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Prog. Theor. Phys. Vol. 98 No. 6 (1997) pp. 1251-1259
Reexamination of Standard Solar Model to the Solar Neutrino Problems
Kimiyo Fukasaku and
Takehisa Fujita
Department of Physics, Faculty of Science and Technology
Nihon University, Tokyo 101
(Received July 7, 1997)
Abstract:
We examine the calculation of the solar neutrino flux based on the
standard solar model (SSM). It is found that the solar neutrino data
(KAMIOKANDE experiment)
can be described well by the SSM with careful employment of
nuclear data of 7 Be (p,γ) 8 B. The main point is
that the simple-minded product ansatz of Coulomb plus nuclear parts
should have a few percent uncertainties which induce a large
reduction of the neutrino flux from 8 B. Also, if the electron
capture of 7 Be inside the sun is suppressed, then the GALLEX
experiment can be understood from the SSM calculation.
URL :
http://ptp.ipap.jp/link?PTP/98/1251/
DOI : 10.1143/PTP.98.1251
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