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dc.contributor.authorLotay, G.
dc.contributor.authorDoherty, D. T.
dc.contributor.authorJanssens, R. V. F.
dc.contributor.authorSeweryniak, D.
dc.contributor.authorAlbers, H. M.
dc.contributor.authorAlmaraz-Calderon, S.
dc.contributor.authorCarpenter, M. P.
dc.contributor.authorChampagne, A. E.
dc.contributor.authorChiara, C. J.
dc.contributor.authorHoffman, C. R.
dc.contributor.authorIliadis, C.
dc.contributor.authorKankainen, A.
dc.contributor.authorLauritsen, T.
dc.contributor.authorZhu, S.
dc.date.accessioned2022-06-22T11:44:48Z
dc.date.available2022-06-22T11:44:48Z
dc.date.issued2022
dc.identifier.citationLotay, G., Doherty, D. T., Janssens, R. V. F., Seweryniak, D., Albers, H. M., Almaraz-Calderon, S., Carpenter, M. P., Champagne, A. E., Chiara, C. J., Hoffman, C. R., Iliadis, C., Kankainen, A., Lauritsen, T., & Zhu, S. (2022). Revised decay properties of the key 93-keV resonance in the 25Mg(p,γ) reaction and its influence on the MgAl cycle in astrophysical environments. <i>Physical Review C</i>, <i>105</i>(4), Article L042801. <a href="https://doi.org/10.1103/PhysRevC.105.L042801" target="_blank">https://doi.org/10.1103/PhysRevC.105.L042801</a>
dc.identifier.otherCONVID_147090236
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/81985
dc.description.abstractThe γ-decay properties of an excited state in 26Al at 6398.3(8) keV have been reexamined using the 11B+16O fusion-evaporation reaction. This level represents a key 93.1(8)-keV resonance in the 25Mg+p system and its relative branching to the 26Al ground state, f0, has been determined to be 0.76±0.03 (stat.) ±0.10 (syst.). This is a significantly higher value than the most recent evaluation and implies a considerable increase in the production of cosmic γ rays from 26Al radioactivity.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.titleRevised decay properties of the key 93-keV resonance in the 25Mg(p,γ) reaction and its influence on the MgAl cycle in astrophysical environments
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-202206223590
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.numberinseries4
dc.relation.volume105
dc.type.versionpublishedVersion
dc.rights.copyright© 2022 American Physical Society (APS)
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.subject.ysoastrofysiikka
dc.subject.ysoydinfysiikka
dc.subject.ysomagnesium
dc.subject.ysoalumiini
dc.subject.ysokosminen säteily
dc.subject.ysogammasäteily
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p20188
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p3518
jyx.subject.urihttp://www.yso.fi/onto/yso/p19563
jyx.subject.urihttp://www.yso.fi/onto/yso/p14258
jyx.subject.urihttp://www.yso.fi/onto/yso/p14248
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.105.L042801
jyx.fundinginformationThis work was supported by the US Department of Energy, Office of Science, Office of Nuclear Physics, under Contract No. DEAC02-06CH11357 and Grants No. DEFG02-94ER40834, No. DEFG02-97ER41041, and No. DEFG02-97ER41033. UK personnel were supported by the Science and Technologies Facilities Council (STFC). This research uses resources of ANL's ATLAS facility, which is a DOE Office of Science User facility.
dc.type.okmA1


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