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相关论文: Are solar neutrino oscillations robust?

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We perform a global fit to neutrino oscillation and coherent neutrino-nucleus scattering data, using both timing and energy information from the COHERENT experiment. The results are used to set model-independent bounds on four-fermion…

高能物理 - 唯象学 · 物理学 2020-10-05 Pilar Coloma , Ivan Esteban , M. C. Gonzalez-Garcia , Michele Maltoni

Solar and KamLAND data are in slight tension when interpreted in the standard two-flavor oscillations framework and this may be alleviated allowing for a non-zero value of the mixing angle theta_13. Here we show that, likewise, non-standard…

高能物理 - 唯象学 · 物理学 2009-12-01 A. Palazzo , J. W. F. Valle

What can we learn from solar neutrino observations? Is there any solution to the solar neutrino anomaly which is favored by the present experimental panorama? After SNO results, is it possible to affirm that neutrinos have mass? In order to…

高能物理 - 唯象学 · 物理学 2009-11-07 A. M. Gago , M. M. Guzzo , P. C. de Holanda , H. Nunokawa , O. L. G. Peres , V. Pleitez , R. Zukanovich Funchal

In this letter we highlight the inherent problems associted with the inverted hierarchical model of neutrinos with only three generations and suggest possible solutions within the MSSM. we discuss the new parametrisation of the solar mixing…

高能物理 - 唯象学 · 物理学 2009-11-10 Mahadev Patgiri , N. Nimai Singh

The reported signal at the LSND experiment, when interpreted as neutrino mixing with $\delta m^2 = 6 \;\rm{eV}^2$, provides evidence for neutrinos with a cosmologically significant mass. However, attempts to reconcile this interpretation of…

天体物理学 · 物理学 2009-10-28 Christian Y. Cardall , George M. Fuller

Maximum mixing in atmospheric neutrino oscillation, as well as vanishing of the MNS matrix element $U_{e3}$, are consequences of a 2-3 symmetry, under which the neutrino mass matrix is invariant under the interchange of second and third…

高能物理 - 唯象学 · 物理学 2009-11-07 C. S. Lam

The Sudbury Neutrino Observatory (SNO) has measured day and night solar neutrino energy spectra and rates. For charged current events, assuming an undistorted $^8$B spectrum, the night minus day rate is $14.0% \pm 6.3% ^{+1.5}_{-1.4}%$ of…

核实验 · 物理学 2012-08-27 SNO Collaboration

An approximation that is often used in fits to reactor and atmospheric neutrino data and in some studies of future neutrino oscillation experiments is to assume one dominant scale, $\Delta m^2$, of neutrino mass squared differences, in…

高能物理 - 唯象学 · 物理学 2010-05-28 Irina Mocioiu , Robert Shrock

A statistical analysis of the solar neutrino data is presented assuming the solar neutrino deficit to be resolved by the resonant interaction of the neutrino magnetic moment with the solar magnetic field. Four field profiles are…

高能物理 - 唯象学 · 物理学 2011-05-23 Joao Pulido

Within the framework of an SO(10) GUT model that can accommodate both the atmospheric and the LMA solar neutrino mixing solutions, we present explicit predictions for the neutrino oscillation parameters \sin^2 2\theta_{13}, \sin^2…

高能物理 - 唯象学 · 物理学 2009-11-07 Carl H. Albright , S. Geer

We present an analysis of the global neutrino oscillation data including the LSND result in terms of four-neutrino mass schemes and a CPT violating three-neutrino framework. We find that the strong preference of oscillations into active…

高能物理 - 唯象学 · 物理学 2007-05-23 Thomas Schwetz

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

Solar neutrino oscillations are supported by KamLAND's antineutrino measurements, but certain solar neutrino data - the observed shape of the ${}^8$B flux and the difference between day and night counting rates measured in Super-Kamiokande…

高能物理 - 唯象学 · 物理学 2018-01-01 Francesco Vissani

We present the constraints on neutrino oscillation parameters $\Delta m^2_{\odot}$ and $\theta_{\odot}$ governing the solar neutrino oscillations from two generation analysis of solar and KamLAND data. We include the latest 766.3 ton year…

高能物理 - 唯象学 · 物理学 2014-11-18 Srubabati Goswami , Abhijit Bandyopadhyay , Sandhya Choubey

In this paper we use solar neutrino data to derive stringent bounds on Majorana neutrino transition moments (TMs). Should such be present, they would contribute to the neutrino--electron scattering cross section and hence alter the signal…

高能物理 - 唯象学 · 物理学 2008-11-26 W. Grimus , M. Maltoni , T. Schwetz , M. A. Tortola , J. W. F. Valle

It has been known for some time that the well established LMA solution to the observed solar neutrino deficit fails to predict a flat energy spectrum for SuperKamiokande as opposed to what the data indicates. It also leads to a Chlorine…

高能物理 - 唯象学 · 物理学 2010-04-01 C. R. Das , Joao Pulido

We perform a phenomenological analysis of neutrino oscillation in a four generation framework introducing an additional sterile neutrino. In such a scenario, more than one pattern is possible that can accommodate three hieararchically…

高能物理 - 唯象学 · 物理学 2009-08-07 Srubabati Goswami

The physics implications of the just published salt phase data from the SNO experiment are examined. The effect of these data on the allowed ranges of the solar neutrino oscillation parameters, $\Delta_m^2_{21}$ and $\sin^2\theta_{12}$, are…

高能物理 - 唯象学 · 物理学 2010-04-05 Abhijit Bandyopadhyay , Sandhya Choubey , Srubabati Goswami , S. T. Petcov , D. P. Roy

We consider the impact of neutral-current (NC) non-standard neutrino interactions (NSI) on the determination of the neutrino mass ordering. We show that in presence of NSI there is an exact degeneracy which makes it impossible to determine…

高能物理 - 唯象学 · 物理学 2017-04-19 Pilar Coloma , Thomas Schwetz

In the light of the $\nu_\mu\to\nu_e$ neutrino oscillations which may have been observed at the LSND experiment we explore the consequences of two inverted mass schemes where solar neutrino oscillations occur between $\nu_e$ and $\nu_\tau$.…

高能物理 - 唯象学 · 物理学 2016-09-01 G. Raffelt , J. ~Silk