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dc.contributor.authorHeylen, H.
dc.contributor.authorBabcock, C.
dc.contributor.authorBillowes, J.
dc.contributor.authorBissell, M.L.
dc.contributor.authorBlaum, K.
dc.contributor.authorCampbell, P.
dc.contributor.authorCheal, B.
dc.contributor.authorRuiz, R.F. Garcia
dc.contributor.authorGeppert, Ch.
dc.contributor.authorGins, W.
dc.contributor.authorKreim, K.
dc.contributor.authorMoore, Iain
dc.contributor.authorNeugart, R.
dc.contributor.authorNeyens, G.
dc.contributor.authorNörtershäuser, W.
dc.contributor.authorPapuga, J.
dc.contributor.authorYordanov, D.T.
dc.date.accessioned2016-07-04T05:32:37Z
dc.date.available2016-07-04T05:32:37Z
dc.date.issued2015
dc.identifier.citationHeylen, H., Babcock, C., Billowes, J., Bissell, M.L., Blaum, K., Campbell, P., Cheal, B., Ruiz, R. G., Geppert, Ch., Gins, W., Kreim, K., Moore, I., Neugart, R., Neyens, G., Nörtershäuser, W., Papuga, J., & Yordanov, D.T. (2015). Collinear Laser Spectroscopy on Neutron-rich Mn Isotopes Approaching N = 40. <i>Acta Physica Polonica B</i>, <i>46</i>(3), 699-702. <a href="https://doi.org/10.5506/APhysPolB.46.699" target="_blank">https://doi.org/10.5506/APhysPolB.46.699</a>
dc.identifier.otherCONVID_24697857
dc.identifier.otherTUTKAID_66095
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/50700
dc.description.abstractWe have studied 51,53−64Mn (Z = 25) via bunched-beam collinear laser spectroscopy at ISOLDE, CERN. Model-independent information on the ground- and isomeric state spins, as well as their g-factors is obtained from the measured hyperfine spectra. The spins are essential for further establishing the level schemes in the mass region, while the g-factors reveal the changing ground state wave functions in the Mn chain approaching N = 40.
dc.language.isoeng
dc.publisherFaculty of Physics, Astronomy and Applied Computer Science, Jagiellonian University
dc.relation.ispartofseriesActa Physica Polonica B
dc.subject.otherneutron-rich isotopes
dc.titleCollinear Laser Spectroscopy on Neutron-rich Mn Isotopes Approaching N = 40
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201607013446
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiainePhysicsen
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2016-07-01T12:15:25Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.format.pagerange699-702
dc.relation.issn0587-4254
dc.relation.numberinseries3
dc.relation.volume46
dc.type.versionpublishedVersion
dc.rights.copyright© the Authors, 2016. This is an open access article distributed under a Creative Commons Attribution 3.0 License. Funded by SCOAP3.
dc.rights.accesslevelopenAccessfi
dc.subject.ysomangaani
jyx.subject.urihttp://www.yso.fi/onto/yso/p1635
dc.rights.urlhttp://creativecommons.org/licenses/by/3.0/
dc.relation.doi10.5506/APhysPolB.46.699
dc.type.okmA1


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© the Authors, 2016. This is an open access article distributed under a Creative Commons Attribution 3.0 License. Funded by SCOAP3.
Ellei muuten mainita, aineiston lisenssi on © the Authors, 2016. This is an open access article distributed under a Creative Commons Attribution 3.0 License. Funded by SCOAP3.