Ponencia
Implications of Sm-151(n,gamma) cross section at n_TOF
Autor/es | Marrone, S.
Abbondanno, U. Aerts, G. Capote del Villar, Ramón Lozano Leyva, Manuel Luis Quesada Molina, José Manuel Wisshak, K. |
Departamento | Universidad de Sevilla. Departamento de Física Atómica, Molecular y Nuclear |
Fecha de publicación | 2006 |
Fecha de depósito | 2020-09-18 |
Publicado en |
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ISBN/ISSN | 0-7354-0323-6 0094-243X (impreso) 1551-7616 (electrónico) |
Resumen | 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. |
Agencias financiadoras | European Commission (EC) |
Identificador del proyecto | FIKW-CT-2000-00107 |
Cita | 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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