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dc.date.accessioned |
2014-03-01T01:34:44Z |
|
dc.date.available |
2014-03-01T01:34:44Z |
|
dc.date.issued |
2010 |
en |
dc.identifier.issn |
05562813 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/20827 |
|
dc.title |
The Zr92(n,γ) reaction and its implications for stellar nucleosynthesis |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1103/PhysRevC.81.055801 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1103/PhysRevC.81.055801 |
en |
heal.identifier.secondary |
055801 |
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 Zr92(n,γ) 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. © 2010 The American Physical Society. |
en |
heal.journalName |
Physical Review C - Nuclear Physics |
en |
dc.identifier.doi |
10.1103/PhysRevC.81.055801 |
en |
dc.identifier.volume |
81 |
en |
dc.identifier.issue |
5 |
en |