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We revisit correlations of neutrino oscillation parameters in reactor and long-baseline neutrino oscillation experiments. A framework based on an effective value of $\theta_{13}$ is presented, which can easily reproduce experimental…

High Energy Physics - Phenomenology · Physics 2018-04-25 Manfred Lindner , Werner Rodejohann , Xun-Jie Xu

This article describes an optimal method (conflation) to consolidate data from different experiments, and illustrates the advantages of conflation by graphical examples involving gaussian input distributions, and by a concrete numerical…

Data Analysis, Statistics and Probability · Physics 2009-02-02 Theodore P. Hill , Jack Miller

We show that the Frobenius group $T_{13} = Z_{13} \rtimes Z_3$ is a suitable family symmetry group to study neutrino oscillations. Our approach is to catalog all possibilities within an effective field theory approach, assuming only…

High Energy Physics - Phenomenology · Physics 2011-09-07 Christine Hartmann , A. Zee

The MINOS experiment observes the NuMI beam produced by the Main Injector accelerator at two detector stations, one 1 km and the other 735 km from the neutrino production target. From the disappearance of neutrinos in flight between the two…

High Energy Physics - Experiment · Physics 2019-08-13 Patricia Vahle

Neutrino interactions recorded in a 5.1 fiducial kiloton-year exposure of the Soudan-2 iron tracking calorimeter are analyzed for effects of neutrino oscillations. Using contained single track and single shower events, we update our…

High Energy Physics - Experiment · Physics 2009-10-31 W. Anthony Mann

We present an updated global fit of neutrino oscillation data in the simplest three-neutrino framework. In the present study we include up-to-date analyses from a number of experiments. Concerning the atmospheric and solar sectors, we give…

High Energy Physics - Phenomenology · Physics 2021-02-12 P. F. de Salas , D. V. Forero , S. Gariazzo , P. Martínez-Miravé , O. Mena , C. A. Ternes , M. Tórtola , J. W. F. Valle

We present a framework for the analysis of data from neutrino oscillation experiments. The framework performs a profile likelihood fit and employs a forward-folding technique to optimize its model with respect to the oscillation parameters.…

Computational Physics · Physics 2025-07-03 Denise Hellwig , Stefan Schoppmann , Philipp Soldin , Achim Stahl , Christopher Wiebusch

Up to now, future neutrino beam experiments have been designed and optimized in order to look for CP violation, \theta_{13} and the mass hierarchy under the conservative assumption that \theta_{13} is very small. However, the recent results…

High Energy Physics - Phenomenology · Physics 2015-05-30 Pilar Coloma , Enrique Fernandez-Martinez

We propose a novel neutrino mixing pattern in terms of only two small integers 1 and 2 together with their square roots and the imaginary number $i$. This ansatz is referred to as the "tetra-maximal" mixing because it can be expressed as a…

High Energy Physics - Phenomenology · Physics 2008-11-26 Zhi-zhong Xing

Neutrino Oscillation, in which a given flavour of neutrino transforms into another is a powerful tool for probing small neutrino masses. The intrinsic neutrino properties involved are neutrino mass squared difference $\Delta m^2$ and the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Srubabati Goswami

The solar neutrino data are analyzed in a frequentist framework, using the Crow-Gardner and Feldman-Cousins prescriptions for the construction of confidence regions. Including in the fit only the total rates measured by the various…

High Energy Physics - Phenomenology · Physics 2009-11-07 Paolo Creminelli , Giovanni Signorelli , Alessandro Strumia

The minimal interpretation of the atmospheric neutrino data suggests that the muon neutrino oscillates into another species with a mixing angle close to the maximal $\pi/4$. In the Exact Parity Symmetric Model, both the muon and electron…

High Energy Physics - Phenomenology · Physics 2011-03-10 J. Bunn , R. Foot , R. R. Volkas

The mixing of three active neutrino flavors is parameterized by the unitary PMNS matrix. If there are more than three neutrino flavors and if the extra generations are heavy isosinglets, the effective $3\times 3$ mixing matrix for the three…

High Energy Physics - Phenomenology · Physics 2021-05-11 Luis Salvador Miranda , Pedro Pasquini , Ushak Rahaman , Soebur Razzaque

We review the present status of three-flavour neutrino oscillations, taking into account the latest available neutrino oscillation data presented at the Neutrino 2008 Conference. This includes the data released this summer by the MINOS…

