Abstract
Since the discovery of molecular resonances in \(^{12}\hbox {C}+^{12}\hbox {C}\) in the early sixties a great deal of research work has been undertaken to study \(\alpha \)-clustering and resonant effects of the fusion process at sub-Coulomb barrier energies. The modified astrophysical \(S^{*}\) factors of \(^{12}\hbox {C}+^{12}\hbox {C}\) fusion have been extracted from direct fusion measurements at deep sub-barrier energies near the Gamow window. They were also obtained by the indirect Trojan horse method (THM). A comparison of direct measurements and the THM, which elucidates problems in the analysis of the THM, is discussed in this Letter to the Editor.
Data Availability Statement
This manuscript has no associated data or the data will not be deposited. [Authors’ comment: All data generated during this study are contained in the published article.]
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Acknowledgements
A.M.M. acknowledges a support from the U.S. DOE Grant No. DE-FG02-93ER40773 and the NNSA Grant No. DENA000384. X.T. is supported in part by the National Key Research and Development program (MOST 2016YFA0400501) from the Ministry of Science and Technology of China and from the key research program (XDPB09-2). A.M.M. thanks Dr. Goldberg for very useful comments.
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Communicated by N. Alamanos.
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Beck, C., Mukhamedzhanov, A.M. & Tang, X. Status on \(^{\mathbf {12}}\mathbf {C}+{}^{\mathbf {12}}{\mathbf {C}}\) fusion at deep subbarrier energies: impact of resonances on astrophysical \(S^{*}\) factors. Eur. Phys. J. A 56, 87 (2020). https://doi.org/10.1140/epja/s10050-020-00075-2
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DOI: https://doi.org/10.1140/epja/s10050-020-00075-2