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This paper reviews the constraints on the solar neutrino mixing parameters with data collected by the Homestake, SAGE, GALLEX, Kamiokande, SuperKamiokande, and SNO experiments. An emphasis will be given to the global solar neutrino analyses…

High Energy Physics - Experiment · Physics 2009-11-10 Alain Bellerive

The next generation of searches for neutrinoless double beta decay (0{\nu}\b{eta}\b{eta}) are poised to answer deep questions on the nature of neutrinos and the source of the Universe's matter-antimatter asymmetry. They will be looking for…

Data Analysis, Statistics and Probability · Physics 2023-12-25 Z. Fu , C. Grant , D. M. Krawiec , A. Li , L. Winslow

Assuming the current best-fit solutions to the solar neutrino problem at large mixing angle, we briefly illustrate how prospective data from the Sudbury Neutrino Observatory (SNO) and from the Kamioka Liquid scintillator Anti-Neutrino…

High Energy Physics - Phenomenology · Physics 2016-09-06 G. L. Fogli , E. Lisi , A. Palazzo , A. M. Rotunno

A joint analysis of solar neutrino data together with the new KamLAND data is presented in the RSFP framework. It is investigated that how the new KamLAND data effects the allowed regions at different $\mu B$ values. A limit on $\mu B$…

High Energy Physics - Phenomenology · Physics 2008-10-07 D. Yilmaz

In this thesis we explore the implications of neutrino oscillations in the context of the solar neutrino data, the atmospheric neutrino data and results from the terrestrial accelerator/reactor neutrino oscillation experiments. We perform…

High Energy Physics - Phenomenology · Physics 2007-05-23 Sandhya Choubey

We show how neutrino data can be used in order to constrain the free parameters of possible extensions to the standard model of elementary particles (SM). For definiteness, we focus in the recently proposed unparticle scenario. We show that…

High Energy Physics - Phenomenology · Physics 2014-11-20 J. Barranco , A. Bolanos , O. G. Miranda , C. A. Moura , T. I. Rashba

There is no consistent solar model which can describe all experimental data on the solar neutrinos. The problem can be formulated essentially in a model independent way. The key points are the comparison of the Homestake and the Kamiokande…

High Energy Physics - Phenomenology · Physics 2009-09-25 Alexei Yu. Smirnov

While KamLAND apparently rules out Resonant-Spin-Flavor-Precession (RSFP) as an explanation of the solar neutrino deficit, the solar neutrino fluxes in the Cl and Ga experiments vary with solar rotation rates. Added to this evidence,…

High Energy Physics - Phenomenology · Physics 2016-09-06 D. O. Caldwell , P. A. Sturrock

Nuclear power reactors are the most intense man-made source of antineutrino's and have long been recognized as promising sources for coherent elastic neutrino-nucleus scattering (CE$\nu$NS) studies. Its observation and the spectral shape of…

Nuclear Theory · Physics 2024-06-25 Leendert Hayen

Every second greater than $10^{25}$ antineutrinos radiate to space from Earth, shining like a faint antineutrino star. Underground antineutrino detectors have revealed the rapidly decaying fission products inside nuclear reactors, verified…

Instrumentation and Detectors · Physics 2016-02-04 Shawn M. Usman , Glenn R. Jocher , Stephen T. Dye , William F. McDonough , John G. Learned

Recently, several models have been suggested to reduce the tension between Gallium and reactor antineutrino spectral ratio data which is found in the framework of 3+1 active-sterile neutrino mixing. Among these models, we consider the…

High Energy Physics - Phenomenology · Physics 2023-12-04 Carlo Giunti , Christoph A. Ternes

Atmospheric neutrino and solar neutrino data from the first phase of Super-Kamiokande (SK-I) are presented. The observed data are used to study atmospheric and solar neutrino oscillations. Zenith angle distributions from various atmospheric…

High Energy Physics - Experiment · Physics 2019-08-14 M. Ishitsuka

The T2K collaboration: reports evidence for electron neutrino appearance at the atmospheric mass splitting, |\Delta m_{32}^2|=2.4x10^{-3} eV^2. An excess of electron neutrino interactions over background is observed from a muon neutrino…

