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Phys. Rev. C 81, 055801 (2010) [9 pages]

The 92Zr(n,γ) reaction and its implications for stellar nucleosynthesis

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G. Tagliente et al. (n_TOF Collaboration)
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Received 22 April 2009; revised 26 February 2010; published 5 May 2010

Because the relatively small neutron capture cross sections of the zirconium isotopes are difficult to measure, the results of previous measurements are often not adequate for a number of problems in astrophysics and nuclear technology. Therefore, the 92Zr(n,γ) cross section has been remeasured at the CERN n_TOF facility, providing a set of improved parameters for 44 resonances in the neutron energy range up to 40 keV. With this information the cross-section uncertainties in the keV region could be reduced to 5% as required for s-process nucleosynthesis studies and technological applications.

© 2010 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.81.055801
DOI:
10.1103/PhysRevC.81.055801
PACS:
25.40.Lw, 25.70.Ef, 27.60.+j, 28.41.Qb