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Solar Models and Neutrino Problem
1982The discrepancy between observed and predicted neutrino capture rate has led us to consider another possibility about the solar interior. The evolutionary sequence of standard models and contaminated solar models are constructed. Both evolutionary study begins with the threshold of stability.
N. Kiziloğlu, D. Ezer
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The Solar Neutrino Problem Revisited
Publications of the Astronomical Society of Australia, 1981The discrepancy between the observed and predicted flux of neutrinos from the Sun is well known. Past attempts at reconciling this difference have been unconvincing (Kuchowicz 1976, Rood 1978), and hence investigations in this area continue.
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The problems with solar neutrinos
AIP Conference Proceedings, 1995Nuclear fusion processes in the center of the sun produce neutrinos as well as photons. Detection of these neutrinos constrains both the intrinsic properties of the neutrinos, such as their mass and mixing, and the models of the sun used to calculate the solar neutrino flux.
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The solar-neutrino problem, 1995
Il Nuovo Cimento C, 1995The status of the Solar-Neutrino Problem (SNP), as is seen in 1995, is reviewed. Basically, there are two principal solutions to the SNP: i) withstandard neutrino (neutrino of SM of electroweak interactions) and ii) withnon-standard neutrino (neutrino beyond the SM).
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Solar neutrino problem still perplexes
Physics World, 1992500 Years after Christopher Columbus sailed from Spain and bumped into something he didn't expect, physicists from around the world gathered at the 15th International Conference on Neutrino Physics and Astrophysics in Granada, Spain, the home of Columbus' patron Queen Isabella, in the hope of running into something unexpected as well.
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THE SOLAR NEUTRINO PROBLEM WITHIN MSW THEORY
Modern Physics Letters A, 1993It is shown that the experiments on solar neutrinos can be accounted in terms of the Mikheyev-Smirnov-Wolfestein theory with ∆m2=6×10−6 eV 2 and sin 2 2θ=7×10−3. In the scenario proposed here the high energy neutrinos, from 8 B , have a survival probability around 1/3, the intermediate ones, around the 7 Be line a very small one ~ 2×10−3 and the low ...
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Neutrino decay solution of the solar neutrino problem revisited.
1992The neutrino decay solution of the solar neutrino problem is revisited in the context of majoron models. It is shown that for a particular range of parameters this scenario reconciles both the Homestake data and the Kamiokande data. The prediction for gallium detectors is also given. It is shown that the sensitivity of Borexino is sufficient to observe
Z. G. Berezhiani +3 more
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Grand unified neutrino spectrum at Earth: Sources and spectral components
Reviews of Modern Physics, 2020Edoardo Vitagliano +2 more
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