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

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 $^6$Li. 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 ($3^+_1$, $0^+_1$ and $2^+_1$) of $^6$Li. All relevant $E1$, $M1$, and $E2$ transitions from the initial continuum states in $^7$Be to the final bound states (${3/2}^-_1$ and ${1/2}^-_1$) states are included. It is found that the calculated total astrophysical $S$ factor for this reaction agrees well with the experimental data.
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Contributor : Michel Lion <>
Submitted on : Tuesday, October 6, 2015 - 8:38:10 AM
Last modification on : Thursday, June 11, 2020 - 10:02:05 PM

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G.X. Dong, K. Fossez, N. Michel, M. Ploszajczak. Astrophysical S-factor for $^6$Li$(p,\gamma)$$^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. pp.05003, ⟨10.1051/epjconf/201610905003⟩. ⟨in2p3-01212039⟩



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