dc.creator | Sattarov, A. | |
dc.creator | Mukhamedzhanov, AM | |
dc.creator | Azhari, A. | |
dc.creator | Gagliardi, Carl A. | |
dc.creator | Trache, L. | |
dc.creator | Tribble, Robert E. | |
dc.date.accessioned | 2011-09-13T21:27:39Z | |
dc.date.available | 2011-09-13T21:27:39Z | |
dc.date.issued | 1999 | |
dc.identifier.citation | A. Sattarov, A. M. Mukhamedzhanov, A. Azhari, Carl A. Gagliardi, L. Trache and Robert E. Tribble. Phys.Rev.C 60 035801 1999. "Copyright (1999) by the American Physical Society." | en |
dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevC.60.035801 | |
dc.identifier.uri | https://hdl.handle.net/1969.1/126891 | |
dc.description | Journals published by the American Physical Society can be found at http://publish.aps.org/ | en |
dc.description.abstract | The Be-9(p, gamma) B-10 reaction plays an important role in primordial and stellar nucleosynthesis of light elements in the p shell, but the energy dependence of S(E) has not been well understood. We reanalyze the existing Be-9(p, gamma) B-10 experimental data within the framework of the R-matrix method. The direct capture part of the S factor is calculated using the experimentally measured asymptotic normalization coefficients for B-10 --> Be-9 + p. The fitted parameters of the low-lying B-10 resonances are also required to be consistent with previous measurements of Li-6(alpha, gamma) log. A good simultaneous fit to both radiative capture reactions is found, in contrast to previous analyses. These results demonstrate that experimentally measured asymptotic normalization coefficients, coupled to the R-matrix method, can provide a reasonable determination of direct radiative capture rates, even when the captured proton is tightly bound in the final nucleus. [S0556-2813(99)03608-0]. | en |
dc.language.iso | en | |
dc.publisher | American Physical Society | |
dc.subject | THERMONUCLEAR REACTION-RATES | en |
dc.subject | CROSS-SECTION | en |
dc.subject | LIGHT-NUCLEI | en |
dc.subject | LOW ENERGIES | en |
dc.subject | NORMALIZATION | en |
dc.subject | Physics | en |
dc.title | Astrophysical S factor for Be-9(p,gamma)B-10 | en |
dc.type | Article | en |
local.department | Physics and Astronomy | en |