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Zeptosecond contact times for element Z=120 synthesis
Albers, H. M. (Corresponding author)GSI* ; Khuyagbaatar, J.GSI*HIM* ; Hinde, D. J. ; Carter, I. P. ; Cook, K. J. ; Dasgupta, M. ; Düllmann, C. E.GSI*HIM* ; Eberhardt, K.HIM* ; Jeung, D. Y. ; Kalkal, S. ; Kindler, B.GSI* ; Lobanov, N. R. ; Lommel, B.GSI* ; Mokry, C.HIM* ; Prasad, E. ; Rafferty, D. C. ; Runke, J.GSI* ; Sekizawa, K. ; Sengupta, C. ; Simenel, C. ; Simpson, E. C. ; Smith, J. F. ; Thörle-Pospiech, P.HIM* ; Trautmann, N.GSI* ; Vo-Phuoc, K. ; Walshe, J. ; Williams, E. ; Yakushev, A.GSI*
2020
North-Holland Publ.
Amsterdam
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Please use a persistent id in citations: doi:10.1016/j.physletb.2020.135626 doi:10.15120/GSI-2020-01314
Note: The authors would like to warmly thank Dr. T. Kibedi and all of the staff at the Heavy Ion Accelerator Facility operated by the Australian National University for their help with accelerator op-erations. We also acknowledge J. Steiner and V. Yakusheva for target preparations. This work was supported by the Australian Research Council via research grants DP140101377, DP160101254 and DP170102318, as well as through the German Academic Exchange Service (DAAD) via funds of the German Federal Ministry of Education and Research (BMBF). We also acknowledge the Aus-tralian Federal Government NCRIS program through the HIA capability for support of accelerator operations. Additionally, H.M. Albers, J. Khuyagbaatar, Ch.E. Düllmann and A. Yakushev would like to express their gratitude to the ANU for hosting them during beamtimes.""hisisanopenaccessarticleundertheCCBYlicense(http://creativecommons.org/licenses/by/4.0/).FundedbySCOAP3.
Contributing Institute(s):
- SHE Chemie (SHC)
- Kernspektroskopie (KSP)
- HIM / Superheavy Elements (MSH)
- Targetlabor (TTL)
Research Program(s):
- 612 - Cosmic Matter in the Laboratory (POF3-612) (POF3-612)
Experiment(s):
- External experiment at external facility/ no experiment at GSI (POF3; other)
Appears in the scientific report
2020
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