Low-energy photodisintegration of
Be and
Be
reactions at astrophysical conditions
V.D. Efros1 - H. Oberhummer2 - A. Pushkin3 - I.J. Thompson4
1 Russian Research Centre "Kurchatov Institute'', Kurchatov Square 1, 123182 Moscow, Russia
2 Institut für Kernphysik, Wiedner Hauptstrasse 8-10, TU Wien, A-1040, Vienna, Austria
3 Department of Mathematical Physics, Lund Institute of Technology, P.O. Box, 118 S-221 00 Lund, Sweden
4 Department of Physics, University of Surrey, Guildford GU2 5XH, United Kingdom
Received: 19 January 1998 Communicated by B. Povh
Abstract
A semi-microscopic model for the low-energy photodisintegration of the 9Be nucleus is constructed,
and the experimental data are analyzed with its help.
The older radioactive isotope data are supported by this analysis. The theoretical
photodisintegration cross section is derived. The astrophysical rates
for the reaction Be
and the reverse
photodisintegration of 9Be
are calculated. The new reaction rate for
Be
is compared with previous estimations.
PACS
25.20.Dc Photon absorption and scattering -
25.40.Lw Radioactive capture -
97.10.Cv Stellar structure, interiors, evolution, nucleosynthesis, ages -
21.60.Gx Cluster models -
21.45.+v Few-body systems
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