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We perform a global three generation analysis of the current solar and atmospheric evidence in favor of neutrino oscillations. We also include the negative results coming from CHOOZ to constrain the nu_e mixing. We study the zones of…

高能物理 - 唯象学 · 物理学 2007-05-23 G. L. Fogli , E. Lisi , A. Marrone , D. Montanino , A. Palazzo

We present an up-to-date global analysis of solar, atmospheric, reactor and accelerator neutrino data in the framework of three-neutrino oscillations. We discuss in detail the statistical significance of the observed "hint" of non-zero…

高能物理 - 唯象学 · 物理学 2011-06-17 M. C. Gonzalez-Garcia , Michele Maltoni , Jordi Salvado

We determine the neutrino parameters for MSW and vacuum oscillations (active and sterile neutrinos) that are allowed by the separate, and collective, imposition of the constraints from total event rates in the chlorine, GALLEX, SAGE, and…

高能物理 - 唯象学 · 物理学 2009-03-02 J. N. Bahcall , P. I. Krastev , A. Yu. Smirnov

Effects of the 1-3 leptonic mixing on the solar neutrino observables are studied and the signatures of non-zero $\theta_{13}$ are identified. For this we have re-derived the formula for $3\nu$-survival probability including all relevant…

高能物理 - 唯象学 · 物理学 2009-11-10 Srubabati Goswami , Alexei Yu. Smirnov

We study neutrino oscillations and the level-crossing probability PLZ in power-law potential profiles A(r)\propto r^n. We give local and global adiabaticity conditions valid for all mixing angles theta and discuss different representations…

高能物理 - 唯象学 · 物理学 2009-09-25 M. Kachelriess , A. Strumia , R. Tomas , J. W. F. Valle

This article summarises the status of the solar neutrino oscillation phenomenology at the end of 2002 in the light of the SNO and KamLAND results. We first present the allowed areas obtained from global solar analysis and demonstrate the…

高能物理 - 唯象学 · 物理学 2008-11-26 Srubabati Goswami

We make a general study of possibility of generating solar scale $\Delta_{\odot}$ and the CHOOZ angle $U_{e3}$ radiatively by assuming that they are zero at some high scale. The most general neutrino mass matrix leading to this result is…

高能物理 - 唯象学 · 物理学 2014-11-17 Anjan S. Joshipura

We present "Before and After" global oscillation solutions, as well as predicted "Before and After" values and ranges for ten future solar neutrino observables (for BOREXINO, KamLAND, SNO, and a generic p-p neutrino detector). We have…

高能物理 - 唯象学 · 物理学 2009-11-07 John N. Bahcall , M. C. Gonzalez-Garcia , Carlos Peña-Garay

We present a global analysis of all the available solar neutrino data treating consistently the 8B and hep neutrino fluxes as free parameters. The analysis reveals at 99.7% C.L. eight currently-allowed discrete regions in two-neutrino…

高能物理 - 唯象学 · 物理学 2010-02-03 John N. Bahcall , Plamen I. Krastev , Alexei Yu. Smirnov

We have analyzed the most recent available Super-Kamiokande data in a three flavor neutrino oscillation model. We have here neglected possible matter effects and performed a fit to atmospheric and solar Super-Kamiokande data. We have…

高能物理 - 唯象学 · 物理学 2011-09-13 Christoph Meier , Tommy Ohlsson

We study in detail the power of the reactor experiment kamLAND for discriminating existing solutions to the SNP and giving accurate information on neutrino masses and mixing angles. Assuming the expected signal corresponding to various…

高能物理 - 唯象学 · 物理学 2008-11-26 P. Aliani , V. Antonelli , M. Picariello , E. Torrente-Lujan

We present the results of a global analysis of the neutrino oscillation data available as of fall 2018 in the framework of three massive mixed neutrinos with the goal at determining the ranges of allowed values for the six relevant…

高能物理 - 唯象学 · 物理学 2019-02-19 Ivan Esteban , M. C. Gonzalez-Garcia , Alvaro Hernandez-Cabezudo , Michele Maltoni , Thomas Schwetz

We present a systematic analysis of the three-flavor Mikheyev-Smirnov-Wolfenstein (MSW) oscillation solutions to the solar neutrino problem, in the hypothesis that the two independent neutrino square mass differences, $\delta m^2$ and…

高能物理 - 唯象学 · 物理学 2009-10-07 G. L. Fogli , E. Lisi , D. Montanino

We determine the neutrino mixing and mass parameters that are allowed by the Super-Kamiokande atmospheric neutrino data in a three-neutrino model with one mass-squared difference contributing to the oscillations. We find that although…

高能物理 - 唯象学 · 物理学 2009-09-15 V. Barger , T. J. Weiler , K. Whisnant

Neutrino masses and their mixing are studied in detail in the framework of a supersymmetric standard model with bilinear R-parity violation. In this scenario, the mixing matrix among the neutrinos is in a restrictive form. We find that only…

高能物理 - 唯象学 · 物理学 2008-11-26 Fumihiro Takayama , Masahiro Yamaguchi

We have considered the results of solar and atmospheric neutrino oscillation experiments in the scheme of mixing of three neutrinos with a mass hierarchy. It is shown that the recent results of the CHOOZ experiment imply that |U_{e3}|^2<<1…

高能物理 - 唯象学 · 物理学 2008-11-26 S. M. Bilenky , C. Giunti

We analyzed the solar, terrestrial and atmospheric neutrinos experiments using the three-flavor neutrino framework and got the allowed regions for parameters (\Delta m_{12}^2, \sin^22\theta_{12}, \Delta m_{23}^2, \theta_{13}, \theta_{23}).…

高能物理 - 唯象学 · 物理学 2016-09-06 T. Teshima , T. Sakai , O. Inagaki

A global analysis of the data from all the solar neutrino experiments combined with the recent KamLAND data is presented. A formula frequently used in the literature gives survival probability for three active solar neutrino flavors in…

高能物理 - 唯象学 · 物理学 2008-11-26 A. B. Balantekin , H. Yuksel

We present new constraints on the neutrino oscillation parameters $/textyen Delta m^{2}_{21}$, $/textyen theta_{12}$, and $/textyen theta_{13}$ from a three-flavor analysis of solar and KamLAND data. The KamLAND data set includes data…

高能物理 - 实验 · 物理学 2012-08-27 The KamLAND Collaboration

The results of a solar model independent analysis of the existing solar neutrino data under the assumption of MSW transitions in matter or vacuum oscillations (in the cases of $\nu_{e}$--$\nu_{\mu}(\nu_{\tau})$ and…

高能物理 - 唯象学 · 物理学 2009-10-28 S. M. Bilenky , C. Giunti