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相关论文: The MSW conversion of solar neutrinos and random m…

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We present a generalization of the resonant neutrino conversion in matter, including a random component in the matter density profile. The study is focused on the effect of such matter perturbations upon both large and small mixing angle…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Rossi

We consider the implications of solar matter density random noise upon resonant neutrino conversion. The evolution equation describing MSW-like conversion is derived in the framework of the Schr\"odinger approach. We study quantitatively…

高能物理 - 唯象学 · 物理学 2009-09-17 H. Nunokawa , A. Rossi , V. B. Semikoz , J. W. F. Valle

We present the evolution equation describing MSW conversion, derived in the framework of the Schr\"odinger approach, in the presence of matter density fluctuations. Then we analyse the effect of such fluctuations in the MSW scenario as a…

高能物理 - 唯象学 · 物理学 2009-10-28 Anna Rossi

We study the effect of random matter density fluctuations in the sun on resonant neutrino conversion in matter by solving numerically the evolution equation for the neutrino system including the full effect of the random matter density…

高能物理 - 唯象学 · 物理学 2007-05-23 A. A. Bykov , M. C. Gonzalez-Garcia , C. Peña-Garay , V. Yu. Popov , V. B. Semikoz

Large mixing MSW solutions to the solar neutrino problem appear to be currently favored by the data. We discuss the possibility of discriminating them by means of present and future experiments. In particular, we show that the study of…

高能物理 - 唯象学 · 物理学 2009-11-07 Antonio Palazzo

A new more rigorous and accurate method for treating neutrino oscillations in the context of the MSW effect in a medium is proposed. This leads to a new type of resonance condition which for small mixing angles puts rather stringent…

高能物理 - 唯象学 · 物理学 2009-09-25 G. K. Leontaris , J. D. Vergados

We consider flavor changing effective neutrino interactions in the context of massive neutrinos in the issue of atmospheric neutrinos. Assuming as usual that this is an indication of the oscillation of muon neutrinos into tau neutrinos we…

高能物理 - 唯象学 · 物理学 2007-05-23 J. C. Montero , V. Pleitez

We investigate the effects of random density fluctuations on neutrino oscillations in the Sun environment. We show how the average of certain quantities which can be used to describe the MSW effect can be computed analytically. We examine…

高能物理 - 唯象学 · 物理学 2016-09-01 Emilio Torrente-Lujan

The large mixing angle (LMA) MSW solution to the solar neutrino problem seems favored by the data at the moment over the small mixing angle (SMA) MSW solution and the vacuum (VAC) solution. In this paper the various main types of models of…

高能物理 - 唯象学 · 物理学 2011-05-12 Ilja Dorsner , S. M. Barr

We consider the effect on matter-enhanced neutrino flavor transformation of a randomly fluctuating, delta-correlated matter density. The fluctuations will produce a distribution of neutrino survival probabilities. We find the mean and…

天体物理学 · 物理学 2008-11-26 A. B. Balantekin , J. M. Fetter , F. N. Loreti

The Lehmann-Newton-Wu mass matrix, which was recently applied to neutrinos, is further investigated. The analytic results presented earlier are confirmed numerically for the solar density profile of the Standard Solar Model. The combined…

高能物理 - 唯象学 · 物理学 2009-10-31 Per Osland , Geir Vigdel

The solar neutrino problem is reviewed and the possible vacuum oscillation and MSW solutions of the problem are considered.

高能物理 - 唯象学 · 物理学 2009-10-31 S. T. Petcov

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

The MSW (Mikheyev-Smirnov-Wolfenstein) effect is the effect of transformation of one neutrino species (flavor) into another one in a medium with varying density. Three basic elements of the effect include: the refraction of neutrinos in…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Yu. Smirnov

The MSW (Mikheyev-Smirnov-Wolfenstein) effect is the adiabatic or partially adiabatic neutrino flavor conversion in medium with varying density. The main notions related to the effect, its dynamics and physical picture are reviewed. The…

高能物理 - 唯象学 · 物理学 2009-11-10 A. Yu. Smirnov

We describe how to consistently incorporate solar model uncertainties, along with experimental errors and correlations, when analyzing solar neutrino data to derive confidence limits on parameter space for proposed solutions of the solar…

高能物理 - 唯象学 · 物理学 2008-11-26 Evalyn Gates , Lawrence M. Krauss , Martin White

We present an exact analytic solution to the neutrino evolution equation in matter with periodic step-function density profile and discuss in detail the parametric resonance of neutrino oscillations that can occur in such a system. Solar…

高能物理 - 唯象学 · 物理学 2008-11-26 E. Kh. Akhmedov

Solar model independent tests of the vacuum oscillation and MSW solutions of the solar neutrino problem are considered. Detailed predictions for time (seasonal) variations of the signals in the future solar neutrino detectors (SNO, Super…

高能物理 - 唯象学 · 物理学 2009-09-25 P. I. Krastev , S. T. Petcov

The status of solar neutrino experiments and their implications for both nonstandard astrophysics ({\it e.g.,} cool sun models) and nonstandard neutrino properties ({\it e.g.,} MSW conversions) are discussed. Assuming that all of the…

高能物理 - 唯象学 · 物理学 2007-05-23 Paul Langacker

In the first part of these lectures the neutrino mixing hypothesis will be considered in detail. We will discuss the possible schemes of neutrino mixing and present the data of the recent experiments searching for effects due to…

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