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The neutrino mixing sum rule $\theta_{12} - \theta_{13}\cos(\delta) \approx \theta^\nu_{12}$ provides a possibility to explore the structure of the neutrino mass matrix in the presence of charged lepton corrections, since it relates the 1-2…

High Energy Physics - Phenomenology · Physics 2010-10-27 S. Antusch , P. Huber , S. F. King , T. Schwetz

We explore the possibility of generating a non-zero $U_{e3}$ element of the neutrino mixing matrix from tribimaximal neutrino mixing by adding a light sterile neutrino to the active neutrinos. Small active-sterile mixing can provide the…

High Energy Physics - Phenomenology · Physics 2016-10-11 S. Dev , Desh Raj , Radha Raman Gautam

The recent result from the chromium source experiment carried out by the GALLEX collaboration implies interesting limits on the parameters $\Delta m^2$ and $\sin^22\theta$ describing neutrino oscillations. Values of $\Delta m^2~>~0.17$…

High Energy Physics - Phenomenology · Physics 2009-10-07 J. N. Bahcall , P. I. Krastev , E. Lisi

This paper discusses recent results and near-term prospects of the long-baseline neutrino experiments MINOS, MINOS+, T2K and NOvA. The non-zero value of the third neutrino mixing angle {\theta}13 allows experimental analysis in a manner…

High Energy Physics - Experiment · Physics 2016-02-17 Tsuyoshi Nakaya , Robert K. Plunkett

Neutrino oscillations are studied employing sources of low energy monoenergetic neutrinos following electron capture by the nucleus and measuring electron recoils. Since the neutrino energy is very low the oscillation length appearing in…

High Energy Physics - Phenomenology · Physics 2011-01-27 J. D. Vergados , Y. Giomataris , Yu. N. Novikov

The status of the electroweak precision data as of winter 2003 and the corresponding theoretical calculations are presented. The possible problems within the data and the calculations are discussed in a critical way. If the NuTeV anomaly…

High Energy Physics - Phenomenology · Physics 2007-05-23 Klaus Moenig

We determine constraints on parameters of a single eV-scale light neutrino using IceCube-59 data. Particular emphasis is put on the question whether such an analysis can rule out sterile neutrino hints. While important complementary…

High Energy Physics - Phenomenology · Physics 2016-02-17 Manfred Lindner , Werner Rodejohann , Xun-Jie Xu

We study theoretical constraints on the parameter space under the conditions from vacuum stability and triviality in the three-loop radiative seesaw model with TeV-scale right-handed neutrinos which are odd under the $Z_2$ parity. In this…

High Energy Physics - Phenomenology · Physics 2011-05-12 Mayumi Aoki , Shinya Kanemura , Kei Yagyu

Oscillations of three neutrinos with all squared mass splittings around 10^{-3} eV^2 are not firmly excluded by solar neutrino experiments. We carefully verify that they are also perfectly compatible with atmospheric neutrino experiments:…

High Energy Physics - Phenomenology · Physics 2009-10-31 Alessandro Strumia

We consider a scenario with unitary mixing of the three light standard neutrinos and a non-unitary mixing contribution of a heavier massive neutrino that can generate short-baseline neutrino oscillations. We show that this scenario predicts…

High Energy Physics - Phenomenology · Physics 2019-08-08 C. Giunti

Current neutrino data are consistent with the so-called tribimaximal mixing scenario, which predicts \sin^2 \theta_{12}=1/3, zero U_{e3} and maximal \theta_{23}. This implies a special form of the neutrino mass matrix. Introducing small…

High Energy Physics - Phenomenology · Physics 2014-11-18 F. Plentinger , W. Rodejohann

We present limits on sterile neutrino mixing using 4,438 live-days of atmospheric neutrino data from the Super-Kamiokande experiment. We search for fast oscillations driven by an eV$^2$-scale mass splitting and for oscillations into sterile…

