Measurement of the 17 O(p,γ)18F reaction rate at astrophysically relevant energies

U. Hager, L. Buchmann, B. Davids, J. Fallis, B. R. Fulton, N. Galinski, U. Greife, D. A. Hutcheon, D. Ottewell, A. Rojas, C. Ruiz, and K. Setoodehnia
Phys. Rev. C 85, 035803 – Published 14 March 2012

Abstract

The 17O(p,γ)18F reaction plays an important role in hydrogen-burning nucleosynthesis. Conflicting values for the low-energy behavior of its cross section exist in the literature. We present direct measurements of the astrophysical S factor of the 17O(p,γ)18F reaction at center-of-mass energies between 250 and 500 keV. These measurements were conducted in inverse kinematics at the DRAGON recoil separator.

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  • Received 15 November 2011

DOI:https://doi.org/10.1103/PhysRevC.85.035803

©2012 American Physical Society

Authors & Affiliations

U. Hager1,*, L. Buchmann2, B. Davids2, J. Fallis2, B. R. Fulton3, N. Galinski2, U. Greife1, D. A. Hutcheon2, D. Ottewell2, A. Rojas2, C. Ruiz2, and K. Setoodehnia4

  • 1Colorado School of Mines, Golden, Colorado, USA
  • 2TRIUMF, Vancouver, Canada V6T 2A3
  • 3Department of Physics, University of York, York YO10 5DD, United Kingdom
  • 4McMaster University, Hamilton, Ontario, Canada

  • *uhager@mines.edu

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Issue

Vol. 85, Iss. 3 — March 2012

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