Implications of $^{151}$Sm(n,$\gamma$) Cross Section at n_TOF
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en
Communication dans un congrès
Este ítem está publicado en
Frontiers in Nuclear Structure, Astrophysics, and Reactions - FINUSTAR, Frontiers in Nuclear Structure, Astrophysics, and Reactions - FINUSTAR, 2005-09-12, Isle of Kos. 2006, vol. 831, n° 831, p. 502-504
AIP Press
Resumen en inglés
The accurate knowledge of the $^{151}$Sm(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 ...Leer más >
The accurate knowledge of the $^{151}$Sm(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 $^{151}$Sm were derived from a transmission measurement. Nowadays thanks to the innovative features of neutron time-of-flight facility (n_TOF), it was possible to measure $^{151}$Sm(n,$\gamma$) cross section in a wide energy range and with good accuracy. We present, here, the main experimental results together with the implications concerning the nuclear astrophysical part.< Leer menos
Palabras clave en inglés
neutron radiative capture
samarium
nuclei with mass number 150 to 189
time of flight spectroscopy
astronomy
Orígen
Importado de HalCentros de investigación