High-precision (p,t) reaction to determine Al25(p,γ)Si26 reaction rates

A. Matic, A. M. van den Berg, M. N. Harakeh, H. J. Wörtche, G. P. A. Berg, M. Couder, J. Görres, P. LeBlanc, S. O’Brien, M. Wiescher, K. Fujita, K. Hatanaka, Y. Sakemi, Y. Shimizu, Y. Tameshige, A. Tamii, M. Yosoi, T. Adachi, Y. Fujita, Y. Shimbara, H. Fujita, T. Wakasa, B. A. Brown, and H. Schatz
Phys. Rev. C 82, 025807 – Published 18 August 2010

Abstract

Since the identification of ongoing Al26 production in the universe, the reaction sequence Mg24(p,γ)Al25(β+ν)Mg25(p,γ)Al26 has been studied intensively. At temperatures where the radiative capture on Al25 (t1/2=7.2 s) becomes faster than the β+ decay, the production of Al26 can be reduced due to the depletion of Al25. To determine the resonances relevant for the Al25(p,γ)Si26 bypass reaction, we measured the Si28(p,t)Si26 reaction with high-energy precision using the Grand Raiden spectrometer at the Research Center for Nuclear Physics, Osaka. Several new energy levels were found above the p threshold and for known states excitation energies were determined with smaller uncertainties. The calculated stellar rates of the bypass reaction agree well with previous results, suggesting that these rates are well established.

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  • Received 15 June 2010

DOI:https://doi.org/10.1103/PhysRevC.82.025807

©2010 American Physical Society

Authors & Affiliations

A. Matic*, A. M. van den Berg, M. N. Harakeh, and H. J. Wörtche

  • Kernfysisch Versneller Instituut, University of Groningen, Zernikelaan 25, NL-9747 AA Groningen, The Netherlands

G. P. A. Berg, M. Couder, J. Görres, P. LeBlanc, S. O’Brien, and M. Wiescher

  • Department of Physics and the Joint Institute for Nuclear Astrophysics, University of Notre Dame, Notre Dame, Indiana 46556, USA

K. Fujita, K. Hatanaka, Y. Sakemi, Y. Shimizu, Y. Tameshige§, A. Tamii, and M. Yosoi

  • Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka 560-0047, Japan

T. Adachi, Y. Fujita, and Y. Shimbara

  • Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan

H. Fujita

  • School of Physics, University of the Witwatersrand, P.O. Wits, Johannesburg 2050, South Africa

T. Wakasa

  • Department of Physics, Kyushu University, Fukuoka 812-8581, Japan

B. A. Brown and H. Schatz

  • Department of Physics and Astronomy, National Superconducting Cyclotron Laboratory and the Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA

  • *Present address: Forschungszentrum Dresden-Rossendorf, Postfach 510119, 01314 Dresden, D-01328 Dresden, Germany.
  • Present address: GSI Helmholtzzentrum für Schwerionenforschung GmbH, Planckstraße 1, D-64291 Darmstadt, Germany.
  • Present address: Center for Nuclear Study, University of Tokyo, Wako, Saitama 351-0198, Japan.
  • §Present address: Office for Development of Proton Therapy Center, Regional Health Services Division, Department of Health and Welfare Fukui Prefectural Government, Fukui City, Fukui Prefecture 910-0846, Japan.

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Vol. 82, Iss. 2 — August 2010

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