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
Date Issued
2018-01-01
Author(s)
Praena, J.
Sabate-Gilarte, M.
Porras, I.
Quesada, J. M.
Altstadt, S.
Andrzejewski, J.
Audouin, L.
Becares, V.
Barbagallo, M.
Becvar, F.
Belloni, F.
Berthoumieux, E.
Billowes, J.
Boccone, V.
Bosnar, D.
Brugger, M.
Calvino, F.
Calviani, M.
Cano-Ott, D.
Carrapico, C.
Cerutti, F.
Chiaveri, E.
Chin, M.
Colonna, N.
Cortes, G.
Cortes-Giraldo, M. A.
Diakaki, M.
Dietz, M.
Domingo-Pardo, C.
Dressler, R.
Duran, I.
Eleftheriadis, C.
Ferrari, A.
Fraval, K.
Furman, V.
Goebel, K.
Gomez-Hornillos, M. B.
Ganesan, S.
Garcia, A. R.
Giubrone, G.
Goncalves, I. F.
Gonzalez-Romero, E.
Goverdovski, A.
Griesmayer, E.
Guerrero, C.
Gunsing, F.
Heftrich, T.
Hernandez-Prieto, A.
Heyse, J.
Jenkins, D. G.
Jericha, E.
Kaeppeler, F.
Kadi, Y.
Karadimos, D.
Katabuchi, T.
Ketlerov, V.
Khryachkov, V.
Kivel, N.
Koehler, P.
Kokkoris, M.
Kroll, J.
Krticka, M.
Lampoudis, C.
Langer, C.
Leal-Cidoncha, E.
Lederer-Woods, C.
Leeb, H.
Leong, L. S.
Lerendegui-Marco, J.
Losito, R.
Mallick, A.
Manousos, A.
Marganiec, J.
Martinez, T.
Massimi, C.
Mastinu, P.
Mastromarco, M.
Mendoza, E.
Mengoni, A.
Milazzo, P. M.
Mingrone, F.
Mirea, M.
Mondelaers, W.
Paradela, C.
Pavlik, A.
Perkowski, J.
Plompen, A. J. M.
Reifarth, R.
Riego-Perez, A.
Robles, M.
Rubbia, C.
Ryan, J. A.
Sarmento, R.
Saxena, A.
Schillebeeckx, P.
Schmidt, S.
Schumann, D.
Sedyshev, P.
Tagliente, G.
Tain, J. L.
Tarifeno-Saldivia, A.
Tarrio, D.
Tassan-Got, L.
Tsinganis, A.
Valenta, S.
Vannini, G.
Variale, V.
Vaz, P.
Ventura, A.
Vermeulen, M. J.
Vlachoudis, V.
Vlastou, R.
Wallner, A.
Ware, T.
Weigand, M.
Weiss, C.
Wright, T.
Zugec, P.
DOI
10.1103/physrevc.97.064603
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.
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