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dc.contributor.authorVerlinde, M.
dc.contributor.authorKraemer, S.
dc.contributor.authorMoens, J.
dc.contributor.authorChrysalidis, K.
dc.contributor.authorCorreia, J. G.
dc.contributor.authorCottenier, S.
dc.contributor.authorDe Witte, H.
dc.contributor.authorFedorov, D. V.
dc.contributor.authorFedosseev, V. N.
dc.contributor.authorFerrer, R.
dc.contributor.authorFraile, L. M.
dc.contributor.authorGeldhof, S.
dc.contributor.authorGranados, C. A.
dc.contributor.authorLaatiaoui, M.
dc.contributor.authorLima, T. A. L.
dc.contributor.authorLin, P.-C.
dc.contributor.authorManea, V.
dc.contributor.authorMarsh, B. A.
dc.contributor.authorMoore, I.
dc.contributor.authorPereira, L. M. C.
dc.contributor.authorRaeder, S.
dc.contributor.authorVan den Bergh, P.
dc.contributor.authorVan Duppen, P.
dc.contributor.authorVantomme, A.
dc.contributor.authorVerstraelen, E.
dc.contributor.authorWahl, U.
dc.contributor.authorWilkins, S. G.
dc.date.accessioned2019-08-23T11:47:58Z
dc.date.available2019-08-23T11:47:58Z
dc.date.issued2019
dc.identifier.citationVerlinde, M., Kraemer, S., Moens, J., Chrysalidis, K., Correia, J. G., Cottenier, S., De Witte, H., Fedorov, D. V., Fedosseev, V. N., Ferrer, R., Fraile, L. M., Geldhof, S., Granados, C. A., Laatiaoui, M., Lima, T. A. L., Lin, P.-C., Manea, V., Marsh, B. A., Moore, I., . . . Wilkins, S. G. (2019). Alternative approach to populate and study the 229Th nuclear clock isomer. <i>Physical Review C</i>, <i>100</i>(2), Article 024315. <a href="https://doi.org/10.1103/PhysRevC.100.024315" target="_blank">https://doi.org/10.1103/PhysRevC.100.024315</a>
dc.identifier.otherCONVID_32296273
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/65291
dc.description.abstractA new approach to observe the radiative decay of the 229Th nuclear isomer, and to determine its energy and radiative lifetime, is presented. Situated at a uniquely low excitation energy, this nuclear state might be a key ingredient for the development of a nuclear clock or a nuclear laser and, the search for time variations of fundamental constants like the fine structure constant. The isomer’s γ decay towards the ground state will be studied with a high-resolution vacuum ultraviolet (VUV) spectrometer after its production by the β decay of 229Ac. The novel production method presents a number of advantages asserting its competitive nature with respect to the commonly used 233U α-decay recoil source. In this paper, a feasibility analysis of this new concept, and an experimental investigation of its key ingredients, using a pure 229Ac ion beam produced at the ISOLDE radioactive beam facility, is reported.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.rightsCC BY 4.0
dc.subject.otherbeta decay
dc.subject.otherisomer decays
dc.subject.othernuclear structure and decays
dc.titleAlternative approach to populate and study the 229Th nuclear clock isomer
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201908233891
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries2
dc.relation.volume100
dc.type.versionpublishedVersion
dc.rights.copyright© The Authors, 2019
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber654002
dc.relation.grantnumber654002
dc.relation.projectidinfo:eu-repo/grantAgreement/EC/H2020/654002/EU//
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevC.100.024315
dc.relation.funderEuroopan komissiofi
dc.relation.funderEuropean Commissionen
jyx.fundingprogramResearch infrastructures, H2020fi
jyx.fundingprogramResearch infrastructures, H2020en
jyx.fundinginformationThis work has received funding from Research Foundation Flanders (FWO, Belgium), from the Excellence of Science program (EOS, FWO-FNRS, Belgium), by GOA/2015/010 (BOF KU Leuven), by the Interuniversity Attraction Poles Program initiated by the Belgian Science Policy Office (BriX network P7/12), from the European Union’s Horizon 2020 research and innovation program under Grants Agreement No. 654002 (ENSAR) and No. 824096 (RADIATE), from the European Research Council under the European Union’s Seventh Framework Program (ERC-2011-AdG291561-HELIOS), from the Spanish MINECO via Project No. FPA-2015-65035-P and from the FCT-Portugal, Project No. CERN-FIS-PAR-0005-2017. M.V. is supported by an FWO grant (Aspirant - 1121820N).
dc.type.okmA1


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