High Energy Physics - Experiment · Physics 2015-03-26 Kamiokande Collaboration , K. Abe , Y. Haga , Y. Hayato , M. Ikeda , K. Iyogi , J. Kameda , Y. Kishimoto , M. Miura , S. Moriyama , M. Nakahata , Y. Nakano , S. Nakayama , H. Sekiya , M. Shiozawa , Y. Suzuki , A. Takeda , H. Tanaka , T. Tomura , K. Ueno , R. A. Wendell , T. Yokozawa , T. Irvine , T. Kajita , I. Kametani , K. Kaneyuki , K. P. Lee , T. McLachlan , Y. Nishimura , E. Richard , K. Okumura , L. Labarga , P. Fernandez , S. Berkman , H. A. Tanaka , S. Tobayama , J. Gustafson , E. Kearns , J. L. Raaf , J. L. Stone , L. R. Sulak , M. Goldhaber , G. Carminati , W. R. Kropp , S. Mine , P. Weatherly , A. Renshaw , M. B. Smy , H. W. Sobel , V. Takhistov , K. S. Ganezer , B. L. Hartfiel , J. Hill , W. E. Keig , N. Hong , J. Y. Kim , I. T. Lim , T. Akiri , A. Himmel , K. Scholberg , C. W. Walter , T. Wongjirad , T. Ishizuka , S. Tasaka , J. S. Jang , J. G. Learned , S. Matsuno , S. N. Smith , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , A. T. Suzuki , Y. Takeuchi , C. Bronner , S. Hirota , K. Huang , K. Ieki , T. Kikawa , A. Minamino , A. Murakami , T. Nakaya , K. Suzuki , S. Takahashi , K. Tateishi , Y. Fukuda , K. Choi , Y. Itow , G. Mitsuka , P. Mijakowski , J. Hignight , J. Imber , C. K. Jung , C. Yanagisawa , H. Ishino , A. Kibayashi , Y. Koshio , T. Mori , M. Sakuda , R. Yamaguchi , T. Yano , Y. Kuno , R. Tacik , S. B. Kim , H. Okazawa , Y. Choi , K. Nishijima , M. Koshiba , Y. Suda , Y. Totsuka , M. Yokoyama , K. Martens , Ll. Marti , M. R. Vagins , J. F. Martin , P. de Perio , A. Konaka , M. J. Wilking , S. Chen , Y. Zhang , K. Connolly , R. J. Wilkes

Models of neutrino mixing involving one or more sterile neutrinos have resurrected their importance in the light of recent cosmological data. In this case, reactor antineutrino experiments offer an ideal place to look for signatures of…

High Energy Physics - Phenomenology · Physics 2014-08-25 Ivan Girardi , Davide Meloni , Tommy Ohlsson , He Zhang , Shun Zhou

Seesaw mechanism constrains from below mixing between active and sterile neutrinos for fixed sterile neutrino masses. Signal events associated with sterile neutrino decays inside a detector at fixed target experiment are suppressed by the…

High Energy Physics - Phenomenology · Physics 2018-10-09 Igor Krasnov , Timofey Grigorin-Ryabov

Several neutrino experiments have reported results that are potentially inconsistent with our current understanding of the lepton sector. A candidate solution to these so-called short-baseline anomalies is postulating the existence of new,…

High Energy Physics - Phenomenology · Physics 2023-01-27 K. S. Babu , Vedran Brdar , André de Gouvêa , Pedro A. N. Machado

The data on atmospheric neutrinos can be explained assuming the existence of oscillations between muon neutrinos and light sterile neutrinos with mixing close to maximal, and Delta_m^2 approximately equal to 3 E-3 (eV^2). This…

High Energy Physics - Phenomenology · Physics 2017-09-06 Pasquale Di Bari , Paolo Lipari , Maurizio Lusignoli

We propose a neutrino model based on a $\Delta(54)$ flavor symmetry suitable for explaining the current neutrino oscillation data. Neutrino masses arise from the type II seesaw mechanism where the $\Delta(54)$ field assignments has led to a…

High Energy Physics - Phenomenology · Physics 2024-10-21 M. A. Loualidi

A search for muon anti-neutrino to electron anti-neutrino oscillations was conducted by the Liquid Scintillator Neutrino Detector at the Los Alamos Neutron Science Center using muon anti-neutrinos from positive muon decay at rest. A total…

Motivated by the accumulating hints of new sterile neutrino species at the eV scale, we explore the consequences of such an hypothesis on the solar sector phenomenology. After introducing the theoretical formalism needed to describe the MSW…

High Energy Physics - Phenomenology · Physics 2011-07-08 Antonio Palazzo

The discovery of neutrino oscillations has shown that neutrinos, in contradiction to a prediction of the minimal standard model, have mass. Oscillations do not yield a value for the mass, but do set a lower limit of 0.02 eV on the average…

Nuclear Experiment · Physics 2015-02-03 R. G. Hamish Robertson
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