How elements up to 118 were reached and how to go beyond
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 wi...
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doaj-84fd50cc28d74e578a441493904de4072021-08-02T05:29:11ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011630001510.1051/epjconf/201716300015epjconf_fusion2017_00015How elements up to 118 were reached and how to go beyondDüllmann Christoph E.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.https://doi.org/10.1051/epjconf/201716300015 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Düllmann Christoph E. |
spellingShingle |
Düllmann Christoph E. How elements up to 118 were reached and how to go beyond EPJ Web of Conferences |
author_facet |
Düllmann Christoph E. |
author_sort |
Düllmann Christoph E. |
title |
How elements up to 118 were reached and how to go beyond |
title_short |
How elements up to 118 were reached and how to go beyond |
title_full |
How elements up to 118 were reached and how to go beyond |
title_fullStr |
How elements up to 118 were reached and how to go beyond |
title_full_unstemmed |
How elements up to 118 were reached and how to go beyond |
title_sort |
how elements up to 118 were reached and how to go beyond |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2017-01-01 |
description |
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. |
url |
https://doi.org/10.1051/epjconf/201716300015 |
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AT dullmannchristophe howelementsupto118werereachedandhowtogobeyond |
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