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This essay is intended to provide a brief description of the peculiar properties of neutrinos within and beyond the standard theory of weak interactions. The focus is on the flavor oscillations of massive neutrinos, from which one has…

High Energy Physics - Phenomenology · Physics 2016-10-12 Yifang Wang , Zhi-zhong Xing

Neutrino physics is going through a revolutionary progress. In this talk I review what we have learned and why neutrino mass is so important. Neutrino masses and mixings are already shedding new insight into the origin of flavor. Given the…

High Energy Physics - Phenomenology · Physics 2009-09-29 Hitoshi Murayama

Certainly one of the most exciting areas of research at present is neutrino physics. The neutrinos are fantastically numerous in the universe and as such they have bearing on our understanding of the universe. Therefore, we must understand…

High Energy Physics - Phenomenology · Physics 2007-05-23 Riazuddin

The question of neutrino mass is one of the major riddles in particle physics. Recently, strong evidence that neutrinos have nonzero masses has been found. While tiny, these masses could be large enough to contribute significantly to the…

High Energy Physics - Phenomenology · Physics 2008-12-18 Peter Fisher , Boris Kayser , Kevin S. McFarland

Phenomenological implications of neutrino oscillations implied by recent experimental data on pattern of neutrino mass matrix are disscussed. It is shown that it is possible to have a neutrino mass matrix which shows approximate flavor…

High Energy Physics - Phenomenology · Physics 2009-11-10 Riazuddin

An extension of the New Standard Model, by introducing a mixing of the low mass ``active'' neutrinos with heavy ones, or by any model with lepton flavor violation, is considered. This leads to non-orthogonal neutrino production and…

High Energy Physics - Phenomenology · Physics 2008-11-26 J. Holeczek , J. Kisiel , J. Syska , M. Zralek

The recent observation of neutrino oscillations with atmospheric and solar neutrinos, implying that neutrinos are not massless, is a discovery of paramount importance for particle physics and particle astrophysics. This invited lecture…

High Energy Physics - Experiment · Physics 2017-08-23 N. Schmitz

Thanks to compelling evidence that neutrinos can change flavor, we now know that they have nonzero masses, and that leptons mix. In these lectures, we explain the physics of neutrino flavor change, both in vacuum and in matter. Then, we…

High Energy Physics - Phenomenology · Physics 2008-11-26 Boris Kayser

The discovery of neutrino oscillations and the large mixing parameters in the Pontecorvo Maki Nakagawa Sakata matrix has opened a window to search for CP-violation in neutrinos. Two long-baseline neutrino experiments, DUNE and…

High Energy Physics - Experiment · Physics 2022-07-18 Blair Jamieson

The Standard Model of particle physics describes neutrinos as massless, chargeless elementary particles that come in three different flavours. However, recent experiments indicate that neutrinos not only have mass, but also have multiple…

General Physics · Physics 2015-11-23 Spandan Mondal

Neutrino oscillation phenomenon is a definite evidence of physics beyond the Standard Model (SM) and high precision measurement of neutrino properties will certainly give us clue about what lies beyond the SM. In particular, precise…

High Energy Physics - Phenomenology · Physics 2023-06-01 Chee Sheng Fong

We examine the physics capabilities of known flavor neutrino beams from intense muon sources. We find that long-baseline neutrino experiments based on such beams can provide precise measurements of neutrino oscillation mass and mixing…

High Energy Physics - Phenomenology · Physics 2009-09-25 V. Barger , S. Geer , K. Whisnant

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 fact that neutrinos have mass allows them to possess many other properties, like a magnetic dipole moment and a finite decay width. Theoretical expectations for these are, however, well beyond current experimental bounds, and the…

High Energy Physics - Phenomenology · Physics 2009-11-10 Andre de Gouvea

We critically examine the ability of future neutrino telescopes, including Baikal-GVD, KM3NeT, P-ONE, TAMBO, and IceCube-Gen2, to determine the flavor composition of high-energy astrophysical neutrinos, ie, the relative number of $\nu_e$,…

High Energy Physics - Phenomenology · Physics 2021-04-28 Ningqiang Song , Shirley Weishi Li , Carlos A. Argüelles , Mauricio Bustamante , Aaron C. Vincent

The fundamental properties of the lepton sector include the neutrino masses and flavor mixings. Both are difficult to observe because of the extremely small neutrino masses and neutrino-matter cross sections. In these lectures, we focus on…

High Energy Physics - Phenomenology · Physics 2010-12-13 Walter Winter

We investigate the indications of flavor oscillations that come from the anomalous flavor composition of the atmospheric neutrino flux observed in some underground experiments. We study the information coming from the neutrino-induced…

High Energy Physics - Phenomenology · Physics 2009-10-07 G. L. Fogli , E. Lisi , D. Montanino , G. Scioscia

Understanding the physics of neutrinos is of paramount relevance for the development of high energy physics, cosmology and astrophysics, thanks to their characteristics and phenomenology. In particular, the property of changing flavor while…

High Energy Physics - Experiment · Physics 2018-12-13 Mario A. Acero

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

We review long-baseline neutrino experiments in which neutrinos are detected after traversing macroscopic distances. Over such distances neutrinos have been found to oscillate among flavor states. Experiments with solar, atmospheric,…

High Energy Physics - Experiment · Physics 2016-08-23 M. V. Diwan , V. Galymov , X. Qian , A. Rubbia
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