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Prog. Theor. Phys. Vol. 38 No. 5 (1967) pp. 1083-1094
Formation of Li, Be, B in the Expanding Hot Universe
Humitaka Satō
Department of Physics, Faculty of Science, Kyoto University, Kyoto
(Received July 10, 1967)
Abstract:
The hot universe model suggests the element formation by thermonuclear fusion at the early stage of the cosmic expansion. The primordial origin of Li, Be, B is examined. Recent investigation by Wagoner, Fowler and Hoyle gives only the abundance of Li7. In this paper, we estimate the abundances of all the stable isotopes of Li, Be and B produced. In the case of Friedmann models with the present matter density ρ0m = 10-32 ∼ 10-29 g/cm3 and the present radiation temperature T0 ≃ 3°K, the produced quantities are D < 10-2.0. He3 < 10-3.6, He4 < 10-1.0, Li6 < 10-12.7, Li7 < 10-8.6, Be9 < 10-13.3, B10 < 10-16.7 and B11 < 10-13.0, by the ratio to hydrogen in number density. Therefore, the observed abundances of Li, Be, B cannot be explained by the primordial origin.
URL :
http://ptp.ipap.jp/link?PTP/38/1083/
DOI : 10.1143/PTP.38.1083
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