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dc.date.accessioned |
2014-03-01T02:12:08Z |
|
dc.date.available |
2014-03-01T02:12:08Z |
|
dc.date.issued |
2012 |
en |
dc.identifier.issn |
05562813 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/30012 |
|
dc.title |
Resonance neutron-capture cross sections of stable magnesium isotopes and their astrophysical implications |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1103/PhysRevC.85.044615 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1103/PhysRevC.85.044615 |
en |
heal.identifier.secondary |
044615 |
en |
heal.publicationDate |
2012 |
en |
heal.abstract |
We have measured the neutron capture cross sections of the stable magnesium isotopes 24,25,26Mg in the energy range of interest to the s process using the neutron time-of-flight facility n-TOF at CERN. Capture events from a natural metal sample and from samples enriched in 25Mg and 26Mg were recorded using the total energy method based on C62H6 detectors. Neutron resonance parameters were extracted by a simultaneous resonance shape analysis of the present capture data and existing transmission data on a natural isotopic sample. Maxwellian-averaged capture cross sections for the three isotopes were calculated up to thermal energies of 100 keV and their impact on s-process analyses was investigated. At 30 keV the new values of the stellar cross section for 24Mg, 25Mg, and 26Mg are 3.8±0.2 mb, 4.1±0.6 mb, and 0.14±0.01 mb, respectively. © 2012 American Physical Society. |
en |
heal.journalName |
Physical Review C - Nuclear Physics |
en |
dc.identifier.doi |
10.1103/PhysRevC.85.044615 |
en |
dc.identifier.volume |
85 |
en |
dc.identifier.issue |
4 |
en |