Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/40201
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Título : The Zr-92(n,gamma) reaction and its implications for stellar nucleosynthesis
Autor : n_TOF Collaboration, Tagliente, G., Domingo Pardo, César, Taín, José Luis, Colonna, N., Gunsing, F., Mosconi, M., Terlizzi, R.
Fecha de publicación : May-2010
Editor: American Physical Society
Citación : Physical Review - Section C - Nuclear Physics 81 (5): 055801 (2010)
Resumen: 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.
Versión del editor: 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
Citación : Physical Review - Section C - Nuclear Physics 81 (5): 055801 (2010)
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