Presentation
Implications of Sm-151(n,gamma) cross section at n_TOF
Author/s | Marrone, S.
Abbondanno, U. Aerts, G. Capote del Villar, Ramón Lozano Leyva, Manuel Luis Quesada Molina, José Manuel Wisshak, K. |
Department | Universidad de Sevilla. Departamento de Física Atómica, Molecular y Nuclear |
Publication Date | 2006 |
Deposit Date | 2020-09-18 |
Published in |
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ISBN/ISSN | 0-7354-0323-6 0094-243X (impreso) 1551-7616 (electrónico) |
Abstract | The accurate knowledge of the 151Sm(n,γ) 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 151Sm ... The accurate knowledge of the 151Sm(n,γ) 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 151Sm 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 151Sm(n,γ) 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. |
Funding agencies | European Commission (EC) |
Project ID. | FIKW-CT-2000-00107 |
Citation | Marrone, S., Abbondanno, U., Aerts, G., Capote del Villar, R., Lozano Leyva, M.L., Quesada Molina, J.M. y Wisshak, K. (2006). Implications of Sm-151(n,gamma) cross section at n_TOF. En International Conference on Frontiers in Nuclear Structure, Astrophysics and Reactions (FINUSTAR) (502-504), Isla de Kos, (Grecia): American Institute of Physics. |
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