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dc.contributor.authorRauscher, T.
dc.date.accessioned2013-08-06T13:18:12Z
dc.date.available2013-08-06T13:18:12Z
dc.date.issued2010-04
dc.identifier.citationRauscher , T 2010 , ' Relevant energy ranges for astrophysical reaction rates ' , Physical Review C , vol. 81 , no. 4 , 045807 . https://doi.org/10.1103/PhysRevC.81.045807
dc.identifier.issn2469-9985
dc.identifier.otherPURE: 1618803
dc.identifier.otherPURE UUID: 86f8e415-c40b-4d37-a880-e4c9f7ba7d65
dc.identifier.otherWOS: 000277209500088
dc.identifier.otherScopus: 77951717254
dc.identifier.urihttp://hdl.handle.net/2299/11316
dc.description.abstractEffective energy windows (Gamow windows) of astrophysical reaction rates for (p,gamma), (p,n), (p,alpha), (alpha,gamma), (alpha,n), (alpha,p), (n,gamma), (n,p), and (n,alpha) on targets with 10en
dc.format.extent8
dc.language.isoeng
dc.relation.ispartofPhysical Review C
dc.rightsOpen
dc.titleRelevant energy ranges for astrophysical reaction ratesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2010-04
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1103/PhysRevC.81.045807
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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