Published April 17, 2009 | Version v1
Journal article

Measurement of the 60Fe(n,γ)61Fe Cross Section at Stellar Temperatures

  • 1. University of Notre Dame, Department of Physics, Notre Dame, Indiana (United States)
  • 2. GSI Darmstadt, Planckstrasse 1, 64291 Darmstadt (Germany)
  • 3. Laboratory for Environmental and Radiochemistry, PSI, 5232 Villigen PSI (Switzerland)
  • 4. Forschungszentrum Karlsruhe, Institut fuer Kernphysik, Postfach 3640, D-76021 Karlsruhe (Germany)
  • 5. University of Lodz (Poland)
  • 6. Keele University, Keele, Staffordshire ST5 5BG (United Kingdom)

Description

Observations of galactic γ-ray activity have challenged the current understanding of nucleosynthesis in massive stars. Recent measurements of 60Fe abundances relative to 26Alg have underscored the need for accurate nuclear information concerning the stellar production of 60Fe. In light of this motivation, a first measurement of the stellar 60Fe(n,γ)61Fe cross section, the predominant destruction mechanism of 60Fe, has been performed by activation at the Karlsruhe Van de Graaff accelerator. Results show a Maxwellian averaged cross section at kT=25 keV of 9.9±1.4(stat)2.8(syst)mbarn, a significant reduction in uncertainty with respect to existing theoretical discrepancies. This result will serve to significantly constrain models of 60Fe nucleosynthesis in massive stars

Additional details

Publishing Information

Journal Title
Physical Review Letters
Journal Volume
102
Journal Issue
15
Journal Page Range
p. 151101-151101.4
ISSN
0031-9007
CODEN
PRLTAO

Optional Information

Notes
(c) 2009 The American Physical Society