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Spectroscopic factor and proton formation probability for the d3/2 proton emitter 151mLu

dc.contributor.authorWang, F.
dc.contributor.authorSun, B.H.
dc.contributor.authorLiu, Z.
dc.contributor.authorPage, R.D.
dc.contributor.authorQi, C.
dc.contributor.authorScholey, Catherine
dc.contributor.authorAshley, S.F.
dc.contributor.authorBianco, L.
dc.contributor.authorCullen, I.J.
dc.contributor.authorDarby, I.G.
dc.contributor.authorEeckhaudt, Sarah
dc.contributor.authorGarnsworthy, A.B.
dc.contributor.authorGelletly, W.
dc.contributor.authorGomez-Hornillos, M.B.
dc.contributor.authorGrahn, Tuomas
dc.contributor.authorGreenlees, Paul
dc.contributor.authorJenkins, D.G.
dc.contributor.authorJones, G.A.
dc.contributor.authorJones, P.
dc.contributor.authorJoss, D.T.
dc.contributor.authorJulin, Rauno
dc.contributor.authorJuutinen, Sakari
dc.contributor.authorKetelhut, Steffen
dc.contributor.authorKhan, S.
dc.contributor.authorKishada, A.
dc.contributor.authorLeino, Matti
dc.contributor.authorNiikura, M.
dc.contributor.authorNyman, M.
dc.contributor.authorPakarinen, J.
dc.contributor.authorPietri, S.
dc.contributor.authorPodolyak, Z.
dc.contributor.authorRahkila, Panu
dc.contributor.authorRigby, S.
dc.contributor.authorSarén, Jan
dc.contributor.authorShizuma, T.
dc.contributor.authorSorri, Juha
dc.contributor.authorSteer, S.
dc.contributor.authorThomson, J.
dc.contributor.authorThompson, N.J.
dc.contributor.authorUusitalo, Juha
dc.contributor.authorWalker, P.M.
dc.contributor.authorWilliams, S.
dc.contributor.authorZhang, H.F.
dc.contributor.authorZhang, W.Q.
dc.contributor.authorZhu, L.H.
dc.date.accessioned2017-05-08T10:14:53Z
dc.date.available2017-05-08T10:14:53Z
dc.date.issued2017
dc.identifier.citationWang, F., Sun, B.H., Liu, Z., Page, R.D., Qi, C., Scholey, C., Ashley, S.F., Bianco, L., Cullen, I.J., Darby, I.G., Eeckhaudt, S., Garnsworthy, A.B., Gelletly, W., Gomez-Hornillos, M.B., Grahn, T., Greenlees, P., Jenkins, D.G., Jones, G.A., Jones, P., . . . Zhu, L.H. (2017). Spectroscopic factor and proton formation probability for the d3/2 proton emitter 151mLu. <i>Physics Letters B</i>, <i>770</i>, 83-87. <a href="https://doi.org/10.1016/j.physletb.2017.04.034" target="_blank">https://doi.org/10.1016/j.physletb.2017.04.034</a>
dc.identifier.otherCONVID_26965193
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/53826
dc.description.abstractThe quenching of the experimental spectroscopic factor for proton emission from the short-lived d3/2d3/2 isomeric state in 151mLu was a long-standing problem. In the present work, proton emission from this isomer has been reinvestigated in an experiment at the Accelerator Laboratory of the University of Jyväskylä. The proton-decay energy and half-life of this isomer were measured to be 1295(5) keV and 15.4(8) μs, respectively, in agreement with another recent study. These new experimental data can resolve the discrepancy in the spectroscopic factor calculated using the spherical WKB approximation. Using the R-matrix approach it is found that the proton formation probability indicates no significant hindrance for the proton decay of 151mLu.
dc.language.isoeng
dc.publisherNorth-Holland
dc.relation.ispartofseriesPhysics Letters B
dc.subject.otherproton emitter
dc.subject.otherrecoil-decay tagging
dc.subject.otherspectroscopic factor
dc.subject.otherproton formation probability
dc.subject.otherWKB approximation
dc.titleSpectroscopic factor and proton formation probability for the d3/2 proton emitter 151mLu
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-201705042190
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.date.updated2017-05-04T12:15:06Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.format.pagerange83-87
dc.relation.issn0370-2693
dc.relation.numberinseries0
dc.relation.volume770
dc.type.versionpublishedVersion
dc.rights.copyright© 2017 the Authors. Published by Elsevier B.V. This is an open access article distributed under the terms of the Creative Commons Attribution License. Funded by SCOAP3
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.physletb.2017.04.034
dc.type.okmA1


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© 2017 the Authors. Published by Elsevier B.V. This is an open access article distributed under the terms of the Creative Commons Attribution License. Funded by SCOAP3
Ellei muuten mainita, aineiston lisenssi on © 2017 the Authors. Published by Elsevier B.V. This is an open access article distributed under the terms of the Creative Commons Attribution License. Funded by SCOAP3
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