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Related papers: Four-neutrino model and the K2K experiment

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Recently it was suggested that two very different mass-squared differences play a role in atmospheric neutrino oscillations. The larger of these also accounts for the LSND result and the smaller of these also drives the solar neutrino…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Barenboim , M. Narayan , S. Uma Sankar

The Tokai to Kamioka (T2K) experiment uses a beam of muon neutrinos, produced at the J-PARC facility on the east coast of Japan, to study neutrino oscillations driven by the $\Delta m_{\textrm{atm}}^{2}$ mass splitting. A suite of near…

High Energy Physics - Experiment · Physics 2015-01-20 Martin David Haigh

As neutrino oscillation data becomes ever more precise, the use of approximate formulae for the oscillation probabilities ${\mathcal P}_{\alpha\beta}$ must be examined to ensure that the approximation is adequate. Here, the oscillation…

High Energy Physics - Phenomenology · Physics 2014-06-06 B. K. Cogswell , D. C. Latimer , D. J. Ernst

We review the present status of global analyses of neutrino oscillations, taking into account the most recent neutrino data including the latest KamLAND and K2K updates presented at Neutrino2004, as well as state-of-the-art solar and…

High Energy Physics - Phenomenology · Physics 2009-09-17 M. Maltoni , T. Schwetz , M. A. Tortola , J. W. F. Valle

We study the potential of the CNGS beam in constraining the parameter space of a model with one sterile neutrino separated from three active ones by an $\mathcal{O}(\eVq)$ mass-squared difference, $\Dmq_\Sbl$. We perform our analysis using…

High Energy Physics - Phenomenology · Physics 2009-01-06 A. Donini , M. Maltoni , D. Meloni , P. Migliozzi , F. Terranova

We study oscillations of the high energy atmospheric neutrinos in the Earth into sterile neutrinos with the eV-scale mass. The MSW resonance and parametric enhancement of the $\bar{\nu}_\mu\to\bar{\nu}_s$ oscillations lead to distortion of…

High Energy Physics - Phenomenology · Physics 2015-06-16 Arman Esmaili , Alexei Yu. Smirnov

Within the standard 3nu mass-mixing framework, we present an up-to-date global analysis of neutrino oscillation data (as of January 2016), including the latest available results from experiments with atmospheric neutrinos (Super-Kamiokande…

High Energy Physics - Phenomenology · Physics 2016-06-22 F. Capozzi , E. Lisi , A. Marrone , D. Montanino , A. Palazzo

Oscillations of three pseudo--Dirac flavor neutrinos $\nu_e, \nu_\mu, \nu_\tau$ are considered: $0 < m^{(L)} = m^{(R)} \ll m^{(D)}$ for their Majorana and Dirac masses taken as universal before family mixing. The actual neutrino mass matrix…

High Energy Physics - Phenomenology · Physics 2007-05-23 Wojciech Krolikowski

Anticipating future long-baseline neutrino experiments to search for neutrino oscillations in various oscillation channels, we have analyzed the atmospheric neutrino data in the framework of a model with mixing of three massive neutrino…

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

This work estimates the probability of $\mu$ to $e$ neutrino oscillation with two sterile neutrinos using a 5x5 U-matrix, an extension of the previous estimate with one sterile neutrino and a 4x4 U-matrix. The sterile neutrino-active…

High Energy Physics - Phenomenology · Physics 2016-06-29 Leonard S. Kisslinger

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

We present a simple scheme of mixing of four neutrinos that can accommodate the results of all neutrino oscillation experiments, the observed abundances of primordial elements and the current upper bound for the effective Majorana neutrino…

High Energy Physics - Phenomenology · Physics 2011-08-17 C. Giunti

We demonstrate that the solar and atmospheric neutrino data as well as the recent result of the LSND experiment cannot be satisfied simultaneously with three light neutrinos if we consider the mass degeneracy for two neutrinos in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Ambar Ghosal , Asim K. Ray

Since the 3+1 neutrino models with one light sterile neutrino turn out to be not very effective, at least two light sterile neutrinos may be needed to reconcile the solar and atmospheric neutrino experiments with the LSND result, {\it if}…

High Energy Physics - Phenomenology · Physics 2007-05-23 Wojciech Krolikowski

This paper presents the recent results from Super-Kamiokande atmospheric neutrinos and from K2K accelerator neutrinos. Both results show the signal of neutrino oscillation, and provide new and precise information of oscillation parameters.…

High Energy Physics - Experiment · Physics 2007-05-23 T. Nakaya

We discuss the potential of SNO to constraint the four-neutrino mixing schemes favoured by the results of all neutrino oscillations experiments. These schemes allow simultaneous transitions of solar $\nu_e's$ into active $\nu_\mu$'s,…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. C. Gonzalez-Garcia , C. Peña-Garay

We suggest mass matrices for neutrinos and charged leptons that can explain solar and atmospheric neutrino data. The resulting flavor mixing matrix $V_{\nu}$ has a property that $(V_{\nu})_{13}=0$, thus making $\nu_e \leftrightarrow…

High Energy Physics - Phenomenology · Physics 2009-10-30 Kyungsik Kang , Sin Kyu Kang , Jihn E. Kim , Pyungwon Ko

Neutrino oscillation experiments have measured precisely the mass-squared differences of three neutrino mass eigenstates, and three leptonic mixing angles by utilizing both neutrino and anti-neutrino oscillations. The possible CPT violation…

High Energy Physics - Phenomenology · Physics 2023-02-08 T. V. Ngoc , S. Cao , N. T. Hong Van , P. T. Quyen

The neutrinos of long baseline beams travel inside the Earth's crust where the density is approximately rho = 2.8 g cm^-3. If electron neutrinos participate in the oscillations, matter effects will modify the oscillation probabilities with…

High Energy Physics - Phenomenology · Physics 2009-10-31 Paolo Lipari

We analyze the oscillation signals generated by one extra sterile neutrino. We fully take into account the effects of the established oscillations among active neutrinos. We analyze the effects in solar, atmospheric, reactor and beam…

High Energy Physics - Phenomenology · Physics 2007-05-23 Guido Marandella
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