The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis

Details The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010phrvc..81e5801t&link_type=abstract

Physical Review C, vol. 81, Issue 5, id. 055801

Mathematics

Logic

4

Radiative Capture, Resonances, 90<=A<=149, Structural And Shielding Materials

Scientific paper

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 Zr92(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.

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