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相关论文: Maximal neutrino oscillation solution to the solar…

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The L/E-flatness of the e-like events observed in the recent atmospheric-neutrino data from Super-Kamiokande (SuperK) is interpreted to reflect a new symmetry of the neutrino-oscillation mixing matrix. From that we obtain an analytical set…

高能物理 - 唯象学 · 物理学 2016-09-06 D. V. Ahluwalia

A natural solution to the fermion mass hierarchy problem suggests the existence of a partially conserved chiral symmetry. We show that this can lead to a reasonably natural solution to the solar and atmospheric neutrino problems without…

高能物理 - 唯象学 · 物理学 2009-10-31 C. D. Froggatt , M. Gibson , H. B. Nielsen

The study of solar neutrinos has given since ever a fundamental contribution both to astroparticle and to elementary particle physics, offering an ideal test of solar models and offering at the same time relevant indications on the…

高能物理 - 实验 · 物理学 2012-08-16 V. Antonelli , L. Miramonti , C. Pena-Garay , A. Serenelli

We determine the three-neutrino mixing and mass parameters that are allowed by the solar and atmospheric neutrino data when vacuum oscillations are responsible for both phenomena. The global fit does not appreciably change the allowed…

高能物理 - 唯象学 · 物理学 2009-08-07 V. Barger , K. Whisnant

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

Motivated by the Exact Parity Model and other theories, the hypothesis that each of the known neutrinos oscillates maximally with a sterile partner has been put forward as an explanation of the atmospheric and solar neutrino anomalies. We…

高能物理 - 唯象学 · 物理学 2011-03-10 R. Foot , R. R. Volkas , O. Yasuda

Neutrino oscillations with parameters relevant for the large mixing solution of the solar neutrino problem ($\Delta m^2_{21} = (2 - 20) \cdot 10^{-5}$ eV$^2$, $\sin^2 2\theta_{12} > 0.65$) can lead to observable (up to 10 - 12 %) excess of…

高能物理 - 唯象学 · 物理学 2009-10-31 O. L. G. Peres , A. Y. Smirnov

The status of the solar neutrino problem is reviewed. Attempts to explain the observed deficit and spectral distortion, both by astrophysical and particle physics methods, are described. It is argued that the comparison of all experiments…

高能物理 - 唯象学 · 物理学 2011-06-02 Paul Langacker

Solar and atmospheric neutrino anomalies are described by bimaximal mixing of three neutrinos. Neutrino oscillations in appearance nu_e <--> nu_mu,nu_tau and in disappearance nu_e long baseline and atmospheric experiments are sensitive to…

高能物理 - 唯象学 · 物理学 2009-10-31 M. Jezabek , Y. Sumino

The recent experimental results indicating the neutrino oscillations may strongly suggest that at least one more light neutrino species is required in order to reconcile the existing data. In the simple GUT frameworks, this fact seems…

高能物理 - 唯象学 · 物理学 2009-10-31 Masako Bando , Koichi Yoshioka

We present a supersymmetric model of dark energy from Mass Varying Neutrinos which is stable against radiative corrections to masses and couplings, and free of dynamical instabilities. This is the only such model of dark energy involving…

高能物理 - 唯象学 · 物理学 2009-11-11 Rob Fardon , Ann E. Nelson , Neal Weiner

Long length vacuum oscillations solution of the solar neutrino problem is discussed. We show that there is a strict correlation between a distortion of the neutrino energy spectrum and an amplitude of seasonal variations of the neutrino…

高能物理 - 唯象学 · 物理学 2009-10-30 S. P. Mikheyev , A. Yu. Smirnov

The three active light neutrinos are used to explain the neutrino oscillations. The inherently bi-large mixing neutrino mass matrix and the Fritzsch type, bi-small mixing charged lepton mass matrix are assumed. By requiring the maximal…

高能物理 - 唯象学 · 物理学 2014-11-17 Chun Liu , Jeonghyeon Song

In the Supersymmetric extension of the Standard Model with minimal particle content the three neutrinos can have non trivial masses and mixings, generated at 1 loop due to renormalizable lepton number violating interactions. We show that…

高能物理 - 唯象学 · 物理学 2009-09-25 D. Tommasini

Zee model leads naturally to two heavy, strongly degenerate and almost maximally mixed neutrinos and to one light neutrino with small mixing. This pattern coincides with the one needed for a solution of the atmospheric neutrino problem by…

高能物理 - 唯象学 · 物理学 2009-10-28 Alexei Yu. Smirnov , Morimitsu Tanimoto

The data from all solar neutrino experiments presented at the Neutrino 98 conference has been analyzed and a brief summary of the status of the two most popular neutrino solutions of the solar neutrino problem, the MSW mechanism and vacuum…

高能物理 - 唯象学 · 物理学 2007-05-23 P. I. Krastev

We take as a starting point the Gelmini -- Roncadelli model enlarged by a term with explicit lepton number violation in the Higgs potential and add a neutrino singlet field coupled via a scalar doublet to the usual leptons. This scenario…

高能物理 - 唯象学 · 物理学 2011-09-13 W. Grimus , R. Pfeiffer , T. Schwetz

We discuss general predictions for neutrino masses and mixing angles from R parity violation in the Minimal Supersymmetric Standard Model. If the soft supersymmetry breaking terms are flavor blind at short distance, then the leptonic…

高能物理 - 唯象学 · 物理学 2014-11-17 D. Elazzar Kaplan , Ann E. Nelson

Models with three active neutrinos and one sterile neutrino can naturally account for maximal oscillations of atmospheric neutrinos, explain the solar neutrino deficit, and accommodate the results of the LSND experiment. The models predict…

高能物理 - 唯象学 · 物理学 2007-05-23 V. Barger

We perform an updated phenomenological analysis of the Mikheyev-Smirnov-Wolfenstein (MSW) solutions of the solar neutrino problem, assuming oscillations between two and three neutrino families. The analysis includes the total rates of the…

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