How elements up to 118 were reached and how to go beyond
| dc.contributor.author | Düllmann, Christoph | |
| dc.coverage.spatial | Xi'an, China | |
| dc.date.accessioned | 2023-11-17T01:00:50Z | |
| dc.date.available | 2023-11-17T01:00:50Z | |
| dc.date.created | July 10-13, 2017 | |
| dc.date.issued | 2017 | |
| dc.date.updated | 2022-08-07T08:17:51Z | |
| dc.description.abstract | The 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.mimetype | application/pdf | en_AU |
| dc.identifier.isbn | 9780996452700 | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/306379 | |
| dc.language.iso | en_AU | en_AU |
| dc.provenance | This 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.publisher | EDP Sciences | en_AU |
| dc.relation.ispartofseries | 2017 20th International Conference on Information Fusion | en_AU |
| dc.rights | © The Authors, published by EDP Sciences. | en_AU |
| dc.rights.license | Creative Commons Attribution 4.0 International License | en_AU |
| dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | en_AU |
| dc.source | EPJ Web of Conferences | en_AU |
| dc.title | How elements up to 118 were reached and how to go beyond | en_AU |
| dc.type | Conference paper | en_AU |
| dcterms.accessRights | Open Access | en_AU |
| local.bibliographicCitation.lastpage | 5 | en_AU |
| local.bibliographicCitation.startpage | 1 | en_AU |
| local.contributor.affiliation | Düllmann, Christoph, College of Science, ANU | en_AU |
| local.contributor.authoruid | Düllmann, Christoph, u1010483 | en_AU |
| local.description.notes | Imported from ARIES | en_AU |
| local.description.refereed | Yes | |
| local.identifier.absfor | 510601 - Nuclear physics | en_AU |
| local.identifier.absseo | 280120 - Expanding knowledge in the physical sciences | en_AU |
| local.identifier.ariespublication | a383154xPUB9081 | en_AU |
| local.identifier.doi | 10.1051/epjconf/201716300015 | en_AU |
| local.identifier.scopusID | 2-s2.0-85036671887 | |
| local.identifier.thomsonID | WOS:000463850900015 | |
| local.publisher.url | https://www.epj-conferences.org/ | en_AU |
| local.type.status | Published Version | en_AU |
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