@Article{n_TOFCollaborationTagliente_etal2010,
author="n{\_}TOF Collaboration (Tagliente, G. et al
and Domingo-Pardo, C.
and Tain, J. L.",
title="The Zr-92(n,gamma) reaction and its implications for stellar nucleosynthesis",
journal="Physical Review C",
year="2010",
publisher="Amer Physical Soc",
volume="81",
number="5",
pages="055801--9pp",
abstract="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 Zr-92(n,gamma) 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.",
optnote="ISI:000278144800074",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=444), last updated on Tue, 16 Aug 2011 12:31:08 +0000",
issn="0556-2813",
doi="10.1103/PhysRevC.81.055801",
opturl="https://doi.org/10.1103/PhysRevC.81.055801",
language="English"
}