arXiv · 1510.07717
${^3{\rm He}}(α,γ){^7{\rm Be}}$ and ${^3{\rm H}}(α,γ){^7{\rm Li}}$ astrophysical $S$ factors from the no-core shell model with continuum
Abstract
The ${^3{\rm He}}(α,γ){^7{\rm Be}}$ and ${^3{\rm H}}(α,γ){^7{\rm Li}}$ astrophysical $S$ factors are calculated within the no-core shell model with continuum using a renormalized chiral nucleon-nucleon interaction. The ${^3{\rm He}}(α,γ){^7{\rm Be}}$ astrophysical $S$ factors agree reasonably well with the experimental data while the ${^3{\rm H}}(α,γ){^7{\rm Li}}$ ones are overestimated. The seven-nucleon bound and resonance states and the $α+{^3{\rm He}}/{^3{\rm H}}$ elastic scattering are also studied and compared with experiment. The low-lying resonance properties are rather well reproduced by our approach. At low energies, the $s$-wave phase shift, which is non-resonant, is overestimated.
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Jérémy Dohet-Eraly, Petr Navrátil, Sofia Quaglioni, Wataru Horiuchi, Guillaume Hupin, Francesco Raimondi. 2016-02-14. ${^3{\rm He}}(α,γ){^7{\rm Be}}$ and ${^3{\rm H}}(α,γ){^7{\rm Li}}$ astrophysical $S$ factors from the no-core shell model with continuum. https://doi.org/10.1016/j.physletb.2016.04.021
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