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Solar Neutrino Problem

Published online by Cambridge University Press:  25 April 2016

A. J. R. Prentice
A. J. R. Prentice*
Affiliation:
Mathematics Department, Monash University, Clayton
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Extract

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. Numerous suggestions, often quite bizarre, have been made to account for the low flux, but so far no convincing explanation has been offered – see Fowler.

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Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 4 , October 1973 , pp. 226 - 227
Copyright
Copyright © Astronomical Society of Australia 1973

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References

1 Davis, R. Jr., Rogers, L.C. and Radeka, V., Bull. Amer. Phys. Soc, 16, 631 (1971).Google Scholar
2 Fowler, W.A., Nature, 238, 24 (1972).Google Scholar
3 Larson, R.B., Mon. Nat. Astr. Soc. 145, 271 (1969).CrossRefGoogle Scholar
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5 Prentice, A.J.R., Mon. Nat. Ast. Soc. in press (1973).Google Scholar
6 Prentice, A.J.R., Astron. Astrophys., Submitted (1973).Google Scholar