Examination of the role of the O14(α,p)F17 reaction rate in type-I x-ray bursts

J. Hu, J. J. He, A. Parikh, S. W. Xu, H. Yamaguchi, D. Kahl, P. Ma, J. Su, H. W. Wang, T. Nakao, Y. Wakabayashi, T. Teranishi, K. I. Hahn, J. Y. Moon, H. S. Jung, T. Hashimoto, A. A. Chen, D. Irvine, C. S. Lee, and S. Kubono
Phys. Rev. C 90, 025803 – Published 12 August 2014

Abstract

The O14(α,p)F17 reaction is one of the key reactions involved in the breakout from the hot-CNO cycle to the rp-process in type-I x-ray bursts (XRBs). The resonant properties in the compound nucleus Ne18 have been investigated through resonant elastic scattering of F17+p. The radioactive F17 beam was separated by the Center for Nuclear Study radioactive ion beam separator (CRIB) and bombarded a thick H2 gas target at 3.6 MeV/nucleon. The recoiling light particles were measured by three ΔEE silicon telescopes at laboratory angles of θlab3,10, and 18. Five resonances at Ex=6.15, 6.28, 6.35, 6.85, and 7.05 MeV were observed in the excitation functions, and their spin-parities have been determined based on an R-matrix analysis. In particular, Jπ=1 was firmly assigned to the 6.15-MeV state which dominates the thermonuclear O14(α,p)F17 rate below 2 GK. As well, a possible new excited state in Ne18 was observed at Ex=6.85±0.11 MeV with tentative J=0 assignment. This state could be the analog state of the 6.880 MeV (0) level in the mirror nucleus O18, or a bandhead state (0+) of the six-particle four-hole (6p-4h) band. A new thermonuclear O14(α,p)F17 rate has been determined, and the astrophysical impact of multiple recent rates has been examined using an XRB model. Contrary to previous expectations, we find only a modest impact on predicted nuclear energy generation rates from using reaction rates differing by up to several orders of magnitude.

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  • Received 3 June 2014
  • Revised 6 July 2014

DOI:https://doi.org/10.1103/PhysRevC.90.025803

©2014 American Physical Society

Authors & Affiliations

J. Hu1,2, J. J. He1,*, A. Parikh3,4,†, S. W. Xu1,5, H. Yamaguchi2, D. Kahl2, P. Ma1, J. Su6, H. W. Wang7, T. Nakao2, Y. Wakabayashi8, T. Teranishi9, K. I. Hahn10, J. Y. Moon11, H. S. Jung11,‡, T. Hashimoto12, A. A. Chen13, D. Irvine13, C. S. Lee11, and S. Kubono1,8

  • 1Key Laboratory of High Precision Nuclear Spectroscopy and Center for Nuclear Matter Science, Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China
  • 2Center for Nuclear Study (CNS), University of Tokyo, Wako Branch at RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
  • 3Departament de Física i Enginyeria Nuclear, EUETIB, Universitat Politècnica de Catalunya, Barcelona E-08036, Spain
  • 4Institut d'Estudis Espacials de Catalunya, Barcelona E-08034, Spain
  • 5University of Chinese Academy of Sciences, Beijing 100049, China
  • 6China Institute of Atomic Energy (CIAE), P.O. Box 275(46), Beijing 102413, China
  • 7Shanghai Institute of Applied Physics (SINAP), Chinese Academy of Sciences (CAS), Shanghai 201800, China
  • 8RIKEN Nishina Center, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
  • 9Department of Physics, Kyushu University, 6-10-1 Hakozaki, Fukuoka 812-8581, Japan
  • 10Department of Science Education, Ewha Womans University, Seoul 120-750, Republic of Korea
  • 11Department of Physics, Chung-Ang University, Seoul 156-756, Republic of Korea
  • 12Research Center for Nuclear Physics (RCNP), Osaka University, 10-1 Mihogaoka, Ibaraki, Osaka, 567-0047, Japan
  • 13Department of Physics & Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, Canada

  • *jianjunhe@impcas.ac.cn
  • anuj.r.parikh@upc.edu
  • Present address: Department of Physics, University of Notre Dame, Indiana 46556, USA.

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Vol. 90, Iss. 2 — August 2014

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