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Related papers: Testing LSND at long-baseline neutrino experiments

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Positive evidence for neutrino oscillations is mounting from the solar and atmospheric neutrino anomalies and the LSND experiment. Accordingly, the neutrino mass differences appear to lie in the sub-eV range and at least some of the mixing…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Raffelt

The long awaited experimental results from MiniBooNE have recently been announced. This experiment tests whether neutrino oscillations can occur at a higher mass squared difference $\sim1 {eV}^2$ compared to well established observations of…

Popular Physics · Physics 2008-11-26 Ranjan Laha , Sudhir K. Vempati

It is shown that at least four massive neutrinos are needed in order to accommodate the evidences in favor of neutrino oscillations found in solar and atmospheric neutrino experiments and in the LSND experiment. Among all four-neutrino…

High Energy Physics - Phenomenology · Physics 2007-05-23 Carlo Giunti

It is shown that at least four massive neutrinos are needed in order to accommodate the evidences in favor of neutrino oscillations found in solar and atmospheric neutrino experiments and in the LSND experiment. Among all four-neutrino…

High Energy Physics - Phenomenology · Physics 2011-04-15 Carlo Giunti

It is shown that at least four massive neutrinos are needed in order to accommodate the evidences in favor of neutrino oscillations found in solar and atmospheric neutrino experiments and in the LSND experiment. Among all four-neutrino…

High Energy Physics - Phenomenology · Physics 2007-05-23 Carlo Giunti

Evidences in favor of neutrino oscillations, obtained in the solar and atmospheric neutrino experiments, are discussed. Neutrino oscillations in the solar and atmospheric ranges of the neutrino mass-squared differences are considered in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. M. Bilenky

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…

High Energy Physics - Phenomenology · Physics 2007-05-23 V. Barger

Our knowledge of the neutrino sector of the Standard Model has recently undergone a revolution. Deficits of the atmospheric muon neutrino flux and the solar electron neutrino flux compared to their predicted values can be understood in…

High Energy Physics - Phenomenology · Physics 2009-10-31 V. Barger

We present the results of an analysis of the data of reactor and accelerator neutrino oscillation experiments in the framework of a model with mixing of three massive neutrino fields and a neutrino mass hierarchy. The results of the LSND…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. M. Bilenky , A. Bottino , C. Giunti , C. W. Kim

We consider a class of theories in which neutrino masses depend significantly on environment, as a result of interactions with the dark sector. Such theories of mass varying neutrinos (MaVaNs) were recently introduced to explain the origin…

High Energy Physics - Phenomenology · Physics 2009-11-10 David B. Kaplan , Ann E. Nelson , Neal Weiner

Measurements of various features of the fluxes of atmospheric and solar neutrinos have provided evidence for neutrino oscillations and therefore for neutrino masses and mixing. We review the phenomenology of neutrino oscillations in vacuum…

High Energy Physics - Phenomenology · Physics 2009-09-29 M. C. Gonzalez-Garcia , Y. Nir

SNO's neutral current measurement has added a new piece to the emerging neutrino physics puzzle. Putting together the presently available experimental information, an essentially unique picture emerges: The solar neutrino anomaly is…

High Energy Physics - Phenomenology · Physics 2009-11-07 R. Foot , R. R. Volkas

We discuss all possible schemes with four massive neutrinos inspired by the existing experimental indications in favour of neutrino mixing, namely the atmospheric, solar and LSND neutrino experiments. We argue that the scheme with a…

High Energy Physics - Phenomenology · Physics 2011-04-15 W. Grimus

We construct a mass matrix for the four neutrino flavors, three active and one sterile, needed to fit oscillations in all three neutrino experiments: atmospheric, solar, and LSND, simultaneously. It organizes the neutrinos into two doublets…

High Energy Physics - Phenomenology · Physics 2011-02-07 James M. Gelb , S. P. Rosen

Observations of atmospheric neutrinos offer compelling evidence that neutrinos have mass and do oscillate. Preliminary data are compatible with maximal $\nu_\mu$--$\nu_\tau$ mixing, but not with pure $\nu_\mu$--$\nu_e$ mixing. In a general…

High Energy Physics - Phenomenology · Physics 2007-05-23 Howard Georgi , Sheldon L. Glashow

The current case for atmospheric $\nu_\mu$ oscillations into active or sterile neutrinos is reviewed. It is argued that neither the study of neutral current events at Super-Kamiokande, nor the information obtained from future long baseline…

High Energy Physics - Phenomenology · Physics 2011-09-13 Achim Geiser

The three neutrino mass matrices in the $SU(5)\times U(2)$ model are studied focusing on the neutrino oscillation experiments. The atmospheric neutrino anomaly could be explained by the large $\nu_{\mu} - \nu_{\tau}$ oscillation. The long…

High Energy Physics - Phenomenology · Physics 2011-02-11 Morimitsu Tanimoto

We make a model-independent analysis of all available data that indicate neutrino oscillations. Using probability diagrams, we confirm that a mass spectrum with two nearly degenerate pairs of neutrinos separated by a mass gap of $\simeq1$…

High Energy Physics - Phenomenology · Physics 2009-08-07 V. Barger , S. Pakvasa , T. J. Weiler , K. Whisnant

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…

High Energy Physics - Phenomenology · Physics 2009-08-07 Srubabati Goswami

We suggest the possibility that the anomalies observed in the LSND experiment and the Gallium radioactive source experiments may be due to neutrino oscillations generated by a large squared-mass difference of about 20 - 30 eV^2. We consider…

High Energy Physics - Phenomenology · Physics 2008-11-26 Carlo Giunti , Marco Laveder
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