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        Implications of Sm-151(n,gamma) cross section at n_TOF

        Author
        Marrone, S.
        Abbondanno, U.
        Aerts, G.
        Alvarez, H.
        Alvarez-Velarde, F.
        Andriamonje, S.
        Andrzejewski, J.
        Assimakopoulos, P.
        Audouin, L.
        Badurek, G.
        Baumann, P.
        Bevcar, F.
        Berthoumieux, E.
        Calvino, F.
        Cano-Ott, D.
        Capote, R.
        De Albornoz, A. Carrillo
        Cennini, P.
        Chepell, V.
        Chiaveri, E.
        Colonna, N.
        Cortes, G.
        Couture, A.
        Cox, J.
        David, S.
        Dolfini, R.
        Domingo-Pardo, C.
        Dahlfors, M.
        Dridi, W.
        Duran, I.
        Eleftheriadis, C.
        Embid-Segura, M.
        Ferrant, L.
        Feffari, A.
        Ferreira-Marques, R.
        Fitzpatrick, L.
        Frais-Koelb, H.
        Fujii, K.
        Furman, W.
        Guerrer, C.
        Goncalves, I.
        Goverdovski, A.
        Gramegna, F.
        Griesmayer, E.
        Gunsing, F.
        Haas, B.
        Haight, R.
        Heil, M.
        Herrera-Martinez, A.
        Igashira, M.
        Isaev, S.
        Jericha, E.
        Kadi, Y.
        Kappeler, F.
        Karamanis, D.
        Karadimos, D.
        Kerveno, M.
        Ketlerov, V.
        Koehler, P.
        Konovalov, V.
        Kossionides, E.
        Krticka, M.
        Lamboudis, C.
        Leeb, H.
        Lindote, A.
        Lopes, I.
        Lozano, M.
        Lukic, S.
        Marganiec, J.
        Marques, L.
        Mastinu, P.
        Mengoni, A.
        Milazzo, P. M.
        Moreau, C.
        Mosconi, M.
        Neves, F.
        Oberhummer, H.
        O'Brien, S.
        Oshima, M.
        Pancin, J.
        Papachristodoulou, C.
        Papadopoulos, C. T.
        Paradela, C.
        Patronis, N.
        Pavlik, A.
        Pavlopoulos, P.
        Perrot, L.
        Plag, R.
        Plompen, A.
        Plukis, A.
        Poch, A.
        Pretel, C.
        Quesada, J.
        Rauscher, T.
        Reifarth, R.
        Rosetti, M.
        Rubbia, C.
        Rudolf, G.
        Rullhusen, P.
        Salgado, J.
        Sarchiapone, L.
        Savvidis, I.
        Stephan, C.
        Tagliente, G.
        Tain, J. L.
        Tassan-Got, L.
        Tavora, L.
        Terlizzi, R.
        Dillmann, I.
        Vannini, G.
        Vaz, P.
        Ventura, A.
        Villamarin, D.
        Vincente, M. C.
        Vlachoudis, V.
        Vlastou, R.
        Voss, F.
        Walter, S.
        Wendler, H.
        Wiescher, M.
        Wisshak, K.
        Attention
        2299/14866
        Abstract
        The accurate knowledge of the Sm-151(n,gamma) cross section has important implications for the nuclear technologies as well as for fundamental studies. Due to its radioactivity, the only experimental data available on Sm-151 were derived from a transmission measurement [1]. Nowadays thanks to the innovative features of neutron time-of-flight facility (n_TOF), it was possible to measure Sm-151(n,gamma) cross section in a wide energy range and with good accuracy [2]. We present, here, the main experimental results together with the implications concerning the nuclear astrophysical part.
        Publication date
        2006
        Published in
        Frontiers in Nuclear Structure Astrophysics, and Reactions: FINUSTAR
        Other links
        http://hdl.handle.net/2299/14866
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