Thermonuclear 28P(p, γ)29S reaction rate and astrophysical implication in ONe nova explosion

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作者：
Liu, J.B. [1 ,2 ]
José, J. [3 ,4 ]
Hou, S.Q. [1 ,2 ,5 ]
Pignatari, M. [5 ,6 ,7 ,8 ,9 ]
Trueman, T.C.L. [5 ,6 ,7 ,8 ]
Longland, R. [10 ,11 ]
Li, J.G. [1 ,2 ]
Bertulani, C.A. [12 ]
Xu, X.X. [1 ,2 ]
机构：
[1] Key Laboratory of High Precision Nuclear Spectroscopy, Institute of Modern Physics, Chinese Academy of Sciences, 509 Nanchang Rd, Lanzhou,730000, China
[2] School of Nuclear Science and Technology, University of Chinese Academy of Sciences, 19A Yuquan Rd, Shijingshan District, Beijing,100049, China
[3] Departament de Física, Universitat Politècnica de Catalunya, Barcelona,08019, Spain
[4] Institut d'Estudis Espacials de Catalunya, Universitat Politècnica de Catalunya, Barcelona,08034, Spain
[5] NuGrid Collaboration, Canada
[6] Konkoly Observatory, HUN-REN, Konkoly Thege M. út 15a-17, Budapest,H-1121, Hungary
[7] CSFK, MTA Centre of Excellence, Konkoly Thege Miklós út 15-17, Budapest,1121, Hungary
[8] E. A. Milne Centre for Astrophysics, University of Hull, Cottingham Rd, Kingston upon Hull,HU6 7RX, United Kingdom
[9] Joint Institute for Nuclear Astrophysics, Center for the Evolution of the Elements, 640 S Shaw Lane, East Lansing,MI,48824, United States
[10] Department of Physics, North Carolina State University, Raleigh,NC,27695, United States
[11] Triangle Universities Nuclear Laboratory, Durham,NC,27708, United States
[12] Department of Physics and Astronomy, Texas A&M University-Commerce, Commerce,TX,75429, United States
来源：
Astronomy and Astrophysics | 2024年 / 687卷
基金：
国家重点研发计划;
关键词：
This work was financially supported by the National Key R & D Program of China Grant No. 2022YFA1603300; Longyuan Youth Talent Program of Gansu Province; the Strategic Priority Research Program of Chinese Academy of Sciences Grant No. XDB34020204; and in part by the National Science Foundation under Grant No. OISE-1927130 (IReNA). J.J. acknowledges support from the MINECO grant PID2020-117252GB-I00; by the EU Feder funds; and by the AGAUR/Generalitat de Catalunya grant SGR386/2021. C.A.B. acknowledges support by the U.S. DOE grant DE-FG02- 08ER41533 and the Helmholtz Research Academy Hesse for FAIR. M.P. and TT acknowledge the ongoing access to viper; the University of Hull High Performance Computing Facility. J.J; M.P. and T.T. acknowledge the support of the European Union's Horizon 2020 research and innovation programme (ChETEC-INFRA - Project no. 101008324). M.P. acknowledges the support from the "Lendulet-2023\"" LP2023-10 Programme of the Hungarian Academy of Sciences (Hungary);
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