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We discuss consequences of assuming that the (Majorana) neutrino mass matrix $M_\nu$ and the charged lepton mass matrix $M_l$ satisfy, $S_\nu^T M_\nu S_\nu=-M_\nu~,T_l^\dagger M_lM_l^\dagger T_l=M_lM_l^\dagger$ with respect to some discrete…

High Energy Physics - Phenomenology · Physics 2016-08-31 Anjan S Joshipura , Newton Nath

The recent T2K and MINOS indications for a "large" theta_13 neutrino mixing angle can be accommodated in principle by an infinite number of Yukawa flavour structures in the seesaw model. Without considering any explicit flavour symmetry,…

High Energy Physics - Phenomenology · Physics 2015-05-28 Xiaoyong Chu , Mikael Dhen , Thomas Hambye

A model of neutrino oscillation experiments is constructed. The experiments incorporated are: solar neutrinos (Chlorine, Gallium, Super-K, and SNO), reactor neutrinos (Bugey and CHOOZ), beam stop neutrinos (LSND decay at rest and decay in…

Nuclear Theory · Physics 2007-05-23 D. C. Latimer , D. J. Ernst

The Daya Bay experiment was the first to report simultaneous measurements of reactor antineutrinos at multiple baselines leading to the discovery of $\bar{\nu}_e$ oscillations over km-baselines. Subsequent data has provided the world's most…

