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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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Wendler, H |
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Wisshak, K |
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dc.date.accessioned |
2014-03-01T01:24:43Z |
|
dc.date.available |
2014-03-01T01:24:43Z |
|
dc.date.issued |
2006 |
en |
dc.identifier.issn |
0556-2813 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/17410 |
|
dc.subject.classification |
Physics, Nuclear |
en |
dc.subject.other |
GALACTIC CHEMICAL EVOLUTION |
en |
dc.subject.other |
CROSS-SECTION |
en |
dc.subject.other |
S-PROCESS |
en |
dc.subject.other |
CHRONOMETERS |
en |
dc.subject.other |
ABUNDANCES |
en |
dc.subject.other |
FACILITY |
en |
dc.subject.other |
DETECTOR |
en |
dc.subject.other |
ELEMENTS |
en |
dc.subject.other |
SYSTEM |
en |
dc.subject.other |
STARS |
en |
dc.title |
New measurement of neutron capture resonances in Bi209 |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1103/PhysRevC.74.025807 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1103/PhysRevC.74.025807 |
en |
heal.identifier.secondary |
025807 |
en |
heal.language |
English |
en |
heal.publicationDate |
2006 |
en |
heal.abstract |
The neutron capture cross section of Bi209 has been measured at the CERN n_TOF facility by employing the pulse-height-weighting technique. Improvements over previous measurements are mainly because of an optimized detection system, which led to a practically negligible neutron sensitivity. Additional experimental sources of systematic error, such as the electronic threshold in the detectors, summing of γ-rays, internal electron conversion, and the isomeric state in bismuth, have been taken into account. γ-Ray absorption effects inside the sample have been corrected by employing a nonpolynomial weighting function. Because Bi209 is the last stable isotope in the reaction path of the stellar s-process, the Maxwellian averaged capture cross section is important for the recycling of the reaction flow by α decays. In the relevant stellar range of thermal energies between kT=5 and 8 keV our new capture rate is about 16% higher than the presently accepted value used for nucleosynthesis calculations. At this low temperature an important part of the heavy Pb-Bi isotopes are supposed to be synthesized by the s-process in the He shells of low mass, thermally pulsing asymptotic giant branch stars. With the improved set of cross sections we obtain an s-process fraction of 19±3% of the solar bismuth abundance, resulting in an r-process residual of 81±3%. The present (n,γ) cross-section measurement is also of relevance for the design of accelerator driven systems based on a liquid metal Pb/Bi spallation target. © 2006 The American Physical Society. |
en |
heal.publisher |
AMERICAN PHYSICAL SOC |
en |
heal.journalName |
Physical Review C - Nuclear Physics |
en |
dc.identifier.doi |
10.1103/PhysRevC.74.025807 |
en |
dc.identifier.isi |
ISI:000240239100068 |
en |
dc.identifier.volume |
74 |
en |
dc.identifier.issue |
2 |
en |