학술논문

High-resolution cross section measurements for neutron interactions on 89Y with incident neutron energies up to 95 keV
Document Type
Original Paper
Author
Tagliente, G.Milazzo, P. M.Paradela, C.Kopecky, S.Vescovi, D.Alaerts, G.Damone, L. A.Heyse, J.Krtička, M.Schillebeeckx, P.Mengoni, A.Wynants, R.Valenta, S.Aberle, O.Alcayne, V.Amaducci, S.Andrzejewski, J.Audouin, L.Babiano-Suarez, V.Bacak, M.Barbagallo, M.Bécares, V.Bečvář, F.Bellia, G.Berthoumieux, E.Billowes, J.Bosnar, D.Brown, A. S.Busso, M.Caamaño, M.Caballero, L.Calviani, M.Calviño, F.Cano-Ott, D.Casanovas, A.Cerutti, F.Chen, Y. H.Chiaveri, E.Colonna, N.Cortés, G. P.Cortés-Giraldo, M. A.Cosentino, L.Cristallo, S.Diakaki, M.Dietz, M.Domingo-Pardo, C.Dressler, R.Dupont, E.Durán, I.Eleme, Z.Fernández-Domíngez, B.Ferrari, A.Ferro-Gonçalves, I.Finocchiaro, P.Furman, V.Garg, R.Gawlik, A.Gilardoni, S.Glodariu, T.Göbel, K.González-Romero, E.Guerrero, C.Gunsing, F.Heinitz, S.Jenkins, D. G.Jericha, E.Kadi, Y.Käppeler, F.Kimura, A.Kivel, N.Kokkoris, M.Kopatch, Y.Kurtulgil, D.Ladarescu, I.Larsen, A. C.Lederer-Woods, C.Lerendegui-Marco, J.Lo Meo, S.Lonsdale, S. J.Lugaro, M.Macina, D.Manna, A.Martínez, T.Masi, A.Massimi, C.Mastinu, P. F.Mastromarco, M.Matteucci, F.Maugeri, E.Mazzone, A.Mendoza, E.Michalopoulou, V.Mingrone, F.Musumarra, A.Negret, A.Nolte, R.Ogállar, F.Oprea, A.Patronis, N.Pavlik, A.Perkowski, J.Piersanti, L.Porras, I.Praena, J.Quesada, J. M.Radeck, D.Ramos Doval, D.Reifarth, R.Rochman, D.Rubbia, C.Sabaté-Gilarte, M.Saxena, A.Schumann, D.Smith, A. G.Spelta, M.Sosnin, N.Stamatopoulos, A.Tain, J. L.Talip, Z.Tarifeño-Saldivia, A. E.Tassan-Got, L.Torres-Sánchez, P.Tsinganis, A.Ulrich, J.Urlass, S.Vannini, G.Variale, V.Vaz, P.Ventura, A.Vlachoudis, V.Vlastou, R.Wallner, A.Woods, P. J.Wright, T. J.Žugec, P.
Source
The European Physical Journal A: Hadrons and Nuclei. 60(1)
Subject
Language
English
ISSN
1434-601X
Abstract
The cross section of the 89γ8989Y(n, 89γ8989) reaction has important implications in nuclear astrophysics and for advanced nuclear technology. Given its neutron magic number N = 50 and a consequent small neutron capture cross section, 89γ8989Y represents one of the key nuclides for the stellar s-process. It acts as a bottleneck in the neutron capture chain between the Fe seed and the heavier elements. Moreover, it is located at the overlapping region, where both the weak and main s-process components take place. 89γ8989Y, the only stable yttrium isotope, is also used in innovative nuclear reactors. Neutron capture and transmission measurements were performed at the time-of-flight facilities n_TOF at CERN and GELINA at JRC-Geel. Resonance parameters of individual resonances were extracted from a resonance analysis of the experimental transmission and capture yields, up to a neutron incident energy of 95 keV. Even though a comparison with results reported in the literature shows differences in resonance parameters, the present data are consistent with the Maxwellian averaged cross section suggested by the astrophysical database KADoNiS.