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Vlastou, R |
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dc.contributor.author |
Voss, F |
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dc.contributor.author |
Walter, S |
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dc.contributor.author |
Wendler, H |
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Wiescher, M |
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dc.contributor.author |
Wisshak, K |
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dc.date.accessioned |
2014-03-01T02:50:24Z |
|
dc.date.available |
2014-03-01T02:50:24Z |
|
dc.date.issued |
2006 |
en |
dc.identifier.issn |
0094243X |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/35111 |
|
dc.subject |
151Sm |
en |
dc.subject |
Level density |
en |
dc.subject |
Neutron capture |
en |
dc.subject |
Neutron strength function |
en |
dc.subject |
Nucleosynthesis |
en |
dc.subject |
s process |
en |
dc.title |
Implications of151Sm(n,γ) cross section at n_TOF |
en |
heal.type |
conferenceItem |
en |
heal.identifier.primary |
10.1063/1.2200996 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1063/1.2200996 |
en |
heal.publicationDate |
2006 |
en |
heal.abstract |
The accurate knowledge of the151Sm(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 on151Sm were derived from a transmission measurement. Nowadays thanks to the innovative features of neutron time-of-flight facility (n_TOF), it was possible to measure151Sm(n,γ) 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. © 2006 American Institute of Physics. |
en |
heal.journalName |
AIP Conference Proceedings |
en |
dc.identifier.doi |
10.1063/1.2200996 |
en |
dc.identifier.volume |
831 |
en |
dc.identifier.spage |
502 |
en |
dc.identifier.epage |
504 |
en |