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Reaction rates for the s-process neutron source 22 Ne + α

dc.contributor.authorLongland, R
dc.contributor.authorIliadis, C
dc.contributor.authorKarakas, Amanda
dc.date.accessioned2015-12-10T23:27:03Z
dc.date.issued2012
dc.date.updated2015-12-10T11:03:43Z
dc.description.abstractThe 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.issn0556-2813
dc.identifier.urihttp://hdl.handle.net/1885/68040
dc.publisherAmerican Physical Society
dc.sourcePhysical Review C: Nuclear Physics
dc.titleReaction rates for the s-process neutron source 22 Ne + α
dc.typeJournal article
local.bibliographicCitation.issue6
local.contributor.affiliationLongland, R, Universitat Politecnica de Catalunya
local.contributor.affiliationIliadis, C, University of North Carolina
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidKarakas, Amanda, u4382192
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020202 - Nuclear Physics
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB1598
local.identifier.citationvolume85
local.identifier.doi10.1103/PhysRevC.85.065809
local.identifier.scopusID2-s2.0-84863492174
local.identifier.thomsonID000305605600011
local.type.statusPublished Version

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