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Theory suggests the existence of neutrino masses, but little more. Facts are coming close to reveal our fantasy: solar and atmospheric neutrino data strongly indicate the need for neutrino conversions, while LSND provides an intriguing…

High Energy Physics - Phenomenology · Physics 2009-09-17 J. W. F. Valle

Neutrinos are neutral, spin-$\frac{1}{2}$ particles which undergo only weak interactions. The experimentally observed phenomenon of neutrino oscillation establishes the fact that neutrinos are massive and there is mixing between different…

High Energy Physics - Phenomenology · Physics 2016-03-16 Monojit Ghosh

The mixing of three and four massive neutrinos is considered. It is shown that the neutrino oscillation data are not compatible with a hierarchy of couplings in the three-neutrino case. In the case of four neutrinos, a hierarchy of masses…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. M. Bilenky , C. Giunti , W. Grimus

Inspired by the neutrino oscillations data, we consider the exact $\mu-\tau$ symmetry, implemented at the level of the neutrino mass matrix, as a good initial framework around which to study and describe neutrino phenomenology. Working in…

High Energy Physics - Phenomenology · Physics 2021-07-14 N. Chamoun , C. Hamzaoui , S. Lashin , S. Nasri , M. Toharia

Proposed medium-baseline reactor neutrino experiments offer unprecedented opportunities to probe, at the same time, the mass-mixing parameters which govern $\nu_e$ oscillations both at short wavelength (delta m^2 and theta_{12}) and at long…

High Energy Physics - Phenomenology · Physics 2014-01-15 F. Capozzi , E. Lisi , A. Marrone

A revolution in our understanding of the neutrino sector is underway, driven by observations that are interpreted in terms of changes in neutrino flavors as they propagate. Since neutrino oscillations occur only if neutrinos are massive,…

High Energy Physics - Phenomenology · Physics 2007-05-23 V. Barger , K. Whisnant

Neutrino oscillations change when in media in comparison to vacuum oscillations due to the scattering of neutrinos on matter constituents, electrons particularly. This can be easily described by introducing new effective matter mixing…

High Energy Physics - Phenomenology · Physics 2018-10-02 Tomas Nosek

We discuss which information on neutrino masses and mixing can be obtained from the results of all neutrino oscillation experiments in the cases of three and four massive neutrinos. We show that in the three-neutrino case the neutrino…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. M. Bilenky , C. Giunti , W. Grimus

Neutrino oscillations reveal several small parameters, namely, $\theta_{13}$, the solar mass splitting {\em vis-\`{a}-vis} the atmospheric one, and the deviation of $\theta_{23}$ from maximal mixing. Can these small quantities all be traced…

High Energy Physics - Phenomenology · Physics 2015-05-27 Soumita Pramanick , Amitava Raychaudhuri

I review the interpretation of solar and atmospheric neutrino data in terms neutrino oscillations and describe some ways to account for the required neutrino masses and mixing angles from first principles, both within top-down and bottom-up…

High Energy Physics - Phenomenology · Physics 2009-09-17 J. W. F. Valle

Neutrino oscillations data indicates that neutrino mixings are consistent with an apparent $\nu_\mu - \nu_\tau$ exchange symmetry in neutrino mass matrix. We observe that in the mininimally extended standard model with the see-saw…

High Energy Physics - Phenomenology · Physics 2008-11-26 Juan Carlos Gómez-Izquierdo , Abdel Pérez-Lorenzana

We suggest an approach to explain the observed pattern of the neutrino masses and mixing which employs the weakly broken quark-lepton symmetry and does not require introduction of an ad hoc symmetry of the neutrino sector. The mass matrices…

High Energy Physics - Phenomenology · Physics 2009-11-10 I. Dorsner , A. Yu. Smirnov

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

In this talk I review the present status of neutrino masses and mixing and some of their implications for particle physics phenomenology. I first discuss the minimum extension of the Standard Model of particle physics required to…

High Energy Physics - Phenomenology · Physics 2009-11-10 M. C. Gonzalez-Garcia

We construct a model that allows us to determine the three neutrino masses directly from the experimental mass squared differences, $\Delta_{\rm atm}$ and $\Delta_{\rm sol}$, together with the assumption that $\Lambda = \surd (1/6) = \surd…

High Energy Physics - Phenomenology · Physics 2007-05-23 Peter Kaus , Sydney Meshkov

We present a new global fit of neutrino oscillation parameters within the simplest three-neutrino picture, including new data which appeared since our previous analysis~\cite{Forero:2014bxa}. In this update we include new long-baseline…

High Energy Physics - Phenomenology · Physics 2018-06-20 P. F. de Salas , D. V. Forero , C. A. Ternes , M. Tortola , J. W. F. Valle

Maximum mixing in atmospheric neutrino oscillation, as well as vanishing of the MNS matrix element $U_{e3}$, are consequences of a 2-3 symmetry, under which the neutrino mass matrix is invariant under the interchange of second and third…

High Energy Physics - Phenomenology · Physics 2009-11-07 C. S. Lam

We study the link between neutrino oscillations and leptogenesis in the minimal framework assuming an SO(10) see-saw mechanism with 3 families. Dirac neutrino masses being fixed, the solar and atmospheric data then generically induce a…

High Energy Physics - Phenomenology · Physics 2009-10-31 Emmanuel Nezri , Jean Orloff

This work explores the possibility of resorting to neutrino phenomenology to detect evidence of new physics, caused by the residual signals of the supposed quantum structure of spacetime. In particular, this work investigates the effects on…

High Energy Physics - Phenomenology · Physics 2021-10-19 Marco Danilo Claudio Torri

Recent works combining neutrino oscillation and cosmological data to determine the neutrino hierarchy found a range of odds in favour of the normal hierarchy. These results arise from differing approaches to incorporating prior knowledge…

Cosmology and Nongalactic Astrophysics · Physics 2020-04-15 Constance Mahony , Boris Leistedt , Hiranya V. Peiris , Jonathan Braden , Benjamin Joachimi , Andreas Korn , Linda Cremonesi , Ryan Nichol