TY - JOUR
T1 - Determination of the astrophysical S factor of the 8B(p, γ)9C capture reaction from the d(8B, 9C)n reaction
AU - Beaumel, D.
AU - Kubo, T.
AU - Teranishi, T.
AU - Sakurai, H.
AU - Fortier, S.
AU - Mengoni, A.
AU - Aoi, N.
AU - Fukuda, N.
AU - Hirai, M.
AU - Imai, N.
AU - Iwasaki, H.
AU - Kumagai, H.
AU - Laurent, H.
AU - Lukyanov, S. M.
AU - Maison, J. M.
AU - Motobayashi, T.
AU - Nakamura, T.
AU - Ohnuma, H.
AU - Pita, S.
AU - Yoneda, K.
AU - Ishihara, M.
N1 - Funding Information:
We wish to thank the RIKEN RARF and Orsay tandem accelerator staffs. We acknowledge Dr. N. Smirnova for shell-model calculations, and Dr. Y. Blumenfeld, Dr. S. Galès and Dr. J.P. Thibaud for careful reading of the manuscript. Part of this work was achieved within the IN2P3-RIKEN agreements and supported by the Science and Technology Agency of the Japanese government.
Copyright:
Copyright 2007 Elsevier B.V., All rights reserved.
PY - 2001/8/16
Y1 - 2001/8/16
N2 - The asymptotic normalization coefficients for the virtual decay 9C → 8B + p have been determined by measuring the cross-section of the 8B(d, n)9C reaction in inverse kinematics at 14.4 MeV/u, using the RIPS facility. The deduced astrophysical S factor S18 of the 8B(p, γ)9C capture reaction in the center of mass energy range 1-100 keV is S18 = 45 ± 13 eV b.
AB - The asymptotic normalization coefficients for the virtual decay 9C → 8B + p have been determined by measuring the cross-section of the 8B(d, n)9C reaction in inverse kinematics at 14.4 MeV/u, using the RIPS facility. The deduced astrophysical S factor S18 of the 8B(p, γ)9C capture reaction in the center of mass energy range 1-100 keV is S18 = 45 ± 13 eV b.
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U2 - 10.1016/S0370-2693(01)00828-0
DO - 10.1016/S0370-2693(01)00828-0
M3 - Article
AN - SCOPUS:0035899530
SN - 0370-2693
VL - 514
SP - 226
EP - 232
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
IS - 3-4
ER -