Instrumentation and Detectors · Physics 2016-02-02 F. P. An , J. Z. Bai , A. B. Balantekin , H. R. Band , D. Beavis , W. Beriguete , M. Bishai , S. Blyth , R. L. Brown , I. Butorov , D. Cao , G. F. Cao , J. Cao , R. Carr , W. R. Cen , W. T. Chan , Y. L. Chan , J. F. Chang , L. C. Chang , Y. Chang , C. Chasman , H. Y. Chen , H. S. Chen , M. J. Chen , Q. Y. Chen , S. J. Chen , S. M. Chen , X. C. Chen , X. H. Chen , X. S. Chen , Y. X. Chen , Y. Chen , J. H. Cheng , J. Cheng , Y. P. Cheng , J. J. Cherwinka , S. Chidzik , K. Chow , M. C. Chu , J. P. Cummings , J. de Arcos , Z. Y. Deng , X. F. Ding , Y. Y. Ding , M. V. Diwan , L. Dong , J. Dove , E. Draeger , X. F. Du , D. A. Dwyer , W. R. Edwards , S. R. Ely , S. D. Fang , J. Y. Fu , Z. W. Fu , L. Q. Ge , V. Ghazikhanian , R. Gill , J. Goett , M. Gonchar , G. H. Gong , H. Gong , Y. A. Gornushkin , M. Grassi , L. S. Greenler , W. Q. Gu , M. Y. Guan , R. P. Guo , X. H. Guo , R. W. Hackenburg , R. L. Hahn , R. Han , S. Hans , M. He , Q. He , W. S. He , K. M. Heeger , Y. K. Heng , A. Higuera , P. Hinrichs , T. H. Ho , M. Hoff , Y. K. Hor , Y. B. Hsiung , B. Z. Hu , L. M. Hu , L. J. Hu , T. Hu , W. Hu , E. C. Huang , H. Z. Huang , H. X. Huang , P. W. Huang , X. Huang , X. T. Huang , P. Huber , G. Hussain , Z. Isvan , D. E. Jaffe , P. Jaffke , K. L. Jen , S. Jetter , X. P. Ji , X. L. Ji , H. J. Jiang , W. Q. Jiang , J. B. Jiao , R. A. Johnson , J. Joseph , L. Kang , S. H. Kettell , S. Kohn , M. Kramer , K. K. Kwan , M. W. Kwok , T. Kwok , C. Y. Lai , W. C. Lai , W. H. Lai , T. J. Langford , K. Lau , L. Lebanowski , J. Lee , M. K. P. Lee , R. T. Lei , R. Leitner , J. K. C. Leung , K. Y. Leung , C. A. Lewis , B. Li , C. Li , D. J. Li , F. Li , G. S. Li , J. Li , N. Y. Li , Q. J. Li , S. F. Li , S. C. Li , W. D. Li , X. B. Li , X. N. Li , X. Q. Li , Y. Li , Y. F. Li , Z. B. Li , H. Liang , J. Liang , C. J. Lin , G. L. Lin , P. Y. Lin , S. X. Lin , S. K. Lin , Y. C. Lin , J. J. Ling , J. M. Link , L. Littenberg , B. R. Littlejohn , B. J. Liu , C. Liu , D. W. Liu , H. Liu , J. L. Liu , J. C. Liu , S. Liu , S. S. Liu , X. Liu , Y. B. Liu , C. Lu , H. Q. Lu , J. S. Lu , A. Luk , K. B. Luk , T. Luo , X. L. Luo , L. H. Ma , Q. M. Ma , X. Y. Ma , X. B. Ma , Y. Q. Ma , B. Mayes , K. T. McDonald , M. C. McFarlane , R. D. McKeown , Y. Meng , I. Mitchell , D. Mohapatra , J. Monari Kebwaro , J. E. Morgan , Y. Nakajima , J. Napolitano , D. Naumov , E. Naumova , C. Newsom , H. Y. Ngai , W. K. Ngai , Y. B. Nie , Z. Ning , J. P. Ochoa-Ricoux , A. Olshevskiy , A. Pagac , H. -R. Pan , S. Patton , C. Pearson , V. Pec , J. C. Peng , L. E. Piilonen , L. Pinsky , C. S. J. Pun , F. Z. Qi , M. Qi , X. Qian , N. Raper , B. Ren , J. Ren , R. Rosero , B. Roskovec , X. C. Ruan , W. R. Sands , B. Seilhan , B. B. Shao , K. Shih , W. Y. Song , H. Steiner , P. Stoler , M. Stuart , G. X. Sun , J. L. Sun , N. Tagg , Y. H. Tam , H. K. Tanaka , W. Tang , X. Tang , D. Taychenachev , H. Themann , Y. Torun , S. Trentalange , O. Tsai , K. V. Tsang , R. H. M. Tsang , C. E. Tull , Y. C. Tung , N. Viaux , B. Viren , S. Virostek , V. Vorobel , C. H. Wang , L. S. Wang , L. Y. Wang , L. Z. Wang , M. Wang , N. Y. Wang , R. G. Wang , T. Wang , W. Wang , W. W. Wang , X. T. Wang , X. Wang , Y. F. Wang , Z. Wang , Z. Wang , Z. M. Wang , D. M. Webber , H. Y. Wei , Y. D. Wei , L. J. Wen , D. L. Wenman , K. Whisnant , C. G. White , L. Whitehead , C. A. Whitten , J. Wilhelmi , T. Wise , H. C. Wong , H. L. H. Wong , J. Wong , S. C. F. Wong , E. Worcester , F. F. Wu , Q. Wu , D. M. Xia , J. K. Xia , S. T. Xiang , Q. Xiao , Z. Z. Xing , G. Xu , J. Y. Xu , J. L. Xu , J. Xu , W. Xu , Y. Xu , T. Xue , J. Yan , C. G. Yang , L. Yang , M. S. Yang , M. T. Yang , M. Ye , M. Yeh , Y. S. Yeh , K. Yip , B. L. Young , G. Y. Yu , Z. Y. Yu , S. Zeng , L. Zhan , C. Zhang , F. H. Zhang , H. H. Zhang , J. W. Zhang , K. Zhang , Q. X. Zhang , Q. M. Zhang , S. H. Zhang , X. T. Zhang , Y. C. Zhang , Y. H. Zhang , Y. M. Zhang , Y. X. Zhang , Y. M. Zhang , Z. J. Zhang , Z. Y. Zhang , Z. P. Zhang , J. Zhao , Q. W. Zhao , Y. F. Zhao , Y. B. Zhao , L. Zheng , W. L. Zhong , L. Zhou , N. Zhou , Z. Y. Zhou , H. L. Zhuang , S. Zimmerman , J. H. Zou

We present a model based on the flavour group S3 X Z3 X Z6 to explain the main features of fermion masses and mixing. In particular, in the neutrino sector the breaking of the S3 symmetry is responsible for a naturally small r=\Delta…

High Energy Physics - Phenomenology · Physics 2015-06-04 Davide Meloni

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

The "texture zero mass matrices" for the quarks and leptons describe very well the flavor mixing of the quarks and leptons. We can calculate the angles of the unitarity triangle. We expect the angle alpha of the unitarity triangle to be 90…

High Energy Physics - Phenomenology · Physics 2011-04-26 Harald Fritzsch

Large neutrino mixing angles suggest that the Yukawa sector is invariant under permutations of the fermion families. This S_{3} permutation symmetry is broken at a large energy scale but much below the unification scale. Assuming that the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Francesco Caravaglios , Stefano Morisi

