. Sutton , K. Sutton , A. Suzuki , S. Y. Suzuki , S. Swain , C. Sweeney , A. Sztuc , M. Tada , S. Tairafune , A. Takeda , Y. Takeuchi , N. Talukdar , H. K. Tanaka , H. Tanigawa , P. Tas , A. Teklu , V. V. Tereshchenko , T. Thakore , N. Thamm , J. Thomas , E. Tiras , M. Titus , Y. Torun , C. Touramanis , D. Tran , N. Tran , J. Trokan-Tenorio , T. Tsukamoto , M. Tzanov , Y. Uchida , J. Urheim , M. Vagins , P. Vahle , Z. Vallari , M. Varghese , I. Vasilyev , G. Vasseur , E. Villa , U. Virginet , T. Vladisavljevic , K. J. Vockerodt , T. Wachala , D. Wakabayashi , A. V. Waldron , H. T. Wallace , M. Wallbank , J. G. Walsh , L. Wan , T. K. Warburton , D. Wark , M. O. Wascko , A. Weber , C. Weber , R. Wendell , M. Wetstein , D. Whittington , D. A. Wickremasinghe , M. J. Wilking , C. Wilkinson , J. R. Wilson , J. Wolcott , K. Wood , C. Wret , S. Wu , W. Wu , W. Wu , J. Xia , Y. Xiao , B. Yaeggy , A. Yahaya , K. Yamamoto , T. Yamamoto , C. Yanagisawa , Y. Yang , A. Yankelevich , T. Yano , N. Yershov , U. Yevarouskaya , M. Yokoyama , K. Yonehara , Y. Yoshimoto , N. Yoshimura , S. Zadorozhnyy , R. Zaki , J. Zalesak , A. Zalewska , J. Zalipska , G. Zarnecki , J. Zhang , X. Y. Zhao , H. Zheng , H. Zhong , T. Zhu , M. Ziembicki , E. D. Zimmerman , M. Zito , S. Zsoldos , R. Zwaska

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

The aim of the OPERA experiment is to search for the appearance of the tau neutrino in the quasi pure muon neutrino beam produced at CERN (CNGS). The detector, installed in the Gran Sasso underground laboratory 730 km away from CERN,…

High Energy Physics - Experiment · Physics 2007-06-13 J. Marteau

A particular Fermi-point-splitting (FPS) model is proposed, which allows, for finite values of the three-momentum, the group and phase velocities of the muon-flavor neutrino in vacuum to be superluminal (i.e., muon-neutrino velocities…

High Energy Physics - Phenomenology · Physics 2011-10-04 F. R. Klinkhamer

Thanks to oscillation experiments it is now an established fact that neutrinos are massive particles. Yet, the assessment of neutrinos absolute mass scale is still an outstanding challenge in particle physics and cosmology as oscillation…

Instrumentation and Detectors · Physics 2017-06-28 Andrea Giachero

The oscillations of ultra-relativistic neutrinos are realized by the propagation of assumed zero-mass on-shell neutrinos with the speed of light in vacuum combined with the phase modulation by the small mass term…

High Energy Physics - Phenomenology · Physics 2024-05-08 Kazuo Fujikawa

Bimetric gravity is a ghost-free and observationally viable extension of general relativity, exhibiting both a massless and a massive graviton. The observed abundances of light elements can be used to constrain the expansion history of the…

Cosmology and Nongalactic Astrophysics · Physics 2021-11-04 Marcus Högås , Edvard Mörtsell

If neutrinos have a small but non-zero mass, time-of-flight effects for neutrino bursts from distant sources can yield information on the large-scale geometry of the universe, the effects being proportional to the integral over time of the…

Astrophysics · Physics 2009-10-31 Leo Stodolsky

Two neutrino double $\beta$ decay can create irremovable background even in high energy resolution detectors searching for neutrinoless double $\beta$ decay due to random coincidence of $2\nu2\beta$ events in case of poor time resolution.…

Instrumentation and Detectors · Physics 2013-01-21 D. M. Chernyak , F. A. Danevich , A. Giuliani , E. Olivieri , M. Tenconi , V. I. Tretyak

In this paper, we consider the problem of quantum measurement of neutrino velocity. We show, that the well known neutrino flavor oscillations are always accompanied by the oscillations of neutrino velocity. In particular, the velocity of a…

High Energy Physics - Phenomenology · Physics 2015-04-02 Branislav Sazdović , Milovan Vasilić

In the OPERA experiment, the time of arrival of the neutrino light curve at LNGS is defined by a best-fit to the generating proton PDF at CERN. By a two parameter matched filtering procedure, we determine that the OPERA neutrino light curve…

High Energy Physics - Experiment · Physics 2011-10-24 Maurice H. P. M. van Putten

Neutrinoless double beta ($0\nu\beta\beta$) decay, an important low-energy process, serves not only as a potential test of the Majorana nature of neutrinos, but also as a sensitive probe for new physics beyond the Standard Model. In this…

High Energy Physics - Phenomenology · Physics 2025-10-10 Vivek Banerjee , Sasmita Mishra

We consider Lorentz- and CPT-violating dimension-5 operators to address the issue of superluminal neutrinos recently pointed out in OPERA experiments. We assume these operators in the photon and neutrino sectors coupled to Lorentz-violating…

High Energy Physics - Phenomenology · Physics 2015-06-03 C. A. G. Almeida , M. A. Anacleto , F. A. Brito , E. Passos

The results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed. The data concern different event topologies with average neutrino energies of ~ 4 and ~ 50 GeV. The Multiple Coulomb Scattering of muons…

High Energy Physics - Experiment · Physics 2019-08-14 G. Giacomelli

We examine the performance of the six-parameter $\Lambda$CDM model and its extensions in light of recent cosmological observations, with particular focus on neutrino properties inferred from cosmology. Using a broad suite of nine…

Cosmology and Nongalactic Astrophysics · Physics 2025-02-12 Helena García Escudero , Kevork N. Abazajian

Neutrinoless double-$\beta$ decay ($0\nu\beta\beta$ decay) is a hypothetical process that can occur if the neutrino is its own antiparticle. The COBRA collaboration operates a demonstrator to search for these decays at the Laboratori…

We discuss the possibility that the limiting speed (c_l) appearing in Lorentz equations might be different i.e., slightly larger than the observed speed of light (c_n). We show that such a possibility can be tested by state-of-the-art…

High Energy Physics - Phenomenology · Physics 2015-06-04 Jean-Marie Frere , Simon Mollet , Michel H. G. Tytgat