EPJ Web of Conferences (Jan 2022)
Direct measurement of the 19F(p, αγ)16O reaction in JUNA
- Zhang L.Y.,
- Su J.,
- He J.J.,
- Wiescher M.,
- deBoer R.J.,
- Kahl D.,
- Chen Y.J.,
- Li X.Y.,
- Wang J.G.,
- Zhang L.,
- Cao F.Q.,
- Zhang H.,
- Zhang Z.C.,
- Jiao T.Y.,
- Sheng Y.D.,
- Wang L.H.,
- Song L.Y.,
- Jiang X.Z.,
- Li Z.M.,
- Li E.T.,
- Wang S.,
- Lian G.,
- Li Z.H.,
- Tang X.D.,
- Zhao H.W.,
- Sun L.T.,
- Wu Q.,
- Li J.Q.,
- Cui B.Q.,
- Chen L.H.,
- Ma R.G.,
- Guo B.,
- Xu S.W.,
- Li J.Y.,
- Qi N.C.,
- Sun W.L.,
- Guo X.Y.,
- Zhang P.,
- Chen Y.H.,
- Zhou Y.,
- Zhou J.F.,
- He J.R.,
- Shang C.S.,
- Li M.C.,
- Zhou X.H.,
- Zhang Y.H.,
- Zhang F.S.,
- Hu Z.G.,
- Xu H.S.,
- Cheng J.P.,
- Liu W.P.
Affiliations
- Zhang L.Y.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Su J.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- He J.J.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Wiescher M.
- The Joint Institute for Nuclear Astrophysics, Department of Physics, University of Notre Dame, Notre Dame
- deBoer R.J.
- The Joint Institute for Nuclear Astrophysics, Department of Physics, University of Notre Dame, Notre Dame
- Kahl D.
- Extreme Light Infrastructure – Nuclear Physics, Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering (IFIN-HH)
- Chen Y.J.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Li X.Y.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Wang J.G.
- Institute of Modern Physics, Chinese Academy of Sciences
- Zhang L.
- China Institute of Atomic Energy
- Cao F.Q.
- China Institute of Atomic Energy
- Zhang H.
- China Institute of Atomic Energy
- Zhang Z.C.
- College of Physics and Optoelectronic Engineering, Shenzhen University
- Jiao T.Y.
- Institute of Modern Physics, Chinese Academy of Sciences
- Sheng Y.D.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Wang L.H.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Song L.Y.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Jiang X.Z.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Li Z.M.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Li E.T.
- College of Physics and Optoelectronic Engineering, Shenzhen University
- Wang S.
- Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University
- Lian G.
- China Institute of Atomic Energy
- Li Z.H.
- China Institute of Atomic Energy
- Tang X.D.
- Institute of Modern Physics, Chinese Academy of Sciences
- Zhao H.W.
- Institute of Modern Physics, Chinese Academy of Sciences
- Sun L.T.
- Institute of Modern Physics, Chinese Academy of Sciences
- Wu Q.
- Institute of Modern Physics, Chinese Academy of Sciences
- Li J.Q.
- Institute of Modern Physics, Chinese Academy of Sciences
- Cui B.Q.
- China Institute of Atomic Energy
- Chen L.H.
- China Institute of Atomic Energy
- Ma R.G.
- China Institute of Atomic Energy
- Guo B.
- China Institute of Atomic Energy
- Xu S.W.
- Institute of Modern Physics, Chinese Academy of Sciences
- Li J.Y.
- Institute of Modern Physics, Chinese Academy of Sciences
- Qi N.C.
- Yalong River Hydropower Development Company
- Sun W.L.
- Yalong River Hydropower Development Company
- Guo X.Y.
- Yalong River Hydropower Development Company
- Zhang P.
- Yalong River Hydropower Development Company
- Chen Y.H.
- Yalong River Hydropower Development Company
- Zhou Y.
- Yalong River Hydropower Development Company
- Zhou J.F.
- Yalong River Hydropower Development Company
- He J.R.
- Yalong River Hydropower Development Company
- Shang C.S.
- Yalong River Hydropower Development Company
- Li M.C.
- Yalong River Hydropower Development Company
- Zhou X.H.
- Institute of Modern Physics, Chinese Academy of Sciences
- Zhang Y.H.
- Institute of Modern Physics, Chinese Academy of Sciences
- Zhang F.S.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Hu Z.G.
- Institute of Modern Physics, Chinese Academy of Sciences
- Xu H.S.
- Institute of Modern Physics, Chinese Academy of Sciences
- Cheng J.P.
- Key Laboratory of Beam Technology and Material Modification of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University
- Liu W.P.
- China Institute of Atomic Energy
- DOI
- https://doi.org/10.1051/epjconf/202226008004
- Journal volume & issue
-
Vol. 260
p. 08004
Abstract
The 19F(p, αγ)16O reaction is of crucial importance for Galactic 19F abundances and CNO cycle loss in first generation Population III stars. Due to its extremely small cross sections, the 19F(p, αγ)16O reaction has not been measured in the low energy part of the Gamow window(70-200 keV). As a day-one campaign, the experiment was performed under the extremely low cosmicray-induced background environment of the China JinPing Underground Laboratory(CJPL), one of the deepest underground laboratories in the world. The γ-ray yields were measured over Ec.m. =72.4–344 keV, covering the full Gamow window for the first time. The direct experimental data will help people to expound the fluorine over-abundances, energy generation, as well as heavy-element nuclosynthesis scenario in asymptotic giant branch (AGB) stars, with the astrophysical model on the firm ground.
