Angular distribution for Be-7(d, n)B-8 reaction at E-c.m.=8.3 MeV and the astrophysical S-17(0) factor for Be-7(p, gamma)B-8 reaction

Authors
Wang, YB Liu, WP Bai, XX Li, ZC Li, AL Zhou, SH Zhu, XF Li, XM He, GK Guo, G Lian, G Tang, XD
Citation
Yb. Wang et al., Angular distribution for Be-7(d, n)B-8 reaction at E-c.m.=8.3 MeV and the astrophysical S-17(0) factor for Be-7(p, gamma)B-8 reaction, CHIN PHYS L, 16(12), 1999, pp. 873-875
Citations number
9
Categorie Soggetti
Physics
Journal title
CHINESE PHYSICS LETTERS
ISSN journal
0256307X → ACNP
Volume
16
Issue
12
Year of publication
1999
Pages
873 - 875
Database
ISI
SICI code
0256-307X(1999)16:12<873:ADFBNR>2.0.ZU;2-Z
Abstract
The differential cross section for Be-7(d, n)B-8 reaction at E-c.m. = 8.3 M eV has been measured by using a Be-7 radioactive beam. The reaction cross s ection was determined to be 28 +/- 3 mb. The astrophysical S17(0) factor fo r the Be-7(p,gamma)(8) B reaction was derived to be 24 +/- 5 eV b through t he asymptotic normalization constant of B-8 extracted from the experimental data. This result is found to be consistent with a previous value obtained from the same reaction at E-c.m. = 5.8 MeV, implying the energy independen ce of this indirect method within the uncertainty.