Astrophysical S -factor for $^{6}$Li(p, γ)$^{7}$Be in the coupled-channel Gamow shell model

G.X. Dong 1 K. Fossez 2 N. Michel 1 M. Ploszajczak 1
1 GANIL - Grand Accélérateur National d'Ions Lourds
2 NSCL/FRIB, Michigan State University
Abstract : We have applied the Gamow shell model (GSM) in the coupled-channel representation to study the astrophysical S-factor for the proton radiative capture reaction of 6Li. Reaction channels are built by coupling the proton wave function expanded in different partial waves with the GSM wave functions of the ground state (1+) and the excited states (31+, 01+ and 21+) of 6Li. All relevant E1, M1, and E2 transitions from the initial continuum states in 7Be to the final bound states (3/21− and 1/21−) are included. It is found that the calculated total astrophysical S factor for this reaction agrees well with the experimental data.
Type de document :
Communication dans un congrès
The 13th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG2015) , Jun 2015, Beijing, China. EPJ Web of Conferences, 109, pp.05003, 2016, 〈10.1051/epjconf/201610905003〉
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Contributeur : Michel Lion <>
Soumis le : mercredi 9 mars 2016 - 14:15:00
Dernière modification le : jeudi 1 février 2018 - 01:34:59

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G.X. Dong, K. Fossez, N. Michel, M. Ploszajczak. Astrophysical S -factor for $^{6}$Li(p, γ)$^{7}$Be in the coupled-channel Gamow shell model. The 13th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG2015) , Jun 2015, Beijing, China. EPJ Web of Conferences, 109, pp.05003, 2016, 〈10.1051/epjconf/201610905003〉. 〈in2p3-01285541〉

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