Show simple item record

dc.contributor.authorHorvath, A.
dc.contributor.authorGalonsky, A.
dc.contributor.authorCarlin, N.
dc.contributor.authorDeak, F.
dc.contributor.authorGomi, T.
dc.contributor.authorGuimaraes, V.
dc.contributor.authorHigurashi, Y.
dc.contributor.authorHiroshi, K.
dc.contributor.authorIeki, K.
dc.contributor.authorIwata, Y.
dc.contributor.authorKiss, A.
dc.contributor.authorKolata, J.
dc.contributor.authorRauscher, T.
dc.contributor.authorSchelin, H.
dc.contributor.authorvon Schwarzenberg, J.
dc.contributor.authorSeres, Z.
dc.contributor.authorTakeuchi, S.
dc.contributor.authorTypel, S.
dc.contributor.authorWarner, R.
dc.contributor.authorWeiner, J.
dc.date.accessioned2013-07-02T12:32:11Z
dc.date.available2013-07-02T12:32:11Z
dc.date.issued2003-05-19
dc.identifier.citationHorvath , A , Galonsky , A , Carlin , N , Deak , F , Gomi , T , Guimaraes , V , Higurashi , Y , Hiroshi , K , Ieki , K , Iwata , Y , Kiss , A , Kolata , J , Rauscher , T , Schelin , H , von Schwarzenberg , J , Seres , Z , Takeuchi , S , Typel , S , Warner , R & Weiner , J 2003 , ' Measurements of astrophysical neutron capture cross sections via the inverse reaction ' , Nuclear Physics A , vol. 719 , pp. 9C-12C . https://doi.org/10.1016/S0375-9474(03)00951-5
dc.identifier.issn0375-9474
dc.identifier.otherPURE: 1631828
dc.identifier.otherPURE UUID: 9d9070d4-3d84-499a-8a99-7b468605a427
dc.identifier.otherWOS: 000182530000003
dc.identifier.otherScopus: 0038119697
dc.identifier.urihttp://hdl.handle.net/2299/11014
dc.description.abstractNeutron capture of short-lived isotopes can be important within several astrophysical environments. The laboratory investigation of these reactions can be difficult since these isotopes cannot form a target. We used radioactive beams and measured the inverse reaction instead. Particularly we used (15)C and (9)Li beams to measure the (14)C(n,gamma)(15)C, and (8)Li(n, gamma)(9)Li reactions. We determined the reaction rates within the astrophysically interesting temperature range. Our data for the (14)C capture rises quickly up to 8mub and then it decreases by a factor of two at 1 MeV. We investigated neutron capture by 8 Li which is one possible leak of the bridging reaction (8)Li(alpha, n)(11)B of the A=8 gap. We found that this leak is lower than the theoretical expectations.en
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofNuclear Physics A
dc.subjectREVERSE KINEMATICS
dc.subjectMICROSCOPIC CLUSTER
dc.subjectC-14(N
dc.subjectLI-8(N
dc.subjectLI-9
dc.titleMeasurements of astrophysical neutron capture cross sections via the inverse reactionen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1016/S0375-9474(03)00951-5
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record