Coulomb dissociation of [sup 8]B and the [sup 7]Be([ital p],[gamma])[sup 8]B reaction at low energies
Coulomb dissociation of [sup 8]B and the [sup 7]Be([ital p],[gamma])[sup 8]B reaction at low energies
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低能量下 [sup 8]B 的库仑解离和 [sup 7]Be([ital p],γ)[sup 8]B 反应
DOI:
10.1103/physrevlett.73.2680
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发表时间:
1994
影响因子:
8.6
通讯作者:
K. Furutaka
中科院分区:
文献类型:
--
作者:
T. Motobayashi;N. Iwasa;Y. Ando;M. Kurokawa;H. Murakami;Gen. Ruan;S. Shimoura;S. Shirato;N. Inabe;M. Ishihara;T. Kubo;Y. Watanabe;M. Gai;K. Hahn;Z. Zhao;T. Nakamura;T. Teranishi;Y. Futami;K. Furutaka
The cross section for Coulomb dissociation of [sup 8]B---the [sup 208]Pb([sup 8]B,[sup 7]Be [ital p])[sup 208]Pb reaction---was measured using a [sup 8]B radioactive beam of 46.5 MeV/nucleon energy, and the cross section for the [sup 7]Be([ital p],[gamma])[sup 8]B capture reaction was deduced at low energies; [ital E][sub c.m.]=0.6[minus]1.7 MeV. The extracted astrophysical [ital S][sub 17] factors were found to be consistent with the values measured by Vaughn [ital et] [ital al]. and Filippone [ital et] [ital al]. This result encourages further experimental studies extended to lower relative energies for a new determination of the [ital S][sub 17] value relevant to the [sup 8]B solar neutrino flux.