dc.contributor.author |
Mosconi, M |
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dc.contributor.author |
Heil, M |
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dc.contributor.author |
Kappeler, F |
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dc.contributor.author |
Plag, R |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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dc.contributor.author |
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 |
Wiescher, M |
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dc.contributor.author |
Wisshak, K |
en |
dc.date.accessioned |
2014-03-01T01:28:52Z |
|
dc.date.available |
2014-03-01T01:28:52Z |
|
dc.date.issued |
2008 |
en |
dc.identifier.issn |
0954-3899 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/19013 |
|
dc.subject.classification |
Physics, Nuclear |
en |
dc.subject.classification |
Physics, Particles & Fields |
en |
dc.subject.other |
NEUTRON CROSS-SECTIONS |
en |
dc.subject.other |
INELASTIC-SCATTERING |
en |
dc.subject.other |
NUCLEOSYNTHESIS |
en |
dc.subject.other |
OS-187 |
en |
dc.subject.other |
ISOTOPES |
en |
dc.subject.other |
STARS |
en |
dc.subject.other |
AGE |
en |
dc.title |
Nuclear physics for the Re/Os clock |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1088/0954-3899/35/1/014015 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1088/0954-3899/35/1/014015 |
en |
heal.identifier.secondary |
014015 |
en |
heal.language |
English |
en |
heal.publicationDate |
2008 |
en |
heal.abstract |
Dating the age of the universe by the beta-decay of Re-187 (t(1/2) = 41.2 Gyr) requires the accurate assessment of the s-process reaction flow. The daughter nucleus Os-187 as well as its immediate s-only neighbor Os-186 are shielded from the r-process. Therefore, the radiogenic contribution to Os-187 can be derived via the local approximation of the s-process, which is well justified in this mass region: (<sigma > N-s)(187) = (<sigma > N-s)(186). Accordingly, accurate Maxwellian-averaged (n,gamma) cross sections have to be known for Os-186 and Os-187 over the full range of s-process temperatures. Because Os-187 has low-lying excited states, which are significantly populated during the s-process, neutron captures on these excited states have to be properly taken into account. The input for the corresponding Hauser-Feshbach calculations can be constrained by deriving the strength functions from a detailed resonance analysis of the measured (n,gamma) cross sections as well as by an additional measurement of the inelastic scattering cross section for the first exited level, which dominates the competition between the capture and scattering channels. This contribution reports on measurements of the neutron capture cross sections of Os-186, Os-187 and Os-188 from the eV region to 1MeV at the CERN/n_TOF facility and of the inelastic scattering cross section of Os-187 around 30 keV at the Karlsruhe 3.7 MV Van de Graaff accelerator. Based on these results and on a detailed resonance analysis, improved Maxwellian-averaged cross sections were obtained for thermal energies between 5 keV and 100 keV. The implications of these results for the Re/Os clock are discussed. |
en |
heal.publisher |
IOP PUBLISHING LTD |
en |
heal.journalName |
Journal of Physics G: Nuclear and Particle Physics |
en |
dc.identifier.doi |
10.1088/0954-3899/35/1/014015 |
en |
dc.identifier.isi |
ISI:000252019800016 |
en |
dc.identifier.volume |
35 |
en |
dc.identifier.issue |
1 |
en |