by M. Carmona-Gallardo, B. S. Nara Singh, O. Tengblad, M. Hass, M. Alcorta, M. J. G. Borge, J. A. Briz, C. Cruz, M. Cubero, R Domínguez-Reyes, B. R. Fulton, H. Fynbo, N. Gordillo, G. Haquin, Y. Nir-El, V. Kumar, A. Maira, J. McGrath, A Muñoz-Martín, A. Perea and Z. Yungreis
Abstract:
The astrophysical S factor for the 4 He( 3 He, γ ) 7 Be direct capture reaction plays a major role in the context of solar neutrino flux and primordial 7 Li abundances that demand accurate information on the reaction. We report here our recent cross section measurements using the activation method in the region of E CM = 900-2800 keV, that aim to shed light on the discrepancies in the existing data and lead to a more accurate extrapolation of the S factor.
Reference:
M. Carmona-Gallardo, B. S. Nara Singh, O. Tengblad, M. Hass, M. Alcorta, M. J. G. Borge, J. A. Briz, C. Cruz, M. Cubero, R Domínguez-Reyes, B. R. Fulton, H. Fynbo, N. Gordillo, G. Haquin, Y. Nir-El, V. Kumar, A. Maira, J. McGrath, A Muñoz-Martín, A. Perea and Z. Yungreis, “Astrophysical S factor for the 4 He( 3 He, γ ) 7 Be reaction at medium energies”, Journal of Physics: Conference Series, vol. 337, no. 1, pp. 012061.
Bibtex Entry:
@article{carmona-gallardo_astrophysical_2012,
title = {Astrophysical {S} factor for the 4 {He}( 3 {He}, γ ) 7 {Be} reaction at medium energies},
volume = {337},
issn = {1742-6596},
url = {http://stacks.iop.org/1742-6596/337/i=1/a=012061},
doi = {10.1088/1742-6596/337/1/012061},
abstract = {The astrophysical S factor for the 4 He( 3 He, γ ) 7 Be direct capture reaction plays a major role in the context of solar neutrino flux and primordial 7 Li abundances that demand accurate information on the reaction. We report here our recent cross section measurements using the activation method in the region of E CM = 900-2800 keV, that aim to shed light on the discrepancies in the existing data and lead to a more accurate extrapolation of the S factor.},
language = {en},
number = {1},
urldate = {2017-10-10},
journal = {Journal of Physics: Conference Series},
author = {Carmona-Gallardo, M. and Singh, B. S. Nara and Tengblad, O. and Hass, M. and Alcorta, M. and Borge, M. J. G. and Briz, J. A. and Cruz, C. and Cubero, M. and {R Domínguez-Reyes} and Fulton, B. R. and Fynbo, H. and Gordillo, N. and Haquin, G. and Nir-El, Y. and Kumar, V. and Maira, A. and McGrath, J. and {A Muñoz-Martín} and Perea, A. and Yungreis, Z.},
year = {2012},
pages = {012061},
file = {IOP Full Text PDF:E:\cmam_papers\files\1160\Carmona-Gallardo et al. - 2012 - Astrophysical S factor for the 4 He( 3 He, γ ) 7 B.pdf:application/pdf;IOP Full Text PDF:E:\Usuarios\Administrator\Zotero\storage\YLPJTQXQ\Carmona-Gallardo et al. - 2012 - Astrophysical S factor for the 4 He( 3 He, γ ) 7 B.pdf:application/pdf},
}