2002
DOI: 10.1007/bf03548910
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Solar neutrino physics: Historical evolution, present status and perspectives

Abstract: Solar neutrino physics is an exciting and difficult field of research for physicists, where astrophysics, elementary particle and nuclear physics meet. The Sun produces the energy that life has been using on Earth for many years, about 10 9 y, emits a lot of particles: protons, electrons, ions, electromagnetic quanta... among them neutrinos play an important role allowing to us to check our knowledge on solar characteristics. The main aim of this paper is to offer a practical overview of various aspects concer… Show more

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Cited by 9 publications
(6 citation statements)
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References 428 publications
(287 reference statements)
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“…In this sense we have tried to be as complete as possible, so as to present a self-consistent overview of the current status of the three-neutrino mass-mixing parameters. While we aimed at obtaining technically accurate and complete results, we have not aimed at being bibliographically complete; we refer the reader to [18,22,38,50,53,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79] for an incomplete list of excellent reviews with rich bibliographies of old and recent neutrino papers.…”
Section: Introductionmentioning
confidence: 99%
“…In this sense we have tried to be as complete as possible, so as to present a self-consistent overview of the current status of the three-neutrino mass-mixing parameters. While we aimed at obtaining technically accurate and complete results, we have not aimed at being bibliographically complete; we refer the reader to [18,22,38,50,53,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79] for an incomplete list of excellent reviews with rich bibliographies of old and recent neutrino papers.…”
Section: Introductionmentioning
confidence: 99%
“…Both the soviet-american experiment SAGE, using more than 50 metric tons of metallic gallium [7] , and the Gallex experiment at the Gran Sasso underground laboratory, employing 30 metric tons of natural gallium [8,9] , measured a neutrino signal smaller ( ≈ 60%) than predicted by the SSM. For an historical introduction see for instance [10] .…”
Section: From the Rise Of The Solar Neutrino Problem To Its Solutionmentioning
confidence: 99%
“…here µ, ν = 1, 2, 3, 4, a, b = e, µ, τ ; the first term is the kinetic term, the second and third terms correspond to LI violation, the term with (a L ) corresponds to CPT violation. When taking gravity into account 15 this extension of the Standard Model was investigated in Ref. [128].…”
Section: B Extension Of the Standard Model: Spontaneous Violation Of ...mentioning
confidence: 99%
“…[141,106]. The authors gave a clear scheme for estimating the sensitivity of various neutrino experiments relative to the value of three parametersa L and c L included into the lagrangian (5), and the difference between 15 For a discussion of the problem of calculation of the NO phase in curved space-time see, e.g., work [129], part II, and also Refs. [130,131] and papers cited therein.…”
Section: B Extension Of the Standard Model: Spontaneous Violation Of ...mentioning
confidence: 99%