dc.creator | Mukhamedzhanov, AM | |
dc.creator | Clark, HL | |
dc.creator | Gagliardi, Carl A. | |
dc.creator | Lui, YW | |
dc.creator | Trache, L. | |
dc.creator | Tribble, Robert E. | |
dc.creator | Xu, HM | |
dc.creator | Zhou, XG | |
dc.creator | Burjan, V. | |
dc.creator | Cejpek, J. | |
dc.creator | Kroha, V. | |
dc.creator | Carstoiu, F. | |
dc.date.accessioned | 2011-09-13T21:26:07Z | |
dc.date.available | 2011-09-13T21:26:07Z | |
dc.date.issued | 1997 | |
dc.identifier.citation | A. M. Mukhamedzhanov, H. L. Clark, Carl A. Gagliardi, Y. W. Lui, L. Trache, Robert E. Tribble, H. M. Xu, X. G. Zhou, V. Burjan, J. Cejpek, V. Kroha and F. Carstoiu. Phys.Rev.C 56 1302-1312 1997. "Copyright (1997) by the American Physical Society." | en |
dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevC.56.1302 | |
dc.identifier.uri | https://hdl.handle.net/1969.1/126869 | |
dc.description | Journals published by the American Physical Society can be found at http://publish.aps.org/ | en |
dc.description.abstract | The differential cross sections for the reactions Be-9(B-10, B-10)Be-9 and Be-9(B-10,Be-9)B-10 have been measured at an incident energy of 100 MeV. The elastic scattering data have been used to determine the optical model parameters for the Be-9+B-10 system at this energy. These parameters are then used in distorted-wave Born approximation (DWBA) calculations to predict the cross sections of the Be-9(B-10,Be-9)B-10 proton exchange reaction, populating the ground and low-lying states in B-10. By normalizing the theoretical DWBA proton exchange cross sections to the experimental ones, the asymptotic normalization coefficients (ANC's), defining the normalization of the tail of the B-10 bound state wave functions in the two-particle channel Be-9+p, have been found. The ANC for the virtual decay B-10(g.s.)-->Be-9+p will be used in an analysis of the B-10(Be-7,B-8)Be-9 reaction to extract the ANC's for B-8-->Be-7+p. These ANC's determine the normalization of the Be-7(p,gamma)B-8 radiative capture cross section at very low energies, which is crucially important for nuclear astrophysics. | en |
dc.language.iso | en | |
dc.publisher | American Physical Society | |
dc.subject | ASTROPHYSICAL S-FACTOR | en |
dc.subject | LOW ENERGIES | en |
dc.subject | RADIATIVE-CAPTURE | en |
dc.subject | VERTEX | en |
dc.subject | CONSTANT | en |
dc.subject | LIGHT-NUCLEI | en |
dc.subject | SCATTERING | en |
dc.subject | BE-7(P | en |
dc.subject | Physics | en |
dc.title | Asymptotic normalization coefficients for B-10->Be-9+p | en |
dc.type | Article | en |
local.department | Physics and Astronomy | en |