High Energy Physics - Experiment · Physics 2019-08-17 T2K Collaboration , K. Abe , N. Abgrall , H. Aihara , T. Akiri , J. B. Albert , C. Andreopoulos , S. Aoki , A. Ariga , T. Ariga , S. Assylbekov , D. Autiero , M. Barbi , G. J. Barker , G. Barr , M. Bass , M. Batkiewicz , F. Bay , S. W. Bentham , V. Berardi , B. E. Berger , S. Berkman , I. Bertram , D. Beznosko , S. Bhadra , F. d. M. Blaszczyk , A. Blondel , C. Bojechko , S. Boyd , D. Brailsford , A. Bravar , C. Bronner , D. G. Brook-Roberge , N. Buchanan , R. G. Calland , J. Caravaca Rodriguez , S. L. Cartwright , R. Castillo , M. G. Catanesi , A. Cervera , D. Cherdack , G. Christodoulou , A. Clifton , J. Coleman , S. J. Coleman , G. Collazuol , K. Connolly , L. Cremonesi , A. Curioni , A. Dabrowska , I. Danko , R. Das , S. Davis , M. Day , J. P. A. M. de Andre , P. de Perio , G. De Rosa , T. Dealtry , S. Dennis , C. Densham , F. Di Lodovico , S. Di Luise , J. Dobson , O. Drapier , T. Duboyski , F. Dufour , J. Dumarchez , S. Dytman , M. Dziewiecki , M. Dziomba , S. Emery , A. Ereditato , L. Escudero , A. J. Finch , E. Frank , M. Friend , Y. Fujii , Y. Fukuda , A. Furmanski , V. Galymov , A. Gaudin , S. Giffin , C. Giganti , K. Gilje , T. Golan , J. J. Gomez-Cadenas , M. Gonin , N. Grant , D. Gudin , D. R. Hadley , A. Haesler , M. D. Haigh , P. Hamilton , D. Hansen , T. Hara , M. Hartz , T. Hasegawa , N. C. Hastings , Y. Hayato , C. Hearty , R. L. Helmer , M. Hierholzer , J. Hignight , A. Hillairet , A. Himmel , T. Hiraki , S. Hirota , J. Holeczek , S. Horikawa , K. Huang , A. K. Ichikawa , K. Ieki , M. Ieva , M. Ikeda , J. Imber , J. Insler , T. J. Irvine , T. Ishida , T. Ishii , S. J. Ives , K. Iyogi , A. Izmaylov , A. Jacob , B. Jamieson , R. A. Johnson , J. H. Jo , P. Jonsson , K. K. Joo , C. K. Jung , A. Kaboth , H. Kaji , T. Kajita , H. Kakuno , J. Kameda , Y. Kanazawa , D. Karlen , I. Karpikov , E. Kearns , M. Khabibullin , F. Khanam , A. Khotjantsev , D. Kielczewska , T. Kikawa , A. Kilinski , J. Y. Kim , J. Kim , S. B. Kim , B. Kirby , J. Kisiel , P. Kitching , T. Kobayashi , G. Kogan , A. Kolaceke , A. Konaka , L. L. Kormos , A. Korzenev , K. Koseki , Y. Koshio , K. Kowalik , I. Kreslo , W. Kropp , H. Kubo , Y. Kudenko , S. Kumaratunga , R. Kurjata , T. Kutter , J. Lagoda , K. Laihem , A. Laing , M. Laveder , M. Lawe , M. Lazos , K. P. Lee , C. Licciardi , I. T. Lim , T. Lindner , C. Lister , R. P. Litchfield , A. Longhin , G. D. Lopez , L. Ludovici , M. Macaire , L. Magaletti , K. Mahn , M. Malek , S. Manly , A. Marchionni , A. D. Marino , J. Marteau , J. F. Martin , T. Maruyama , J. Marzec , P. Masliah , E. L. Mathie , V. Matveev , K. Mavrokoridis , E. Mazzucato , N. McCauley , K. S. McFarland , C. McGrew , T. McLachlan , M. Messina , C. Metelko , M. Mezzetto , P. Mijakowski , C. A. Miller , A. Minamino , O. Mineev , S. Mine , A. Missert , M. Miura , L. Monfregola , S. Moriyama , Th. A. Mueller , A. Murakami , M. Murdoch , S. Murphy , J. Myslik , T. Nagasaki , T. Nakadaira , M. Nakahata , T. Nakai , K. Nakajima , K. Nakamura , S. Nakayama , T. Nakaya , K. Nakayoshi , D. Naples , T. C. Nicholls , C. Nielsen , M. Nirkko , K. Nishikawa , Y. Nishimura , H. M. O'Keeffe , Y. Obayashi , R. Ohta , K. Okumura , T. Okusawa , W. Oryszczak , S. M. Oser , M. Otani , R. A. Owen , Y. Oyama , M. Y. Pac , V. Palladino , V. Paolone , D. Payne , G. F. Pearce , O. Perevozchikov , J. D. Perkin , Y. Petrov , E. S. Pinzon Guerra , P. Plonski , E. Poplawska , B. Popov , M. Posiadala , J. -M. Poutissou , R. Poutissou , P. Przewlocki , B. Quilain , E. Radicioni , P. N. Ratoff , M. Ravonel , M. A. M. Rayner , M. Reeves , E. Reinherz-Aronis , F. Retiere , A. Robert , P. A. Rodrigues , E. Rondio , S. Roth , A. Rubbia , D. Ruterbories , R. Sacco , K. Sakashita , F. Sanchez , E. Scantamburlo , K. Scholberg , J. Schwehr , M. Scott , D. I. Scully , Y. Seiya , T. Sekiguchi , H. Sekiya , D. Sgalaberna , M. Shibata , M. Shiozawa , S. Short , Y. Shustrov , P. Sinclair , B. Smith , R. J. Smith , M. Smy , J. T. Sobczyk , H. Sobel , M. Sorel , L. Southwell , P. Stamoulis , J. Steinmann , B. Still , A. Suzuki , K. Suzuki , S. Y. Suzuki , Y. Suzuki , T. Szeglowski , M. Szeptycka , R. Tacik , M. Tada , S. Takahashi , A. Takeda , Y. Takeuchi , H. A. Tanaka , M. M. Tanaka , M. Tanaka , I. J. Taylor , D. Terhorst , R. Terri , L. F. Thompson , A. Thorley , S. Tobayama , W. Toki , T. Tomura , Y. Totsuka , C. Touramanis , T. Tsukamoto , M. Tzanov , Y. Uchida , K. Ueno , A. Vacheret , M. Vagins , G. Vasseur , T. Wachala , A. V. Waldron , C. W. Walter , D. Wark , M. O. Wascko , A. Weber , R. Wendell , R. J. Wilkes , M. J. Wilking , C. Wilkinson , Z. Williamson , J. R. Wilson , R. J. Wilson , T. Wongjirad , Y. Yamada , K. Yamamoto , C. Yanagisawa , S. Yen , N. Yershov , M. Yokoyama , T. Yuan , A. Zalewska , L. Zambelli , K. Zaremba , M. Ziembicki , E. D. Zimmerman , M. Zito , J. Zmuda

