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Domingo-Pardo, C |
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dc.contributor.author |
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dc.contributor.author |
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Walter, S |
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dc.contributor.author |
Wisshak, K |
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dc.date.accessioned |
2014-03-01T01:57:38Z |
|
dc.date.available |
2014-03-01T01:57:38Z |
|
dc.date.issued |
2008 |
en |
dc.identifier.issn |
0954-3899 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/28456 |
|
dc.subject.classification |
Physics, Nuclear |
en |
dc.subject.classification |
Physics, Particles & Fields |
en |
dc.subject.other |
GALACTIC CHEMICAL EVOLUTION |
en |
dc.subject.other |
NEUTRON-CAPTURE |
en |
dc.subject.other |
STARS |
en |
dc.subject.other |
ELEMENTS |
en |
dc.subject.other |
CHRONOMETERS |
en |
dc.subject.other |
LEAD |
en |
dc.title |
The measurement of the Pb-206(n,gamma) cross section and stellar implications |
en |
heal.type |
journalArticle |
en |
heal.identifier.secondary |
014020 |
en |
heal.language |
English |
en |
heal.publicationDate |
2008 |
en |
heal.abstract |
The neutron capture cross section of Pb-206 has been measured at the CERN n_TOF spectrometer using a setup of two C6D6 detectors. In the energy interval from 1 eV to 600 keV the cross section is dominated by resonances, which were analyzed via the R-matrix analysis code SAMMY. In the relevant energy ranges for stellar nucleosynthesis, i. e., at thermal energies of kT = 8 keV and kT = 23 keV, the present Maxwellian average cross section differs by 20% and 9% from the recommended values of Bao et al respectively. From the new cross section the s-abundance of Pb-206 could be reliably determined as 70( 4)%. This result is of importance in order to test and constrain r-process abundance calculations in the actinide region, because the r-process portion of Pb-206 is dominated by alpha-back decays of short-lived transbismuth isotopes. |
en |
heal.publisher |
IOP PUBLISHING LTD |
en |
heal.journalName |
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS |
en |
dc.identifier.isi |
ISI:000252019800021 |
en |
dc.identifier.volume |
35 |
en |
dc.identifier.issue |
1 |
en |