%0 Journal Article
%T The Zr-92(n,gamma) reaction and its implications for stellar nucleosynthesis
%A n_TOF Collaboration (Tagliente, G. et al
%A Domingo-Pardo, C.
%A Tain, J. L.
%J Physical Review C
%D 2010
%V 81
%N 5
%I Amer Physical Soc
%@ 0556-2813
%G English
%F n_TOFCollaborationTagliente_etal2010
%O ISI:000278144800074
%O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=444), last updated on Tue, 16 Aug 2011 12:31:08 +0000
%X 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.
%R 10.1103/PhysRevC.81.055801
%U https://doi.org/10.1103/PhysRevC.81.055801
%P 055801-9pp