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

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. and Wisshak, K. (2006) Implications of Sm-151(n,gamma) cross section at n_TOF. American Institute of Physics (AIP).
Copy

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.

Full text not available from this repository.

EndNote BibTeX Reference Manager Refer Atom Dublin Core Data Cite XML METS MPEG-21 DIDL OpenURL ContextObject in Span OpenURL ContextObject ASCII Citation RIOXX2 XML HTML Citation MODS
Export

Downloads