Neutrino-electron scatterings are purely leptonic processes with robust Standard Model (SM) predictions. Their measurements can therefore provide constraints to physics beyond SM. The $\nuebar$-e data taken at the Kuo-Sheng Reactor Neutrino…

High Energy Physics - Phenomenology · Physics 2014-11-21 M. Deniz er al. , TEXONO Collaboration

In preparation to the experimental results which will be available in the future, we study geo-neutrino production for different models of mantle convection and composition. By using global mass balance for the Bulk Silicate Earth, the…

Geophysics · Physics 2011-01-04 Gianni Fiorentini , Marcello Lissia , Fabio Mantovani , Riccardo Vannucci

In this paper we introduce the concept of what we call "NUDAR" (NeUtrino Direction and Ranging), making the point that measurements of the observed energy and direction vectors can be employed to passively deduce the exact three-dimensional…

The result of the 3-year neutrino magnetic moment measurement at the Kalinin Nuclear Power Plant with the GEMMA spectrometer is presented. Antineutrino-electron scattering is investigated. A high-purity germanium detector of 1.5 kg placed…

High Energy Physics - Experiment · Physics 2010-11-26 A. G. Beda , V. B. Brudanin , E. V. Demidova , V. G. Egorov , D. V. Medvedev , M. V. Shirchenko , A. S. Starostin , Ts. Vylov

In this paper we do a three-generation oscillation analysis of the latest (848 days) Super-Kamiokande (SK) atmospheric neutrino data going beyond the one mass scale dominance (OMSD) approximation. We fix $\Delta_{12} = \Delta_{13}$…

High Energy Physics - Phenomenology · Physics 2011-05-23 Sandhya Choubey , Srubabati Goswami , Kamales Kar

In the framework of the Standard Model with lepton mixing the radiative decay $\nu_i \rightarrow \nu_j \gamma$ of a neutrino of high ($E_\nu \sim 100 \, GeV$) and super-high ($E_\nu \ge 1 \, TeV$) energy is investigated in the Coulomb field…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. A. Gvozdev , N. V. Mikheev , L. A. Vassilevskaya

In the framework of quantum open systems we analyze data from KamLAND by using a model that considers neutrino oscillation in a three-family approximation with the inclusion of the decoherence effect. Using a $\chi^2$ test we find new…

High Energy Physics - Phenomenology · Physics 2017-06-28 G. Balieiro Gomes , M. M. Guzzo , P. C. de Holanda , R. L. N. Oliveira
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