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相关论文: Three flavor implications of CHOOZ result

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We analyze the atmospheric neutrino data in the context of three flavor neutrino oscillations taking account of the matter effects in the earth. With the hierarchy among the vacuum mass eigenvalues $\mu_3^2 \gg \mu_2^2 \geq \mu_1^2$, the…

高能物理 - 唯象学 · 物理学 2009-10-28 Mohan Narayan , G. Rajasekaran , S. Uma Sankar

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 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

Deviations from expectations have been claimed for solar, atmospheric and high energy prompt neutrinos from charm decay. This information, supplemented only by the existing very good upper limits for oscillations of the $\nu_{\mu}$ at…

高能物理 - 唯象学 · 物理学 2011-05-23 G. Conforto , A. Marchionni , F. Martelli , F. Vetrano , M. Lanfranchi , G. Torricelli-Ciamponi

The simplest explanation for the atmospheric neutrino anomaly is the transition of muon neutrinos and antineutrinos into states of different flavor. Data from the reactor experiment Chooz, and the measurement of the energy and angle…

高能物理 - 唯象学 · 物理学 2014-11-17 Paolo Lipari , Maurizio Lusignoli

We analyze the solar and the atmospheric neutrino problems in the context of three flavour neutrino oscillations. We assume a mass hierarchy in the vacuum mass eigenvalues $\mu_3^2 \gg \mu_2^2 \geq \mu_1^2$, but make no approximation…

高能物理 - 唯象学 · 物理学 2008-11-26 Mohan Narayan , M. V. N. Murthy , G. Rajasekaran , S. Uma Sankar

Results of a new analysis of the CHOOZ data, performed in the framework of three-neutrino mixing, are presented. Both the cases of normal and inverted neutrino mass hierarchy are considered. The parameters characterizing the solar neutrino…

高能物理 - 唯象学 · 物理学 2015-06-25 S. M. Bilenky , D. Nicolo , S. T. Petcov

Neutrino oscillation scenarios involving large angle $\nu_{\mu} \to \nu_e$ oscillations are disfavoured in the parameter range $\Delta m^2/eV^2 >~ 10^{-3}$ by recent results from the CHOOZ reactor-based $\bar{\nu}_e$ disappearance…

高能物理 - 唯象学 · 物理学 2007-05-23 R. Foot , R. R. Volkas , O. Yasuda

The basics of neutrino oscillations is presented. Existing evidences of neutrino oscillations, obtained in the atmospheric and solar neutrino experiments, are considered. The new CHOOZ bound on the element $|U_{e3}|^{2}$, obtained from the…

高能物理 - 唯象学 · 物理学 2007-05-23 S. M. Bilenky

With one \Delta m^2 of the appropriate order of magnitude to solve the atmospheric neutrino problem, we study the resulting three-generation vacuum-oscillation fit to the solar neutrino flux. An explanation of the atmospheric neutrino…

高能物理 - 唯象学 · 物理学 2009-10-31 P. Osland , G. Vigdel

Three interesting scenarios for neutrino mixing, i.e., (i) small-large mixing scenario, (ii) nearly bi-maximal mixing scenario and (iii) three-flavor oscillation scenario, are analyzed in connection with three possible assignments of the…

高能物理 - 唯象学 · 物理学 2014-11-17 Yue-Liang Wu

Using the result of the three flavor analysis of the old Kamiokande data, the recent Superkamiokande data of atmospheric neutrinos and the CHOOZ reactor data, it is shown that the third mixing angle $\theta_{13}$ is small. It is proposed to…

高能物理 - 唯象学 · 物理学 2011-04-15 Osamu Yasuda

It is shown that it is possible to account for all three experimental indications for neutrino oscillations with just three neutrino flavors. In particular, we suggest that the solar and atmospheric neutrino anomalies are to be explained by…

高能物理 - 唯象学 · 物理学 2009-10-30 A. Acker , S. Pakvasa

Global fits to all data of candidates for neutrino oscillations are presented in the framework of a three-flavor model. The analysis excludes mass regions where the MSW effect is important for the solar neutrino problem. The best fit gives…

高能物理 - 唯象学 · 物理学 2016-08-25 Tommy Ohlsson , Hakan Snellman

We show that if the solar and atmospheric data are both described by maximal vacuum oscillations at the relevant mass scales then there exists a unique mixing matrix for three neutrino flavors. The solution necessarily conserves CP and…

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

We show how the nearly bi-maximal mixing scenario comes out naturally from gauged $SO(3)_{F}$ flavor symmetry via spontaneous symmetry breaking. An interesting relation between the neutrino mass-squared differences and the mixing angle,…

高能物理 - 唯象学 · 物理学 2007-05-23 Yue-Liang Wu

Assuming three flavour neutrino mixing takes place in vacuum, we investigate the possibility that the solar $\nu_e$ take part in MSW transitions in the Sun due to $\Delta m^2_{31} \sim (10^{-7} - 10^{-4})~eV^2$, followed by long wave length…

高能物理 - 唯象学 · 物理学 2007-05-23 Qiu-Yu Liu

Some implications of the proposal that flavor nondiagonal couplings of neutrinos to gravity might resolve the solar neutrino problem are considered in the context of three neutrino flavors. The two--flavor model is discussed as a limiting…

高能物理 - 唯象学 · 物理学 2009-10-28 J. R. Mureika , R. B. Mann

We present a solution of the solar neutrino deficit using three flavors of neutrinos within the R-parity non-conserving supersymmetric model. In vacuum, mass and mixing is restricted to the nu(mu)-nu(tau) sector only, which we choose in…

高能物理 - 唯象学 · 物理学 2009-01-07 Rathin Adhikari , Arunansu Sil , Amitava Raychaudhuri

We derive the constraints imposed on neutrino masses and mixing angles by performing a combined analysis of the data from the Los Alamos and the other terrestrial neutrino oscillation experiments with the assumption of the flavor-mixing…

高能物理 - 唯象学 · 物理学 2010-11-01 Hisakazu Minakata
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