002112012 001__ 2112012
002112012 003__ SzGeCERN
002112012 005__ 20200515173106.0
002112012 0247_ $$2DOI$$9APS$$a10.1103/PhysRevC.89.054316
002112012 0248_ $$aoai:inspirehep.net:1331909$$pcerncds:CERN$$qINSPIRE:HEP$$qForCDS
002112012 035__ $$9http://inspirehep.net/oai2d$$aoai:inspirehep.net:1331909$$d2015-12-08T12:08:17Z$$h2015-12-09T08:28:43Z$$mmarcxml
002112012 035__ $$9Inspire$$a1331909
002112012 041__ $$aeng
002112012 084__ $$2PACS$$a23.20.En
002112012 084__ $$2PACS$$a21.10.Ky
002112012 084__ $$2PACS$$a21.60.Cs
002112012 084__ $$2PACS$$a27.50.+e
002112012 100__ $$aIllana, A$$uMadrid, Inst. Estructura Materia
002112012 245__ $$aLow-velocity transient-field technique with radioactive ion beams: g factor of the first excited 2$^{+}$ state in $^{72}$Zn
002112012 260__ $$c2014
002112012 300__ $$a11 p
002112012 520__ $$9APS$$aThe g factor of the first excited 2+ state in 72Zn has been measured using the transient-field (TF) technique in combination with Coulomb excitation in inverse kinematics. This experiment presents only the third successful application of the TF method to a short-lived radioactive beam in 10 y, highlighting the intricacies of applying this technique to present and future isotope separator on-line facilities. The significance of the experimental result, g(21+)=+0.47(14), for establishing the structure of the Zn isotopes near N=40 is discussed on the basis of shell-model and beyond-mean-field calculations, the latter accounting for the triaxial degree of freedom, configuration mixing, and particle number and angular momentum projections.
002112012 542__ $$3Publication$$dAmerican Physical Society$$g2014
002112012 65017 $$2INSPIRE$$aNuclear Structure
002112012 65017 $$2SzGeCERN$$aNuclear Physics - Experiment
002112012 690C_ $$aCERN
002112012 690C_ $$aARTICLE
002112012 700__ $$aJungclaus, A$$uMadrid, Inst. Estructura Materia
002112012 700__ $$aOrlandi, R$$uMadrid, Inst. Estructura Materia
002112012 700__ $$aPerea, A$$uMadrid, Inst. Estructura Materia
002112012 700__ $$aBauer, C$$uDarmstadt, Tech. Hochsch.
002112012 700__ $$aBriz, J A$$uMadrid, Inst. Estructura Materia
002112012 700__ $$aEgido, J L$$uMadrid, Autonoma U.
002112012 700__ $$aGernhäuser, R$$uMunich, Tech. U.
002112012 700__ $$aLeske, J$$uDarmstadt, Tech. Hochsch.
002112012 700__ $$aMücher, D$$uMunich, Tech. U.
002112012 700__ $$aPakarinen, J$$uCERN
002112012 700__ $$aPietralla, N$$uDarmstadt, Tech. Hochsch.
002112012 700__ $$aRajabali, M$$uKU Leuven, Dept. Phys. Astron.
002112012 700__ $$aRodríguez, T R$$uDarmstadt, Tech. Hochsch.
002112012 700__ $$aSeiler, D$$uMunich, Tech. U.
002112012 700__ $$aStahl, C$$uDarmstadt, Tech. Hochsch.
002112012 700__ $$aVoulot, D$$uCERN
002112012 700__ $$aWenander, F$$uCERN
002112012 700__ $$aBlazhev, A$$uCologne U.
002112012 700__ $$aDe Witte, H$$uKU Leuven, Dept. Phys. Astron.
002112012 700__ $$aReiter, P$$uCologne U.
002112012 700__ $$aSeidlitz, M$$uCologne U.
002112012 700__ $$aSiebeck, B$$uCologne U.
002112012 700__ $$aVermeulen, M J$$uYork U., England
002112012 700__ $$aWarr, N$$uCologne U.
002112012 773__ $$c054316$$n5$$pPhys. Rev. C$$v89$$y2014
002112012 916__ $$sn$$w201601
002112012 960__ $$a13
002112012 980__ $$aARTICLE