High Energy Physics - Phenomenology · Physics 2010-02-11 Thomas Schwetz , Mariam Tortola , Jose W. F. Valle

CPT symmetry, the combination of Charge Conjugation, Parity and Time reversal, is a cornerstone of our model building strategy and therefore the repercussions of its potential violation will severely threaten the most extended tool we…

High Energy Physics - Phenomenology · Physics 2018-04-06 Gabriela Barenboim , Christoph Andreas Ternes , Mariam Tórtola

We account for the solar and atmospheric neutrino problems by introducing maximal mixing between conventional and sterile neutrino partners. We achieve this by invoking a seesaw-like mechanism which not only provides us with maximally mixed…

High Energy Physics - Phenomenology · Physics 2008-11-26 J P Bowes , R R Volkas

The T2K experiment measures muon neutrino disappearance and electron neutrino appearance in accelerator-produced neutrino and antineutrino beams. With an exposure of $14.7(7.6)\times 10^{20}$ protons on target in neutrino (antineutrino)…

High Energy Physics - Experiment · Physics 2018-10-31 K. Abe , R. Akutsu , A. Ali , J. Amey , C. Andreopoulos , L. Anthony , M. Antonova , S. Aoki , A. Ariga , Y. Ashida , Y. Azuma , S. Ban , M. Barbi , G. J. Barker , G. Barr , C. Barry , M. Batkiewicz , F. Bench , V. Berardi , S. Berkman , R. M. Berner , L. Berns , S. Bhadra , S. Bienstock , A. Blondel , S. Bolognesi , B. Bourguille , S. B. Boyd , D. Brailsford , A. Bravar , C. Bronner , M. Buizza Avanzini , J. Calcutt , T. Campbell , S. Cao , S. L. Cartwright , M. G. Catanesi , A. Cervera , A. Chappell , C. Checchia , D. Cherdack , N. Chikuma , G. Christodoulou , J. Coleman , G. Collazuol , D. Coplowe , A. Cudd , A. Dabrowska , G. De Rosa , T. Dealtry , P. F. Denner , S. R. Dennis , C. Densham , F. Di Lodovico , N. Dokania , S. Dolan , O. Drapier , K. E. Duffy , J. Dumarchez , P. Dunne , S. Emery-Schrenk , A. Ereditato , P. Fernandez , T. Feusels , A. J. Finch , G. A. Fiorentini , G. Fiorillo , C. Francois , M. Friend , Y. Fujii , R. Fujita , D. Fukuda , Y. Fukuda , K. Gameil , C. Giganti , F. Gizzarelli , T. Golan , M. Gonin , D. R. Hadley , L. Haegel , J. T. Haigh , P. Hamacher-Baumann , D. Hansen , J. Harada , M. Hartz , T. Hasegawa , N. C. Hastings , T. Hayashino , Y. Hayato , A. Hiramoto , M. Hogan , J. Holeczek , F. Hosomi , A. K. Ichikawa , M. Ikeda , J. Imber , T. Inoue , R. A. Intonti , T. Ishida , T. Ishii , M. Ishitsuka , K. Iwamoto , A. Izmaylov , B. Jamieson , M. Jiang , S. Johnson , P. Jonsson , C. K. Jung , M. Kabirnezhad , A. C. Kaboth , T. Kajita , H. Kakuno , J. Kameda , D. Karlen , T. Katori , Y. Kato , E. Kearns , M. Khabibullin , A. Khotjantsev , H. Kim , J. Kim , S. King , J. Kisiel , A. Knight , A. Knox , T. Kobayashi , L. Koch , T. Koga , P. P. Koller , A. Konaka , L. L. Kormos , Y. Koshio , K. Kowalik , H. Kubo , Y. Kudenko , R. Kurjata , T. Kutter , M. Kuze , L. Labarga , J. Lagoda , M. Lamoureux , P. Lasorak , M. Laveder , M. Lawe , M. Licciardi , T. Lindner , Z. J. Liptak , R. P. Litchfield , X. Li , A. Longhin , J. P. Lopez , T. Lou , L. Ludovici , X. Lu , L. Magaletti , K. Mahn , M. Malek , S. Manly , L. Maret , A. D. Marino , J. F. Martin , P. Martins , T. Maruyama , T. Matsubara , V. Matveev , K. Mavrokoridis , W. Y. Ma , E. Mazzucato , M. McCarthy , N. McCauley , K. S. McFarland , C. McGrew , A. Mefodiev , C. Metelko , M. Mezzetto , A. Minamino , O. Mineev , S. Mine , A. Missert , M. Miura , S. Moriyama , J. Morrison , Th. A. Mueller , S. Murphy , Y. Nagai , T. Nakadaira , M. Nakahata , Y. Nakajima , K. G. Nakamura , K. Nakamura , K. D. Nakamura , Y. Nakanishi , S. Nakayama , T. Nakaya , K. Nakayoshi , C. Nantais , C. Nielsen , K. Niewczas , K. Nishikawa , Y. Nishimura , T. S. Nonnenmacher , P. Novella , J. Nowak , H. M. O'Keeffe , L. O'Sullivan , K. Okumura , T. Okusawa , W. Oryszczak , S. M. Oser , R. A. Owen , Y. Oyama , V. Palladino , J. L. Palomino , V. Paolone , P. Paudyal , M. Pavin , D. Payne , L. Pickering , C. Pidcott , E. S. Pinzon Guerra , C. Pistillo , B. Popov , K. Porwit , M. Posiadala-Zezula , A. Pritchard , B. Quilain , T. Radermacher , E. Radicioni , P. N. Ratoff , E. Reinherz-Aronis , C. Riccio , E. Rondio , B. Rossi , S. Roth , A. Rubbia , A. C. Ruggeri , A. Rychter , K. Sakashita , F. Sánchez , S. Sasaki , E. Scantamburlo , K. Scholberg , J. Schwehr , M. Scott , Y. Seiya , T. Sekiguchi , H. Sekiya , D. Sgalaberna , R. Shah , A. Shaikhiev , F. Shaker , D. Shaw , M. Shiozawa , A. Smirnov , M. Smy , J. T. Sobczyk , H. Sobel , Y. Sonoda , J. Steinmann , T. Stewart , P. Stowell , Y. Suda , S. Suvorov , A. Suzuki , S. Y. Suzuki , Y. Suzuki , A. A. Sztuc , R. Tacik , M. Tada , A. Takeda , Y. Takeuchi , R. Tamura , H. K. Tanaka , H. A. Tanaka , T. Thakore , L. F. Thompson , W. Toki , C. Touramanis , K. M. Tsui , T. Tsukamoto , M. Tzanov , Y. Uchida , W. Uno , M. Vagins , Z. Vallari , G. Vasseur , C. Vilela , T. Vladisavljevic , V. V. Volkov , T. Wachala , J. Walker , Y. Wang , D. Wark , M. O. Wascko , A. Weber , R. Wendell , M. J. Wilking , C. Wilkinson , J. R. Wilson , R. J. Wilson , C. Wret , Y. Yamada , K. Yamamoto , S. Yamasu , C. Yanagisawa , G. Yang , T. Yano , K. Yasutome , S. Yen , N. Yershov , M. Yokoyama , T. Yoshida , M. Yu , A. Zalewska , J. Zalipska , K. Zaremba , G. Zarnecki , M. Ziembicki , E. D. Zimmerman , M. Zito , S. Zsoldos , A. Zykova

With the latest astronomical data including Cosmic Microwave Background (WMAP three year, CBI, ACBAR, VSA), Type Ia Supernova ("gold sample"), Galaxy Clustering (SDSS 3-D matter power, Lyman-$\alpha$ forest and Baryon Acoustic Oscillating…

Astrophysics · Physics 2010-10-27 Gong-Bo Zhao , Jun-Qing Xia , Xinmin Zhang

The T2K Experiment has observed the appearance of electron neutrinos in a muon-neutrino beam. Twenty eight neutrino candidates pass the selection cuts with a predicted background of $4.64 \pm 0.53$ events, which corresponds to a 6.8$\sigma$…

High Energy Physics - Experiment · Physics 2019-08-14 Michael Wilking

We present a three-parameter neutrino-oscillation model for three flavors of massless neutrinos with Fermi-point splitting and tri-maximal mixing angles. One of these parameters is the T-violating phase \epsilon, for which the experimental…

High Energy Physics - Phenomenology · Physics 2010-11-05 Frans R. Klinkhamer