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Coulomb Excitation of Sn-104 and the Strength of the Sn-100 Shell Closure

dc.contributor.authorJolie, J.
dc.contributor.authorWeick, H.
dc.contributor.authorWendt, A.
dc.contributor.authorWieland, O.
dc.contributor.authorWinfield, J. S.
dc.contributor.authorWollersheim, H. J.
dc.contributor.authorFarinon, F.
dc.contributor.authorGerl, J.
dc.contributor.authorGoel, N.
dc.contributor.authorGrebosz, J.
dc.contributor.authorHabermann, T.
dc.contributor.authorHoischen, R.
dc.contributor.authorJansson, K.
dc.contributor.authorJungclaus, A.
dc.contributor.authorKojouharov, I.
dc.contributor.authorKnoebel, R.
dc.contributor.authorKumar, R.
dc.contributor.authorKurcewicz, J.
dc.contributor.authorKurz, N.
dc.contributor.authorLalovic, N.
dc.contributor.authorMerchan, E.
dc.contributor.authorMoschner, K.
dc.contributor.authorNaqvi, F.
dc.contributor.authorSingh, B. S. Nara
dc.contributor.authorNyberg, J.
dc.contributor.authorNociforo, C.
dc.contributor.authorGuastalla, G.
dc.contributor.authorDiJulio, D. D.
dc.contributor.authorGorska, M.
dc.contributor.authorCederkall, J.
dc.contributor.authorBoutachkov, P.
dc.contributor.authorGolubev, P.
dc.contributor.authorPietri, S.
dc.contributor.authorGrawe, H.
dc.contributor.authorNowacki, F.
dc.contributor.authorSieja, K.
dc.contributor.authorAlgora, A.
dc.contributor.authorAmeil, F.
dc.contributor.authorArici, T.
dc.contributor.authorAtac, A.
dc.contributor.authorBentley, M. A.
dc.contributor.authorBlazhev, A.
dc.contributor.authorBloor, D.
dc.contributor.authorBrambilla, S.
dc.contributor.authorBraun, N.
dc.contributor.authorCamera, F.
dc.contributor.authorDombradi, Zs.
dc.contributor.authorDomingo Pardo, C.
dc.contributor.authorEstrade, A.
dc.contributor.authorObertelli, A.
dc.contributor.authorPfuetzner, M.
dc.contributor.authorPietralla, N.
dc.contributor.authorPodolyak, Z.
dc.contributor.authorProchazka, A.
dc.contributor.authorRalet, D.
dc.contributor.authorReiter, P.
dc.contributor.authorRudolph, D.
dc.contributor.authorSchaffner, H.
dc.contributor.authorSchirru, F.
dc.contributor.authorScruton, L.
dc.contributor.authorSohler, D.
dc.contributor.authorSwaleh, T.
dc.contributor.authorTaprogge, J.
dc.contributor.authorVajta, Zs.
dc.contributor.authorWadsworth, R.
dc.contributor.authorWarr, N.
dc.date.accessioned2021-03-03T15:57:15Z
dc.date.available2021-03-03T15:57:15Z
dc.date.issued2013
dc.identifier.citationGuastalla G., DiJulio D. D. , Gorska M., Cederkall J., Boutachkov P., Golubev P., Pietri S., Grawe H., Nowacki F., Sieja K., et al., "Coulomb Excitation of Sn-104 and the Strength of the Sn-100 Shell Closure", PHYSICAL REVIEW LETTERS, cilt.110, sa.17, 2013
dc.identifier.issn0031-9007
dc.identifier.othervv_1032021
dc.identifier.otherav_419bf4d0-8cd8-4edc-a64a-c4c187957bc6
dc.identifier.urihttp://hdl.handle.net/20.500.12627/47852
dc.identifier.urihttps://doi.org/10.1103/physrevlett.110.172501
dc.description.abstractA measurement of the reduced transition probability for the excitation of the ground state to the first 2(+) state in Sn-104 has been performed using relativistic Coulomb excitation at GSI. Sn-104 is the lightest isotope in the Sn chain for which this quantity has been measured. The result is a key point in the discussion of the evolution of nuclear structure in the proximity of the doubly magic nucleus Sn-100. The value B(E2; 0(+) -> 2(+)) = 0.10(4) e(2)b(2) is significantly lower than earlier results for Sn-106 and heavier isotopes. The result is well reproduced by shell model predictions and therefore indicates a robust N = Z = 50 shell closure. DOI: 10.1103/PhysRevLett.110.172501
dc.language.isoeng
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.titleCoulomb Excitation of Sn-104 and the Strength of the Sn-100 Shell Closure
dc.typeMakale
dc.relation.journalPHYSICAL REVIEW LETTERS
dc.contributor.departmentTechnical University of Darmstadt , ,
dc.identifier.volume110
dc.identifier.issue17
dc.contributor.firstauthorID208762


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