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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 |
Wisshak, K |
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dc.date.accessioned |
2014-03-01T02:00:47Z |
|
dc.date.available |
2014-03-01T02:00:47Z |
|
dc.date.issued |
2010 |
en |
dc.identifier.issn |
0556-2813 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/29132 |
|
dc.subject.classification |
Physics, Nuclear |
en |
dc.subject.other |
CAPTURE CROSS-SECTIONS |
en |
dc.subject.other |
GIANT BRANCH STARS |
en |
dc.subject.other |
NEUTRON-CAPTURE |
en |
dc.subject.other |
N-TOF |
en |
dc.subject.other |
ENERGY RANGE |
en |
dc.subject.other |
ZR ISOTOPES |
en |
dc.subject.other |
S-PROCESS |
en |
dc.subject.other |
FACILITY |
en |
dc.subject.other |
ELEMENTS |
en |
dc.subject.other |
CERN |
en |
dc.title |
The Zr-92(n,gamma) reaction and its implications for stellar nucleosynthesis |
en |
heal.type |
journalArticle |
en |
heal.identifier.secondary |
055801 |
en |
heal.language |
English |
en |
heal.publicationDate |
2010 |
en |
heal.abstract |
Because the relatively small neutron capture cross sections of the zirconium isotopes are difficult to measure, the results of previous measurements are often not adequate for a number of problems in astrophysics and nuclear technology. Therefore, the Zr-92(n,gamma) cross section has been remeasured at the CERN n_TOF facility, providing a set of improved parameters for 44 resonances in the neutron energy range up to 40 keV. With this information the cross-section uncertainties in the keV region could be reduced to 5% as required for s-process nucleosynthesis studies and technological applications. |
en |
heal.publisher |
AMER PHYSICAL SOC |
en |
heal.journalName |
PHYSICAL REVIEW C |
en |
dc.identifier.isi |
ISI:000278144800074 |
en |
dc.identifier.volume |
81 |
en |
dc.identifier.issue |
5 |
en |