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⁵³Mn and ⁶⁰Fe in iron meteoritesNew data, model calculations

dc.contributor.authorLeya, I
dc.contributor.authorDavid, Jean-Christophe
dc.contributor.authorFaestermann, T.
dc.contributor.authorFroehlich, Michaela
dc.contributor.authorKivel, N
dc.contributor.authorKoll, Dominik
dc.contributor.authorKorschinek, Gunther
dc.contributor.authorMcIntyre, Sarah
dc.contributor.authorMerchel, Silke
dc.contributor.authorPavetich, Stefan
dc.contributor.authorRugel, Georg
dc.contributor.authorSchumann, D.
dc.contributor.authorSmith, T
dc.contributor.authorWallner, Anton
dc.date.accessioned2022-03-01T03:26:33Z
dc.date.available2022-03-01T03:26:33Z
dc.date.issued2020
dc.date.updated2022-07-24T08:16:51Z
dc.description.abstractWe measured specific activities of the long-lived cosmogenic radionuclides 60Fe in 28 iron meteorites and 53Mn in 41 iron meteorites. Accelerator mass spectrometry was applied at the 14MV Heavy Ion Accelerator Facility at ANU Canberra for all samples except for two which were measured at the Maier-Leibnitz Laboratory, Munich. For the large iron meteorite Twannberg (IIG), we measured six samples for 53Mn. This work doubles the number of existing individual 60Fe data and quadruples the number of iron meteorites studied for 60Fe. We also significantly extended the entire 53Mn database for iron meteorites. The 53Mn data for the iron meteorite Twannberg vary by more than a factor of 30, indicating a significant shielding dependency. In addition, we performed new model calculations for the production of 60Fe and 53Mn in iron meteorites. While the new model is based on the same particle spectra as the earlier model, we no longer use experimental cross sections but instead use cross sections that were calculated using the latest version of the nuclear model code INCL. The new model predictions differ substantially from results obtained with the previous model. Predictions for the 60Fe activity concentrations are about a factor of 2 higher, for 53Mn, they are ~30% lower, compared to the earlier model, which gives now a better agreement with the experimental data. The Meteoritical Society, 2020.
dc.description.sponsorshipThis work has been supported by the Swiss National Science Foundation (SNF 200021-159562) by the Australian Research Council, project numbers DP140100136, DP180100495, and DP180100496 and by the Group of Eight Australia–Germany Joint Research Co-operation Scheme.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn1086-9379en_AU
dc.identifier.urihttp://hdl.handle.net/1885/261594
dc.language.isoen_AUen_AU
dc.provenanceThis is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.en_AU
dc.publisherUniversity of Arkansas
dc.relationhttp://purl.org/au-research/grants/arc/DP140100136
dc.relationhttp://purl.org/au-research/grants/arc/DP180100495
dc.relationhttp://purl.org/au-research/grants/arc/DP180100496
dc.rights© 2020 The Authors. Meteoritics & Planetary Science published by Wiley Periodicals LLC on behalf of The Meteoritical Society (MET)
dc.rights.licenseCreative Commons Attribution Licenseen_AU
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_AU
dc.sourceMeteoritics and Planetary Science
dc.title⁵³Mn and ⁶⁰Fe in iron meteoritesNew data, model calculations
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue4en_AU
local.bibliographicCitation.lastpage831en_AU
local.bibliographicCitation.startpage818en_AU
local.contributor.affiliationLeya, I, University of Bernen_AU
local.contributor.affiliationDavid, Jean-Christophe, CEA-Saclayen_AU
local.contributor.affiliationFaestermann, T., Technical University of Munichen_AU
local.contributor.affiliationFroehlich, Michaela, College of Science, ANUen_AU
local.contributor.affiliationKivel, N, Paul Scherrer Institut, Villigen PSIen_AU
local.contributor.affiliationKoll, Dominik, College of Science, ANUen_AU
local.contributor.affiliationKorschinek, Gunther, Technical University of Munichen_AU
local.contributor.affiliationMcIntyre, Sarah, College of Science, ANUen_AU
local.contributor.affiliationMerchel, Silke, Helmholtz-Zentrum Dresden-Rossendorf (HZDR)en_AU
local.contributor.affiliationPavetich, Stefan, College of Science, ANUen_AU
local.contributor.affiliationRugel, Georg, Helmholtz-Zentrum Dresden-Rossendorf (HZDR)en_AU
local.contributor.affiliationSchumann, D., Paul Scherrer Instituteen_AU
local.contributor.affiliationSmith, T, University of Bernen_AU
local.contributor.affiliationWallner, Anton, College of Science, ANUen_AU
local.contributor.authoruidFroehlich, Michaela, u5217967en_AU
local.contributor.authoruidKoll, Dominik, u6818102en_AU
local.contributor.authoruidMcIntyre, Sarah, u5189889en_AU
local.contributor.authoruidPavetich, Stefan, u1010673en_AU
local.contributor.authoruidWallner, Anton, u5124538en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor029904 - Synchrotrons; Accelerators; Instruments and Techniquesen_AU
local.identifier.absfor020202 - Nuclear Physicsen_AU
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciencesen_AU
local.identifier.ariespublicationa383154xPUB11398en_AU
local.identifier.citationvolume55en_AU
local.identifier.doi10.1111/maps.13466en_AU
local.identifier.scopusID2-s2.0-85082602752
local.identifier.thomsonIDWOS:000522537600001
local.publisher.urlhttps://www.wiley.com/en-gben_AU
local.type.statusPublished Versionen_AU

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