@Article{n_TOFCollaborationPraena_etal2018,
author="n{\_}TOF Collaboration (Praena, J. et al
and Domingo-Pardo, C.
and Giubrone, G.
and Tain, J. L.
and Tarife{\~{n}}o-Saldivia, A.",
title="Measurement and resonance analysis of the S-33(n,alpha)Si-30 cross section at the CERN n{\_}TOF facility in the energy region from 10 to 300 keV",
journal="Physical Review C",
year="2018",
publisher="Amer Physical Soc",
volume="97",
number="6",
pages="064603--10pp",
abstract="The (33)(n , alpha)Si-30 cross section has been measured at the neutron time-of-flight (n{\_}TOF) facility at CERN in the neutron energy range from 10 to 300 keV relative to the B-10(n, alpha)(7) Li cross-section standard. Both reactions were measured simultaneously with a set of micromegas detectors. The flight path of 185 m has allowed us to obtain the cross section with high-energy resolution. An accurate description of the resonances has been performed by means of the multilevel multichannel R-matrix code SAMMY. The results show a significantly higher area of the biggest resonance (13.45 keV) than the unique high-resolution (n , alpha) measurement. The new parametrization of the 13.45-keV resonance is similar to that of the unique transmission measurement. This resonance is a matter of research in neutron-capture therapy. The S-33(n, alpha)Si-30 cross section has been studied in previous works because of its role in the production of S-36 in stars, which is currently overproduced in stellar models compared to observations.",
optnote="WOS:000434017300004",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=3597), last updated on Tue, 13 Oct 2020 12:47:29 +0000",
issn="2469-9985",
doi="10.1103/PhysRevC.97.064603",
opturl="https://doi.org/10.1103/PhysRevC.97.064603",
language="English"
}