Determination of the astrophysical S factor of the B-8(p, gamma)C-9 capture reaction from the d(B-8, C-9)n reaction

Authors
Beaumel, D Kubo, T Teranishi, T Sakurai, H Fortier, S Mengoni, A Aoi, N Fukuda, N Hirai, M Imai, N Iwasaki, H Kumagai, H Laurent, H Lukyanov, SM Maison, JM Motobayashi, T Nakamura, T Ohnuma, H Pita, S Yoneda, K Ishihara, M
Citation
D. Beaumel et al., Determination of the astrophysical S factor of the B-8(p, gamma)C-9 capture reaction from the d(B-8, C-9)n reaction, PHYS LETT B, 514(3-4), 2001, pp. 226-232
Citations number
24
Categorie Soggetti
Physics
Journal title
PHYSICS LETTERS B
ISSN journal
03702693 → ACNP
Volume
514
Issue
3-4
Year of publication
2001
Pages
226 - 232
Database
ISI
SICI code
0370-2693(20010816)514:3-4<226:DOTASF>2.0.ZU;2-U
Abstract
The asymptotic normalization coefficients for the virtual decay C-9 --> B-8 + p have been determined by measuring the cross-section of the B-8(d, n)C- 9 reaction in inverse kinematics at 14.4 MeV/u, using the RIPS facility. Th e deduced astrophysical S factor S-18 of the B-8(p, gamma)C-9 capture react ion in the center of mass energy range 1-100 keV is S-18 = 45 +/- 13 eVb. ( C) 2001 Elsevier Science B.V. All rights reserved.