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Revised decay properties of the key 93-keV resonance in the Mg25(p,γ) reaction and its influence on the MgAl cycle in astrophysical environments

G. Lotay1, D. T. Doherty1, R. V. F. Janssens2,3, D. Seweryniak4, H. M. Albers4,*, S. Almaraz-Calderon4,†, M. P. Carpenter4, A. E. Champagne2,3, C. J. Chiara4,5,‡ et al.

C. R. Hoffman4, C. Iliadis2,3, A. Kankainen6, T. Lauritsen4, and S. Zhu4,§

  • 1Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
  • 2Department of Physics, University of North Carolina at Chapel Hill, Chapel Hill, North Carolina 27599, USA
  • 3Triangle Universities Nuclear Laboratory, Duke University, Durham, North Carolina 27708, USA
  • 4Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
  • 5Department of Chemistry and Biochemistry, University of Maryland, College Park, Maryland 20742, USA
  • 6Department of Physics, University of Jyväskylä, FI-40014 Jyväskylä, Finland

  • *Present address: GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany.
  • †Present address: Department of Physics, Florida State University, Tallahassee, Florida 32306, USA.
  • ‡Present address: U.S. Army Research Laboratory, Adelphi, Maryland 20783, USA.
  • §Deceased

Phys. Rev. C 105, L042801 – Published 4 April, 2022

DOI: https://doi.org/10.1103/PhysRevC.105.L042801

Abstract

The γ-decay properties of an excited state in Al26 at 6398.3(8) keV have been reexamined using the B11+O16 fusion-evaporation reaction. This level represents a key 93.1(8)-keV resonance in the Mg25+p system and its relative branching to the Al26 ground state, f0, has been determined to be 0.76±0.03 (stat.) ±0.10 (syst.). This is a significantly higher value than the most recent evaluation and implies a considerable increase in the production of cosmic γ rays from Al26 radioactivity.

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