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dc.contributor.authorGaudefroy, L.
dc.contributor.authorSorlin, O.
dc.contributor.authorBeaumel, D.
dc.contributor.authorBlumenfeld, Y.
dc.contributor.authorDombradi, Z.
dc.contributor.authorFortier, S.
dc.contributor.authorFranchoo, S.
dc.contributor.authorGelin, M.
dc.contributor.authorGibelin, J.
dc.contributor.authorGrevy, S.
dc.contributor.authorHammache, F.
dc.contributor.authorIbrahim, F.
dc.contributor.authorKemper, K.
dc.contributor.authorKratz, K.L.
dc.contributor.authorLukyanov, S. M.
dc.contributor.authorMonrozeau, C.
dc.contributor.authorNalpas, L.
dc.contributor.authorNowacki, F.
dc.contributor.authorOstrowski, A. N.
dc.contributor.authorPenionzhkevich, Yu. -E.
dc.contributor.authorPollacco, E.
dc.contributor.authorRoussel-Chomaz, P.
dc.contributor.authorRich, E.
dc.contributor.authorScarpaci, J. A.
dc.contributor.authorLaurent, M. G. St.
dc.contributor.authorRauscher, T.
dc.contributor.authorSohler, D.
dc.contributor.authorStanoiu, M.
dc.contributor.authorTryggestad, E.
dc.contributor.authorVerney, D.
dc.date.accessioned2013-07-02T10:17:00Z
dc.date.available2013-07-02T10:17:00Z
dc.date.issued2006-03
dc.identifier.citationGaudefroy , L , Sorlin , O , Beaumel , D , Blumenfeld , Y , Dombradi , Z , Fortier , S , Franchoo , S , Gelin , M , Gibelin , J , Grevy , S , Hammache , F , Ibrahim , F , Kemper , K , Kratz , K L , Lukyanov , S M , Monrozeau , C , Nalpas , L , Nowacki , F , Ostrowski , A N , Penionzhkevich , Y -E , Pollacco , E , Roussel-Chomaz , P , Rich , E , Scarpaci , J A , Laurent , M G S , Rauscher , T , Sohler , D , Stanoiu , M , Tryggestad , E & Verney , D 2006 , ' Study of the N=28 shell closure in the Ar isotopic chain : a SPIRAL experiment for nuclear astrophysics ' , European Physical Journal A: Hadrons and Nuclei , vol. 27 , no. supp 1 , pp. 309-314 . https://doi.org/10.1140/epja/i2006-08-047-0
dc.identifier.issn1434-6001
dc.identifier.otherPURE: 1626486
dc.identifier.otherPURE UUID: d114e8c9-0272-4e3a-8216-f81f989dc580
dc.identifier.otherWOS: 000208079500048
dc.identifier.otherScopus: 33646429187
dc.identifier.urihttp://hdl.handle.net/2299/11000
dc.description.abstractThe structure of the neutron-rich nucleus (47)Ar has been investigated through the d((46)Ar,(47)Ar)p transfer reaction. The radioactive beam of (46)Ar at 10 A . MeV was provided by the SPIRAL facility at GANIL. The protons corresponding to a neutron pick-up on bound or unbound states mechanism in (47)Ar nuclei were detected at backward angles by the position-sensitive Si array-detector MUST. The transfer-like ejectiles were detected in the SPEG spectrometer. Level scheme, spin assignments and spectroscopic factors have been deduced for (47)Ar and compared to shell model predictions. They suggest a slight erosion of the N = 28 shell gap from the weakening of the spin-orbit interaction arising from the f and p orbitals. These spectroscopic information are subsequently used to infer (n, gamma) reaction rates in the Ar isotopic chain to understand the origin of the (48)Ca/(46)Ca abnormal isotopic ratio observed in certain inclusions of meteorites.en
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofEuropean Physical Journal A: Hadrons and Nuclei
dc.titleStudy of the N=28 shell closure in the Ar isotopic chain : a SPIRAL experiment for nuclear astrophysicsen
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
dcterms.dateAccepted2006-03
rioxxterms.versionofrecordhttps://doi.org/10.1140/epja/i2006-08-047-0
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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