Fusion hindrance for the positive Q-value system 12C+30Si

The fusion excitation function for the positive-Q-value system 12C+30Si (Qfus = +14.1 MeV) has been measured in inverse kinematics down to the μb level and compared with standard coupled-channel calculations. The appearance of the fusion hindrance phenomenon and the evidence of a S-factor maximum ha...

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Main Authors: Galtarossa F., Stefanini A. M., Montagnoli G., Jiang C. L., Colucci G., Bottoni S., Broggini C., Caciolli A., Colović P., Corradi L., Courtin S., Depalo R., Fioretto E., Fruet G., Gal A., Goasduff A., Heine M., Hu S. P., Kaur M., Mijatović T., Montanari D., Scarlassara F., Strano E., Szilner S., Zhang G. X.
Format: Article
Language:English
Published: EDP Sciences 2017-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201716300019
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spelling doaj-bb0e239831ba44d5b8c7454d461d31c42021-08-02T09:43:39ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011630001910.1051/epjconf/201716300019epjconf_fusion2017_00019Fusion hindrance for the positive Q-value system 12C+30SiGaltarossa F.Stefanini A. M.Montagnoli G.Jiang C. L.Colucci G.Bottoni S.Broggini C.Caciolli A.Colović P.Corradi L.Courtin S.Depalo R.Fioretto E.Fruet G.Gal A.Goasduff A.Heine M.Hu S. P.Kaur M.Mijatović T.Montanari D.Scarlassara F.Strano E.Szilner S.Zhang G. X.The fusion excitation function for the positive-Q-value system 12C+30Si (Qfus = +14.1 MeV) has been measured in inverse kinematics down to the μb level and compared with standard coupled-channel calculations. The appearance of the fusion hindrance phenomenon and the evidence of a S-factor maximum have been observed. This result can be significant to extrapolate the behavior of lighter astrophysical relevant systems at deep sub-barrier energies, where existing experimental data are still contradicting and affected by large errors.https://doi.org/10.1051/epjconf/201716300019
collection DOAJ
language English
format Article
sources DOAJ
author Galtarossa F.
Stefanini A. M.
Montagnoli G.
Jiang C. L.
Colucci G.
Bottoni S.
Broggini C.
Caciolli A.
Colović P.
Corradi L.
Courtin S.
Depalo R.
Fioretto E.
Fruet G.
Gal A.
Goasduff A.
Heine M.
Hu S. P.
Kaur M.
Mijatović T.
Montanari D.
Scarlassara F.
Strano E.
Szilner S.
Zhang G. X.
spellingShingle Galtarossa F.
Stefanini A. M.
Montagnoli G.
Jiang C. L.
Colucci G.
Bottoni S.
Broggini C.
Caciolli A.
Colović P.
Corradi L.
Courtin S.
Depalo R.
Fioretto E.
Fruet G.
Gal A.
Goasduff A.
Heine M.
Hu S. P.
Kaur M.
Mijatović T.
Montanari D.
Scarlassara F.
Strano E.
Szilner S.
Zhang G. X.
Fusion hindrance for the positive Q-value system 12C+30Si
EPJ Web of Conferences
author_facet Galtarossa F.
Stefanini A. M.
Montagnoli G.
Jiang C. L.
Colucci G.
Bottoni S.
Broggini C.
Caciolli A.
Colović P.
Corradi L.
Courtin S.
Depalo R.
Fioretto E.
Fruet G.
Gal A.
Goasduff A.
Heine M.
Hu S. P.
Kaur M.
Mijatović T.
Montanari D.
Scarlassara F.
Strano E.
Szilner S.
Zhang G. X.
author_sort Galtarossa F.
title Fusion hindrance for the positive Q-value system 12C+30Si
title_short Fusion hindrance for the positive Q-value system 12C+30Si
title_full Fusion hindrance for the positive Q-value system 12C+30Si
title_fullStr Fusion hindrance for the positive Q-value system 12C+30Si
title_full_unstemmed Fusion hindrance for the positive Q-value system 12C+30Si
title_sort fusion hindrance for the positive q-value system 12c+30si
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2017-01-01
description The fusion excitation function for the positive-Q-value system 12C+30Si (Qfus = +14.1 MeV) has been measured in inverse kinematics down to the μb level and compared with standard coupled-channel calculations. The appearance of the fusion hindrance phenomenon and the evidence of a S-factor maximum have been observed. This result can be significant to extrapolate the behavior of lighter astrophysical relevant systems at deep sub-barrier energies, where existing experimental data are still contradicting and affected by large errors.
url https://doi.org/10.1051/epjconf/201716300019
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