Astrophysical factors of 12 C+12 C fusion from Trojan horse method

Abstract

Carbon-carbon burning plays an important role in many stellar environments. Recently, using the indirect Trojan horse method A. Tumino et al. reported [Nature 557 687 (2018)] a strong rise of the astrophysical factor for the carbon-carbon fusion at low resonance energies. In this paper, we demonstrate that this rise is the artifact of using an invalid plane-wave approximation. It is shown that the calculated renormalization factor decreases the astrophysical factor from [A. Tumino et al., Nature 557 687 (2018)] at the resonance energies of E=0.8-0.9 MeV by as much as ≈ 103 times.

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