Thermonuclear rate for the F19(α,p)Ne22 reaction at stellar temperatures

C. Ugalde, R. E. Azuma, A. Couture, J. Görres, H. Y. Lee, E. Stech, E. Strandberg, W. Tan, and M. Wiescher
Phys. Rev. C 77, 035801 – Published 10 March 2008

Abstract

The F19(α,p)Ne22 reaction is considered to be one of the main sources of fluorine depletion in AGB and Wolf-Rayet stars. The reaction rate still retains large uncertainties due to the lack of experimental studies available. In this work the yields for both exit channels to the ground state and first excited state of Ne22 have been measured and several previously unobserved resonances have been found in the energy range Elab=7921993 keV. The level parameters have been determined through a detailed R-matrix analysis of the reaction data and a new reaction rate is provided on the basis of the available experimental information.

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  • Received 15 October 2007

DOI:https://doi.org/10.1103/PhysRevC.77.035801

©2008 American Physical Society

Authors & Affiliations

C. Ugalde*

  • Department of Physics and The Joint Institute for Nuclear Astrophysics, University of Notre Dame, Notre Dame, Indiana 46556, USA, Department of Physics and Astronomy, University of North Carolina, Chapel Hill, North Carolina 27599, USA, and Triangle Universities Nuclear Laboratory, Box 90308, Durham, North Carolina 27708, USA

R. E. Azuma

  • Department of Physics, University of Toronto, Toronto, Ontario M55 1A7, Canada and The Joint Institute for Nuclear Astrophysics, Notre Dame, Indiana 46556, USA

A. Couture, J. Görres, H. Y. Lee, E. Stech, E. Strandberg, W. Tan, and M. Wiescher

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

  • *cugalde@unc.edu
  • Now at Los Alamos Neutron Science Center, Los Alamos National Laboratory, Los Alamos, New Mexico 87544, USA.
  • Now at Argonne National Laboratory, Argonne, Illinois 60439, USA.

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Issue

Vol. 77, Iss. 3 — March 2008

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