Reaction rates for the s-process neutron source 22 Ne + α
| dc.contributor.author | Longland, R | |
| dc.contributor.author | Iliadis, C | |
| dc.contributor.author | Karakas, Amanda | |
| dc.date.accessioned | 2015-12-10T23:27:03Z | |
| dc.date.issued | 2012 | |
| dc.date.updated | 2015-12-10T11:03:43Z | |
| dc.description.abstract | The 22Ne(α,n)25Mg reaction is an important source of neutrons for the s-process. In massive stars responsible for the weak component of the s-process, 22Ne(α,n)25Mg is the dominant source of neutrons, both during core helium burning and in carbon-shell | |
| dc.identifier.issn | 0556-2813 | |
| dc.identifier.uri | http://hdl.handle.net/1885/68040 | |
| dc.publisher | American Physical Society | |
| dc.source | Physical Review C: Nuclear Physics | |
| dc.title | Reaction rates for the s-process neutron source 22 Ne + α | |
| dc.type | Journal article | |
| local.bibliographicCitation.issue | 6 | |
| local.contributor.affiliation | Longland, R, Universitat Politecnica de Catalunya | |
| local.contributor.affiliation | Iliadis, C, University of North Carolina | |
| local.contributor.affiliation | Karakas, Amanda, College of Physical and Mathematical Sciences, ANU | |
| local.contributor.authoruid | Karakas, Amanda, u4382192 | |
| local.description.embargo | 2037-12-31 | |
| local.description.notes | Imported from ARIES | |
| local.identifier.absfor | 020202 - Nuclear Physics | |
| local.identifier.absfor | 020110 - Stellar Astronomy and Planetary Systems | |
| local.identifier.ariespublication | f5625xPUB1598 | |
| local.identifier.citationvolume | 85 | |
| local.identifier.doi | 10.1103/PhysRevC.85.065809 | |
| local.identifier.scopusID | 2-s2.0-84863492174 | |
| local.identifier.thomsonID | 000305605600011 | |
| local.type.status | Published Version |
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