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dc.contributor.authorKirsebom, Oliver S.
dc.contributor.authorCederkäll, Joakim
dc.contributor.authorJenkins, David G.
dc.contributor.authorJoshi, Pankaj
dc.contributor.authorJulin, Rauno
dc.contributor.authorKankainen, Anu
dc.contributor.authorKibédi, Tibor
dc.contributor.authorTengblad, Olof
dc.contributor.authorTrzaska, Wladyslaw
dc.date.accessioned2018-01-15T09:18:22Z
dc.date.available2018-01-15T09:18:22Z
dc.date.issued2017
dc.identifier.citationKirsebom, O. S., Cederkäll, J., Jenkins, D. G., Joshi, P., Julin, R., Kankainen, A., Kibédi, T., Tengblad, O., & Trzaska, W. (2017). Towards an Experimental Determination of the Transition Strength Between the Ground States of 20F and 20Ne. In <i>NIC 2016 : Proceedings of the 14th International Symposium on Nuclei in the Cosmos</i> (Article 021008). Physical Society of Japan. JPS Conference Proceedings, 14. <a href="https://doi.org/10.7566/JPSCP.14.021008" target="_blank">https://doi.org/10.7566/JPSCP.14.021008</a>
dc.identifier.otherCONVID_27829481
dc.identifier.otherTUTKAID_76424
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/56717
dc.description.abstractElectron capture on 20Ne is thought to play a crucial role in the final evolution of electron-degenerate ONe stellar cores. Recent calculations suggest that the capture process is dominated by the second-forbidden transition between the ground states of 20Ne and 20F, making an experimental determination of this transition strength highly desirable. To accomplish this task we are refurbishing an intermediate-image magnetic spectrometer capable of focusing 7 MeV electrons, and designing a scintillator detector surrounded by an active cosmic-ray veto shield, which will serve as an energy-dispersive device at the focal plane.
dc.language.isoeng
dc.publisherPhysical Society of Japan
dc.relation.ispartofNIC 2016 : Proceedings of the 14th International Symposium on Nuclei in the Cosmos
dc.relation.ispartofseriesJPS Conference Proceedings
dc.subject.otherbeta-decay
dc.subject.otherweak-interaction rates
dc.subject.othernuclear experiment
dc.subject.otherstellar evolution
dc.titleTowards an Experimental Determination of the Transition Strength Between the Ground States of 20F and 20Ne
dc.typeconferenceObject
dc.identifier.urnURN:NBN:fi:jyu-201801081102
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/ConferencePaper
dc.date.updated2018-01-08T16:15:19Z
dc.relation.isbn978-4-89027-118-4
dc.type.coarconference paper
dc.description.reviewstatuspeerReviewed
dc.type.versionpublishedVersion
dc.rights.copyright© the Authors, 2017. This is an open access article distributed under the terms of the Creative Commons License.
dc.rights.accesslevelopenAccessfi
dc.relation.conferenceNuclei in the Cosmos
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.7566/JPSCP.14.021008


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© the Authors, 2017. This is an open access article distributed under the terms of the Creative Commons License.
Ellei muuten mainita, aineiston lisenssi on © the Authors, 2017. This is an open access article distributed under the terms of the Creative Commons License.