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

D. Beaumel, T. Kubo, T. Teranishi, H. Sakurai, S. Fortier, A. Mengoni, N. Aoi, N. Fukuda, M. Hirai, N. Imai, H. Iwasaki, H. Kumagai, H. Laurent, S. M. Lukyanov, J. M. Maison, T. Motobayashi, T. Nakamura, H. Ohnuma, S. Pita, K. YonedaM. Ishihara

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Abstract

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.

Original languageEnglish
Pages (from-to)226-232
Number of pages7
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume514
Issue number3-4
DOIs
Publication statusPublished - Aug 16 2001

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All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics

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