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Solving the Solar Neutrino Problem
Scientific American Sp, 2003Building a detector the size of a 10-story building two kilometers underground is a strange way to study solar phenomena. Yet that has turned out to be the key to unlocking a decades-old puzzle about the physical processes occurring inside the sun. English physicist Arthur Eddington suggested as early as 1920 that nuclear fusion powered the sun, but ...
Arthur B, McDonald +2 more
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Pseudo Dirac neutrinos and the solar-neutrino problem
Physical Review D, 1992Observational consequences of the pseudo-Dirac-neutrino hypothesis of Kobayashi, Lim, and Nojiri are examined in the context of the solar-neutrino problem. Detailed calculations are performed to obtain expected rates at the $^{37}\mathrm{Cl}$, Kamiokande II, and $^{71}\mathrm{Ga}$ detectors.
, Minakata, , Nunokawa
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AIP Conference Proceedings, 1979
A summary of the results of the Brookhaven solar neutrino experiment is given and discussed in relation to solar‐model calculations. A review is given of the merits of various new solar neutrino detectors that have been proposed.
R. Davis Jr. +2 more
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A summary of the results of the Brookhaven solar neutrino experiment is given and discussed in relation to solar‐model calculations. A review is given of the merits of various new solar neutrino detectors that have been proposed.
R. Davis Jr. +2 more
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Il Nuovo Cimento A, 1991
The problem of solar neutrinos is discussed in the case of large magnetic field in the innermost region of the core (
V. de Sabbata, C. Sivaram
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The problem of solar neutrinos is discussed in the case of large magnetic field in the innermost region of the core (
V. de Sabbata, C. Sivaram
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Publications of the Astronomical Society of Australia, 1973
A major crisis facing theoretical nuclear astronomers and physicists today is the apparently very low flux of neutrinos emitted by the Sun. Davis et al. report a measurement of 1.5 ± 1 s.n.u. (1 s.n.u. = 10−36 capture/Cl37/sec) which is a factor of 6 or so smaller than the theoretically predicted values.
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A major crisis facing theoretical nuclear astronomers and physicists today is the apparently very low flux of neutrinos emitted by the Sun. Davis et al. report a measurement of 1.5 ± 1 s.n.u. (1 s.n.u. = 10−36 capture/Cl37/sec) which is a factor of 6 or so smaller than the theoretically predicted values.
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2022
This thesis was scanned from the print manuscript for digital preservation and is copyright the author. Researchers can access this thesis by asking their local university, institution or public library to make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
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This thesis was scanned from the print manuscript for digital preservation and is copyright the author. Researchers can access this thesis by asking their local university, institution or public library to make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
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Publications of the Astronomical Society of Australia, 1975
A few years ago Fowler (1972) published a paper in which he proposed two ‘desperate explanations’ for the solar neutrino problem. Desperation continues to be characteristic of the subject, for, in spite of many investigations over recent years, there is still no unambiguously successful model satisfying all the observational features of the Sun and ...
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A few years ago Fowler (1972) published a paper in which he proposed two ‘desperate explanations’ for the solar neutrino problem. Desperation continues to be characteristic of the subject, for, in spite of many investigations over recent years, there is still no unambiguously successful model satisfying all the observational features of the Sun and ...
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Neutrino oscillations and the solar neutrino problem
European Journal of Physics, 1989Part of the interest in neutrino astrophysics has to do with the fascinating interplay between nuclear and particle physics issues — e.g. whether neutrinos are massive and undergo flavor oscillations, whether they have detectable electromagnetic moments, etc. — and astrophysical phenomena, such as the clustering of matter on large scales, the processes
M E Berbenni Bitsch, A Vancura
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Pramana, 2000
I review the solar neutrino problem and what it has taught us about the Sun and fundamental physics.
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I review the solar neutrino problem and what it has taught us about the Sun and fundamental physics.
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THE SOLAR NEUTRINO PROBLEM AND BOUNDS ON SOLAR NEUTRINO FLUXES
Modern Physics Letters A, 1995We review the current status of the solar neutrino problem. A survey of the experiments and their results are given, and solar physics crucial to the understanding of these results are discussed. Semi-empirical methods are used to derive bounds on the fluxes of the three most important components (pp, 7Be and 8B) of the solar neutrino spectrum. The 8B
WAIKWOK KWONG, S.P. ROSEN
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