Alternative approach to populate and study the 229Th nuclear clock isomer
dc.contributor.author | Verlinde, M. | |
dc.contributor.author | Kraemer, S. | |
dc.contributor.author | Moens, J. | |
dc.contributor.author | Chrysalidis, K. | |
dc.contributor.author | Correia, J. G. | |
dc.contributor.author | Cottenier, S. | |
dc.contributor.author | De Witte, H. | |
dc.contributor.author | Fedorov, D. V. | |
dc.contributor.author | Fedosseev, V. N. | |
dc.contributor.author | Ferrer, R. | |
dc.contributor.author | Fraile, L. M. | |
dc.contributor.author | Geldhof, S. | |
dc.contributor.author | Granados, C. A. | |
dc.contributor.author | Laatiaoui, M. | |
dc.contributor.author | Lima, T. A. L. | |
dc.contributor.author | Lin, P.-C. | |
dc.contributor.author | Manea, V. | |
dc.contributor.author | Marsh, B. A. | |
dc.contributor.author | Moore, I. | |
dc.contributor.author | Pereira, L. M. C. | |
dc.contributor.author | Raeder, S. | |
dc.contributor.author | Van den Bergh, P. | |
dc.contributor.author | Van Duppen, P. | |
dc.contributor.author | Vantomme, A. | |
dc.contributor.author | Verstraelen, E. | |
dc.contributor.author | Wahl, U. | |
dc.contributor.author | Wilkins, S. G. | |
dc.date.accessioned | 2019-08-23T11:47:58Z | |
dc.date.available | 2019-08-23T11:47:58Z | |
dc.date.issued | 2019 | |
dc.identifier.citation | Verlinde, 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.other | CONVID_32296273 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/65291 | |
dc.description.abstract | A 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.mimetype | application/pdf | |
dc.language | eng | |
dc.language.iso | eng | |
dc.publisher | American Physical Society | |
dc.relation.ispartofseries | Physical Review C | |
dc.rights | CC BY 4.0 | |
dc.subject.other | beta decay | |
dc.subject.other | isomer decays | |
dc.subject.other | nuclear structure and decays | |
dc.title | Alternative approach to populate and study the 229Th nuclear clock isomer | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-201908233891 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.contributor.oppiaine | Kiihdytinlaboratorio | fi |
dc.contributor.oppiaine | Accelerator Laboratory | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2469-9985 | |
dc.relation.numberinseries | 2 | |
dc.relation.volume | 100 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © The Authors, 2019 | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.relation.grantnumber | 654002 | |
dc.relation.grantnumber | 654002 | |
dc.relation.projectid | info:eu-repo/grantAgreement/EC/H2020/654002/EU// | |
dc.subject.yso | ydinfysiikka | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1103/PhysRevC.100.024315 | |
dc.relation.funder | Euroopan komissio | fi |
dc.relation.funder | European Commission | en |
jyx.fundingprogram | Research infrastructures, H2020 | fi |
jyx.fundingprogram | Research infrastructures, H2020 | en |
jyx.fundinginformation | This 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.okm | A1 |