English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/40201
Title: The Zr-92(n,gamma) reaction and its implications for stellar nucleosynthesis
Authors: n_TOF Collaboration; Tagliente, G.; Domingo Pardo, César; Taín, José Luis; Colonna, N.; Gunsing, F.; Mosconi, M.; Terlizzi, R.
Issue Date: May-2010
Publisher: American Physical Society
Citation: Physical Review - Section C - Nuclear Physics 81 (5): 055801 (2010)
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 (92)Zr(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.
Publisher version (URL): http://dx.doi.org/10.1103/PhysRevC.81.055801
URI: http://hdl.handle.net/10261/40201
ISSN: 0556-2813
DOI: 10.1103/PhysRevC.81.055801
Appears in Collections:(IFIC) Artículos
Files in This Item:
There are no files associated with this item.
Show full item record

WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.