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The Solar Neutrino Problem
Published online by Cambridge University Press: 25 April 2016
Extract
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 giving a predicted neutrino count rate below the Davis (1972) experimental limit.
- Type
- Invited Papers
- Information
- Publications of the Astronomical Society of Australia , Volume 2 , Issue 6 , October 1975 , pp. 318 - 322
- Copyright
- Copyright © Astronomical Society of Australia 1975
References
Bancall, J.N., Huebner, W.F., Magee, N.H., Merts, A.L., and Ulrich, R.K., Astrophys. J., 184, 1 (1973).Google Scholar
Faulkner, D.J., Da Costa, G.S., and Prentice, A.J.R., Mon. Not. R. Astr. Soc, 170, 589 (1975).Google Scholar
Hill, H.A., Clayton, P.D., Patz, D.L., Healy, A.W., Stebbins, R.T.,Oleson, J.R., and Zanoni, C.A., Rhys. Rev. Lett., 33, 1497 (1974).Google Scholar