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How elements up to 118 were reached and how to go beyond

dc.contributor.authorDüllmann, Christoph
dc.coverage.spatialXi'an, China
dc.date.accessioned2023-11-17T01:00:50Z
dc.date.available2023-11-17T01:00:50Z
dc.date.createdJuly 10-13, 2017
dc.date.issued2017
dc.date.updated2022-08-07T08:17:51Z
dc.description.abstractThe new superheavy elements with Z=113, 115, 117, and 118 were recently accepted into the periodic table and have been named. Elements with Z≥112 are predominantly produced in 48Ca-induced fusion reactions on actinide targets. This pathway is exhausted at Z=118 due to the lack of target materials with sufficiently high proton number to reach elements with Z≥119. Search experiments for yet heavier elements were performed at GSI Darmstadt and FLNR Dubna. The reactions 50Ti + 249Bk, which leads to Z=119, as well as 64Ni + 238U, 58Fe + 244Pu, 54Cr + 248Cm, and 50Ti + 249Cf, leading to Z=120, have been studied. Despite a total duration of these experiments of more than one year, neither succeeded in the identification of a new element. To obtain improved guidance for better-informed search experiments, nuclear reaction studies appear necessary and have recently started. Also technical advances will be an important pillar to this end. At GSI, work towards a new continuous-wave linear accelerator is ongoing and is briefly described.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.isbn9780996452700en_AU
dc.identifier.urihttp://hdl.handle.net/1885/306379
dc.language.isoen_AUen_AU
dc.provenanceThis is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).en_AU
dc.publisherEDP Sciencesen_AU
dc.relation.ispartofseries2017 20th International Conference on Information Fusionen_AU
dc.rights© The Authors, published by EDP Sciences.en_AU
dc.rights.licenseCreative Commons Attribution 4.0 International Licenseen_AU
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_AU
dc.sourceEPJ Web of Conferencesen_AU
dc.titleHow elements up to 118 were reached and how to go beyonden_AU
dc.typeConference paperen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.lastpage5en_AU
local.bibliographicCitation.startpage1en_AU
local.contributor.affiliationDüllmann, Christoph, College of Science, ANUen_AU
local.contributor.authoruidDüllmann, Christoph, u1010483en_AU
local.description.notesImported from ARIESen_AU
local.description.refereedYes
local.identifier.absfor510601 - Nuclear physicsen_AU
local.identifier.absseo280120 - Expanding knowledge in the physical sciencesen_AU
local.identifier.ariespublicationa383154xPUB9081en_AU
local.identifier.doi10.1051/epjconf/201716300015en_AU
local.identifier.scopusID2-s2.0-85036671887
local.identifier.thomsonIDWOS:000463850900015
local.publisher.urlhttps://www.epj-conferences.org/en_AU
local.type.statusPublished Versionen_AU

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