Recent data in the neutrino sector point towards a relatively large value of the reactor angle, incompatible with a vanishing theta_ 13 at about 3 sigma. In order to explain such a result, we propose a SUSY model based on the broken…

High Energy Physics - Phenomenology · Physics 2015-05-30 Davide Meloni

Nailing down the unknown neutrino mixing angle theta_13 is one of the most important goals in current lepton physics. In this context, we perform a global analysis of neutrino oscillation data, focusing on theta_13, and including recent…

High Energy Physics - Phenomenology · Physics 2010-04-06 G. L. Fogli , E. Lisi , A. Marrone , A. Palazzo , A. M. Rotunno

Among neutrino mixings, the reactor mixing angle, \theta_{13}, is observed to be almost vanishing and is consistent with \theta_{13}=0. We discuss how the condition of \theta_{13}=0 constrains models of neutrino mixings and show that, for…

High Energy Physics - Phenomenology · Physics 2010-11-08 Keisuke Yuda , Masaki Yasue

We study non-standard interactions (NSIs) at reactor neutrino experiments, and in particular, the mimicking effects on \theta_13. We present generic formulas for oscillation probabilities including NSIs from sources and detectors.…

High Energy Physics - Phenomenology · Physics 2009-01-16 Tommy Ohlsson , He Zhang

We revisit the discrete dark matter model with $A_4$ flavor symmetry originally introduced by M.Hirsch {\it et.al}. We show that radiative corrections can lead to non-zero $\theta_{13}$ and non-zero mass for the lightest neutrino. We find…

High Energy Physics - Phenomenology · Physics 2015-06-19 Yuta Hamada , Tatsuo Kobayashi , Atsushi Ogasahara , Yuji Omura , Fumihiro Takayama , Daiki Yasuhara

We propose a new mixing pattern for neutrinos with a nonzero mixing angle $\theta_{13}$. Under a simple form, it agrees well with current neutrino oscillation data and displays a number of intriguing features including the $\mu$-$\tau$…

High Energy Physics - Phenomenology · Physics 2013-08-27 Huilin Qu , Bo-Qiang Ma

Recently, three reactor neutrino experiments, Daya Bay, Double Chooz and RENO have directly measured the neutrino mixing angle $\theta_{13}$. In this paper, another important oscillation parameter, effective $\Delta m_{31}^2$ (= $\Delta…

High Energy Physics - Experiment · Physics 2013-08-21 T. J. C. Bezerra , H. Furuta , F. Suekane , T. Matsubara

We study neutrino masses and mixing in Supersymmetric Models without $R$ parity and with generic soft Supersymmetry breaking terms. Neutrinos acquire mass from various sources: tree level neutrino--neutralino mixing, loop effects and…

High Energy Physics - Phenomenology · Physics 2009-10-28 Francesca M. Borzumati , Yuval Grossman , Enrico Nardi , Yosef Nir

A brief review is given of some recent works where baryogenesis and dark matter have a common origin within the $U(1)$ extensions of the standard model and of the minimal supersymmetric standard model. The models considered generate the…

High Energy Physics - Phenomenology · Physics 2017-05-31 Wan-Zhe Feng , Pran Nath

The Daya Bay reactor experiment has reported the most precise measurement of sin$^{2}2\theta_{13}$ and $\Delta m^{2}_{ee}$ by using a data set with the fully constructed design of 8 antineutrino detectors (ADs). We also report on a new…

High Energy Physics - Phenomenology · Physics 2016-07-26 A. Higuera

Recently new reactor antineutrino spectra have been provided for 235U, 239Pu, 241Pu and 238U, increasing the mean flux by about 3 percent. To good approximation, this reevaluation applies to all reactor neutrino experiments. The synthesis…

High Energy Physics - Experiment · Physics 2011-05-12 G. Mention , M. Fechner , Th. Lasserre , Th. A. Mueller , D. Lhuillier , M. Cribier , A. Letourneau

We present a new realization of inverted neutrino mass hierarchy based on $S_3 \times {\cal U}(1)$ flavor symmetry. In this scenario, the deviation of the solar oscillation angle from $\pi/4$ is correlated with the value of $\theta_{13}$,…

High Energy Physics - Phenomenology · Physics 2008-11-26 K. S. Babu , Abdel G. Bachri , Zurab Tavartkiladze