dc.creator | Azhari, A. | |
dc.creator | Burjan, V. | |
dc.creator | Carstoiu, F. | |
dc.creator | Gagliardi, Carl A. | |
dc.creator | Kroha, V. | |
dc.creator | Mukhamedzhanov, AM | |
dc.creator | Tang, X. | |
dc.creator | Trache, L. | |
dc.creator | Tribble, Robert E. | |
dc.date.accessioned | 2011-09-13T21:27:52Z | |
dc.date.available | 2011-09-13T21:27:52Z | |
dc.date.issued | 1999 | |
dc.identifier.citation | A. Azhari, V. Burjan, F. Carstoiu, Carl A. Gagliardi, V. Kroha, A. M. Mukhamedzhanov, X. Tang, L. Trache and Robert E. Tribble. Phys.Rev.C 60 055803 1999. "Copyright (1999) by the American Physical Society." | en |
dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevC.60.055803 | |
dc.identifier.uri | https://hdl.handle.net/1969.1/126892 | |
dc.description | Journals published by the American Physical Society can be found at http://publish.aps.org/ | en |
dc.description.abstract | The N-14(Be-7,B-8)C-13 reaction was studied using an 85 MeV Be-7 radioactive beam. The asymptotic normalization coefficients for the virtual transitions Be-7+pB-8 were determined from the measured cross section. These coefficients specify the amplitude of the tail of the B-8 overlap function in the Be-7+ p channel, and were used to calculate the astrophysical S factor for the direct capture reaction Be-7(p,gamma)B-8 at solar energies S-17(0). We find that S-17(0) = 16.6 +/- 1.9 eV b. [S0556-2813(99)01111-5]. | en |
dc.language.iso | en | |
dc.publisher | American Physical Society | |
dc.subject | ASYMPTOTIC NORMALIZATION COEFFICIENTS | en |
dc.subject | CROSS-SECTION | en |
dc.subject | LOW ENERGIES | en |
dc.subject | BE-7(D,N)B-8 REACTION | en |
dc.subject | COULOMB DISSOCIATION | en |
dc.subject | ANGULAR-DISTRIBUTION | en |
dc.subject | S-17(0) FACTOR | en |
dc.subject | NUCLEI | en |
dc.subject | MODEL | en |
dc.subject | B-8 | en |
dc.subject | Physics | en |
dc.title | The N-14(Be-7,B-8)C-13 reaction and the Be-7(p,gamma)B-8 S factor | en |
dc.type | Article | en |
local.department | Physics and Astronomy | en |