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Related papers: Neutrino oscillations beyond two flavours

200 papers

A simple model of the neutrino mixing is considered, which contains only one right-handed neutrino field, coupled via the mass term to the three usual left-handed fields. This is a simplest model that allows for three-flavour neutrino…

High Energy Physics - Phenomenology · Physics 2009-10-22 Piotr A. Rcaczka , Andrzej Szymacha , Stanisław Tatur

In the present lectures the following topics are considered: general properties of neutrinos, neutrino mass phenomenology (Dirac and Majorana masses), neutrino masses in the simplest extensions of the standard model (including the seesaw…

High Energy Physics - Phenomenology · Physics 2007-05-23 E. Kh. Akhmedov

Neutrino oscillation experiments provide a unique tool for probing neutrino-matter interactions, especially those involving the tau neutrino. We describe the sensitivity of the present atmospheric neutrino data to these interactions in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Alexander Friedland , Cecilia Lunardini , Michele Maltoni

In this paper I should like to present {\bf {{the four new effects}}} in neutrino oscillations that have been recently investigated in my research group at the Department of Theoretical Physics of the Moscow State University. Due to the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Alexander Studenikin

We study the evolution of the neutrinos system in rotating matter. Neutrinos are supposed to be mixed massive particles interacting with background fermions by means of the electroweak forces. First we find the solutions of wave equations…

High Energy Physics - Phenomenology · Physics 2012-06-04 Maxim Dvornikov

This review is focused on neutrino mixing and neutrino oscillations in the light of the recent experimental developments. After discussing possible types of neutrino mixing for Dirac and Majorana neutrinos and considering in detail the…

High Energy Physics - Phenomenology · Physics 2014-11-17 S. M. Bilenky , C. Giunti , W. Grimus

Global fits to all data of candidates for neutrino oscillations are presented in the framework of a three-flavor model. The analysis excludes mass regions where the MSW effect is important for the solar neutrino problem. The best fit gives…

High Energy Physics - Phenomenology · Physics 2016-08-25 Tommy Ohlsson , Hakan Snellman

The favoured resolution of the atmospheric neutrino anomaly involves an oscillation of the muon neutrino to a different state. Current experiments allow for the latter to contain a significantly large fraction of a non-standard flavour. We…

High Energy Physics - Phenomenology · Physics 2007-05-23 Debajyoti Choudhury , Anindya Datta

The effects of three-flavor neutrino oscillation on the supernova neutrino spectrum are studied. We calculate the expected event rate and energy spectra, and their time evolution at the Superkamiokande (SK) and the Sudbury Neutrino…

High Energy Physics - Phenomenology · Physics 2010-05-28 K. Takahashi , M. Watanabe , K. Sato , T. Totani

Sensitive tests of Lorentz invariance can emerge from the study of neutrino oscillations, particularly for atmospheric neutrinos where the effect is conveniently near-maximal and has been observed over a wide range of energies. We assume…

High Energy Physics - Phenomenology · Physics 2007-05-23 Sheldon Lee Glashow

As was shown previously, oscillations of massless neutrinos may be due to the splitting of multiply degenerate Fermi points. In this Letter, we give the details and propose a three-flavor model of Fermi point splittings and neutrino mixings…

High Energy Physics - Phenomenology · Physics 2009-11-10 F. R. Klinkhamer

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 original B. Pontecorvo idea of neutrino oscillations is discussed. Neutrino mixing and basics of neutrino oscillations in vacuum and in matter are considered. Recent evidences in favour of neutrino oscillations, obtained in…

High Energy Physics - Phenomenology · Physics 2014-11-17 W. M. Alberico , S. M. Bilenky

In this lecture we review some of the basic properties of neutrinos, in particular their mass and the oscillation behavior. First we discuss how to describe the neutrino mass. Then, under the assumption that neutrinos are massive and mixed,…

High Energy Physics - Phenomenology · Physics 2007-05-23 C. W. Kim

Neutrino mixing and basics of neutrino oscillations are considered. Recent evidences in favour of neutrino oscillations, obtained in the solar and atmospheric neutrino experiments, are discussed. Neutrino oscillations in the solar and…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. M. Bilenky

Three interesting scenarios for neutrino mixing, i.e., (i) small-large mixing scenario, (ii) nearly bi-maximal mixing scenario and (iii) three-flavor oscillation scenario, are analyzed in connection with three possible assignments of the…

High Energy Physics - Phenomenology · Physics 2014-11-17 Yue-Liang Wu

We consider three active flavor neutrino oscillations where both the mass-square differences play a role in atmospheric neutrino problem. We calculate the matter effects arising due to propagation through earth. We demonstrate that these…

High Energy Physics - Phenomenology · Physics 2009-11-07 Mohan Narayan , S. Uma Sankar , IIT Bombay

Driven by new experimental results, in the latest period several new neutrino oscillation experiments have been proposed. I will outline the main ideas behind the different proposals, in particular concerning atmospheric neutrinos and…

High Energy Physics - Experiment · Physics 2007-05-23 Mario Campanelli

Following the precise measurement of $\theta_{13}$ by reactor experiments three main questions remain within the now standard picture of neutrino oscillations: (1) Is the value of $\theta_{23}$ such that the $\nu_3$ state contains more muon…

High Energy Physics - Experiment · Physics 2019-08-13 M. D. Messier

I describe the current status of the solar neutrino problem, summarizing the arguments that its resolution will require new particle physics. The phenomenon of matter-enhanced neutrino oscillations is reviewed. I consider the implications…

Nuclear Theory · Physics 2007-05-23 W. C. Haxton