English
Related papers

Related papers: LSND, SN1987A, and CPT Violation

200 papers

The Kamioka Liquid-scintillator Anti-Neutrino Detector (KamLAND) has detected for the first time the disappearance of electron antineutrinos from a terrestrial source at the 99.95% C.L. Interpreted in terms of neutrino oscillations, the…

High Energy Physics - Experiment · Physics 2011-07-19 Jason Detwiler

Standard active--sterile neutrino oscillations do not provide a satisfactory description of the LSND evidence for neutrino oscillations together with the constraints from MiniBooNE and other null-result short-baseline oscillation…

High Energy Physics - Phenomenology · Physics 2010-02-03 Thomas Schwetz

A search for muon anti-neutrino to electron anti-neutrino oscillations was conducted by the Liquid Scintillator Neutrino Detector at the Los Alamos Neutron Science Center using muon anti-neutrinos from positive muon decay at rest. A total…

Neutrino oscillations in the presence of Lorentz violation can present novel observable signals in both long- and short-baseline experiments. In this talk we describe the theory and its different regimes depending on properties of the…

High Energy Physics - Phenomenology · Physics 2017-08-23 Jorge S. Diaz

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…

High Energy Physics - Phenomenology · Physics 2010-04-01 C. R. Das , Joao Pulido

A set of quantitative predictions for the day-night asymmetry in the Super - Kamiokande detector is presented. For these predictions, neutrino events are collected in ``samples'' defined by the trajectories in the Earth of the corresponding…

High Energy Physics - Phenomenology · Physics 2007-05-23 Michele Maris

We consider neutrino oscillations in the minimal Standard-Model Extension describing general Lorentz and CPT violation. Among the models without neutrino mass differences is one with two degrees of freedom that reproduces most major…

High Energy Physics - Phenomenology · Physics 2009-07-09 Alan Kostelecky , Matthew Mewes

The IsoDAR antineutrino source, which produces a flux from 8Li isotope decay at rest, when paired with the proposed JUNO (Jiangmen Underground Neutrino Observatory) detector, has unprecedented sensitivity to anti-nu_e disappearance for…

High Energy Physics - Experiment · Physics 2014-03-19 J. M. Conrad , M. H. Shaevitz

Using the results of a high precision calculation of the solar neutrino survival probability for Earth crossing neutrinos in the case of MSW $\nu_e --> \nu_s$ transition solution of the solar neutrino problem, we derive predictions for the…

High Energy Physics - Phenomenology · Physics 2016-09-06 M. Maris , S. T. Petcov

We perform a fit to the full data set corresponding to 33.3 kt-yr of data of the Super-Kamiokande experiment as well as to all other experiments in order to compare the two most likely solutions to the atmospheric neutrino anomaly in terms…

High Energy Physics - Phenomenology · Physics 2009-03-02 M. C. Gonzalez-Garcia , H. Nunokawa , O. L. G. Peres , J. W. F. Valle

We study oscillations of the high energy atmospheric neutrinos in the Earth into sterile neutrinos with the eV-scale mass. The MSW resonance and parametric enhancement of the $\bar{\nu}_\mu\to\bar{\nu}_s$ oscillations lead to distortion of…

High Energy Physics - Phenomenology · Physics 2015-06-16 Arman Esmaili , Alexei Yu. Smirnov

The question of the existence of light sterile neutrinos is of great interest in many areas of particle physics, astrophysics, and cosmology. Furthermore, should the MiniBooNE experiment at Fermilab confirm the LSND oscillation signal, then…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. T. Garvey , A. Green , C. Green , W. C. Louis , G. B. Mills , G. McGregor , H. Ray , R. Schirato , R. G. Van de Water , D. H. White

We compare, using a three neutrino analysis, the allowed neutrino oscillation parameters and solar neutrino fluxes determined by the experimental data available Before and After Neutrino 2004. New data available after Neutrino2004 include…

High Energy Physics - Phenomenology · Physics 2014-11-17 John N. Bahcall , M. C. Gonzalez-Garcia , Carlos Pena-Garay

It has been proposed that a sterile neutrino \nu_h with m_h \approx 50 MeV and a dominant decay mode (\nu_h -> \nu\gamma) may be the origin of the experimental anomaly observed at LSND. We define a particular model that could also explain…

High Energy Physics - Phenomenology · Physics 2015-06-11 Manuel Masip , Pere Masjuan , Davide Meloni

Day - Night asymmetries and electronic spectra distortions for the Super - Kamiokande detector are computed for the transition nu_e -> nu_mu(tau) and for a set of neutrino parameters. The results show the possibility to enhance up to a…

High Energy Physics - Phenomenology · Physics 2007-05-23 M. Maris S. T. Petcov

We calculate accurately the number of solar neutrino events expected as a function of solar zenith angle, with and without neutrino oscillations, for detectors at the locations of Super-Kamiokande, SNO, and the Gran Sasso National…

High Energy Physics - Phenomenology · Physics 2008-11-26 J. N. Bahcall , P. I. Krastev

Light sterile neutrinos mixing with the active ones have been recently proposed to solve different anomalies observed in short-baseline oscillation experiments. These neutrinos can also be produced by oscillations of the active neutrinos in…

High Energy Physics - Phenomenology · Physics 2013-05-30 Alessandro Mirizzi , Ninetta Saviano , Gennaro Miele , Pasquale Dario Serpico

We investigate the extent to which leptonic CP-violation in (3+2) sterile neutrino models leads to different oscillation probabilities for $\bar{\nu}_{\mu}\to\bar{\nu}_e$ and $\nu_{\mu}\to\nu_e$ oscillations at MiniBooNE. We are using a…

High Energy Physics - Phenomenology · Physics 2014-11-18 G. Karagiorgi , A. Aguilar-Arevalo , J. M. Conrad , M. H. Shaevitz , K. Whisnant , M. Sorel , V. Barger

If the atmospheric and the solar neutrino problem are both explained by neutrino oscillations, and if there are only three light neutrinos, then all mass-squared differences between the neutrinos are known. In such a case, existing…

High Energy Physics - Phenomenology · Physics 2009-10-31 Sven Bergmann , Yuval Grossman

The standard solar model (SSM) yield a $^8$B solar neutrino flux which is consistent within the theoretical and experimental uncertainties with that observed at Super-Kamiokande. The combined results from the Super- Kamiokande and the…

Astrophysics · Physics 2011-04-15 Arnon Dar