Includes bibliographical references.
|Statement||edited by Y. Suzuki ... [et al.]|
|Series||Frontiers science series -- no. 35.|
|LC Classifications||QC793.5.N42 W67 2000|
|The Physical Object|
|Pagination||xi, 380 p. :|
|Number of Pages||380|
Neutrino Oscillations and Their Origin: Proceedings of the Third International Workshop Tokyo, Japan 5 - 8 December Y. Suzuki, Y. Fukuda, T. Takeuchi, T. Mori, T. Yoshida This work covers topics such as the latest solar neutrino results in super-kamiokande, weak current in deuterium, proton decay in the semi-simple unification model. Studies of atmospheric neutrinos at a variety of detectors yield a consistent picture of neutrino oscillations, ie. that muon neutrinos oscillate to tau neutrinos with nearly maximal mixing and a mass splitting in the range of a few meV 2. In this article, emphasis will be given to the high-statistics. The aim of this workshop was to put together the efforts from various fields necessary for understanding neutrino oscillations in detail, from both experimental and theoretical points of view. One of the main experimental issues was to understand the absolute flux of both the atmospheric and the solar neutrinos in order to obtain detailed parameter information on neutrino oscillations. The XMASS project is a plan to explore the low background frontier by using ultra-pure liquid xenon. The aims of this project are to observe low-energy solar neutrinos, to search for neutrino-less double beta decays, and to detect WIMP dark matter. Experimental results from a prototype detector, kg liquid xenon detector, are discussed.
Quick Search in Books. Enter words / phrases / DOI / ISBN / keywords / authors / etc. Search. Quick Search anywhere. Enter words / phrases / DOI / ISBN / keywords / authors / etc. Search. Quick search in Citations. Journal Year Volume Issue Page. Search. Advanced . From the point of view of the Earth tomography, these oscillations have a number of advantages over the oscillations of the accelerator or atmospheric neutrinos, which stem from the fact that. Title: Neutrino oscillations: brief history and present status. Authors: S. M. Bilenky (Submitted on 12 Aug ) Abstract: A brief review of the problem of neutrino masses and oscillations is given. In the beginning we present an early history of neutrino masses, mixing and oscillations. Then we discuss all possibilities of neutrino masses and Cited by: 7. Fermi theory of β-decay discovery of ν¯e by Cowan and Reines (NP ) Pontecorvo suggests neutrino oscillations helicity h(νe) = −1 by Goldhaber ⇒ V−A discovery of νµ by Lederman, Steinberger, Schwartz (NP ) ﬁrst discovery of solar neutrinos by Ray Davis (NP ); solar neutrino.
Neutrino oscillations G. Bellini 1, L. Ludhova, G. Ranucci, F.L. Villante2 1Dip. di Fisica, Universit a degli Studi and INFN, Milano, Italy 2Dip. di Scienze Fisiche e Chimiche, Universit a degli Studi and INFN, L’Aquila, Italy Septem Abstract In the last decades, a very important breakthrough has been brought in the elementary particle physicsFile Size: 3MB. The discovery of neutrino oscillations in initiated efforts to form a group to work on the detailed study of the phenomenon. The 4th International Workshop on Neutrino Oscillations and Their Origin was held to discuss progress in both experimental and theoretical study. Title: The Fifth International Workshop on Neutrino Oscillations and their Origin: Tokyo, Japan, February Authors: Suzuki, Y. Publication. Gary Feldman Neutrino Oscillations Oscillations (continued) In general, oscillations will decouple so that they can be approximated by a two-neutrino oscillation: ν α νβ = cos θ sin θ − sin θ cos θ ν 1 ν 2, and P(ν α → νβ) = sin 2 (2 θ)sin 2 ∆ m 12 2 L EFile Size: 1MB.