Journal Article

GSI-2021-00080

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Khuyagbaatar, J. (Corresponding author)GSI*HIM* ; Yakushev, A.GSI* ; Düllmann, C. E.GSI*HIM* ; Ackermann, D.GSI* ; Andersson, L.-L.GSI*HIM* ; Asai, M. ; Block, M.GSI* ; Boll, R. A. ; Brand, H.GSI* ; Cox, D. M. ; Dasgupta, M. ; Derkx, X.HIM* ; Di Nitto, A. ; Eberhardt, K.HIM* ; Even, J.GSI*HIM* ; Evers, M. ; Fahlander, C. ; Forsberg, U. ; Gates, J. M. ; Gharibyan, N. ; Golubev, P. ; Gregorich, K. E. ; Hamilton, J. H. ; Hartmann, W.GSI* ; Herzberg, R.-D. ; Heßberger, F. P.GSI*HIM* ; Hinde, D. J. ; Hoffmann, J.GSI* ; Hollinger, R.GSI* ; Hübner, A.GSI* ; Jäger, E.GSI* ; Kindler, B.GSI* ; Kratz, J. V. ; Krier, J.GSI* ; Kurz, N.GSI* ; Laatiaoui, M.GSI* ; Lahiri, S. ; Lang, R.GSI* ; Lommel, B.GSI* ; Maiti, M. ; Miernik, K. ; Minami, S.GSI* ; Mistry, A. K.GSI* ; Mokry, C.GSI*HIM* ; Nitsche, H. ; Omtvedt, J. P. ; Pang, G. K. ; Papadakis, P. ; Renisch, D. ; Roberto, J. B. ; Rudolph, D. ; Runke, J.GSI* ; Rykaczewski, K. P. ; Sarmiento, L. G. ; Schädel, M.GSI* ; Schausten, B.GSI* ; Semchenkov, A. ; Shaughnessy, D. A. ; Steinegger, P. ; Steiner, J.GSI* ; Tereshatov, E. E. ; Thörle-Pospiech, P.GSI*HIM* ; Tinschert, K.GSI* ; Torres De Heidenreich, T.GSI* ; Trautmann, N.GSI* ; Türler, A. ; Uusitalo, J. ; Wegrzecki, M. ; Wiehl, N.HIM* ; Van Cleve, S. M. ; Yakusheva, V.GSI*HIM*

2020
APS Woodbury, NY

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Please use a persistent id in citations: doi:10.1103/PhysRevC.102.064602

Note: We are grateful for GSI’s Penning ion source and UNI-LAC staff, and the Experimental Electronics department fortheir continuous support of the experiment. This work wasfinancially supported in part by the German BMBF (GrantNo. 05P12UMFNE), the Helmholtz association (Grant No.VH-NG-723), the Helmholtz Institute Mainz, Swedish Re-search Council (Vetenskapsrådet VR Grants No. 2011-5253and No. 2016-3969), the Australian Federal GovernmentARC (Grants No. DP170102318, No. DP170102423, andNo. DP200100601), the US Department of Energy by LLNL(Grant No. DE-AC52-07NA27344), Vanderbilt University(Grant No. DE-FG05-88ER40407), and the Laboratory Di-rected Research and Development Program at LLNL (GrantNo. 11-ERD-011). This work was cosponsored by the Officeof Science, US Department of Energy (DOE), and supportedunder U.S. DOE Grant No. DE-AC05-00OR22725 (ORNL).249Bk material was provided by the U.S. DOE Isotope Pro-gram.

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Contributing Institute(s):

1. HIM / Superheavy Elements (MSH)
2. SHE Chemie (SHC)
3. SHE Physik (SHP)
4. Experimentelektronik (EEL)
5. Ionenquellen (IOS)
6. Ring RF (RRF)
7. Targetlabor (TTL)
8. Kernspektroskopie (KSP)

Research Program(s):

1. 612 - Cosmic Matter in the Laboratory (POF3-612) (POF3-612)

Experiment(s):

1. Experiment at GSI without experiment proposal number ( - ; Facility_outside_beam_time_program )

Appears in the scientific report 2020

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Database coverage:
; Clarivate Analytics Master Journal List ; Current Contents - Electronics and Telecommunications Collection ; Current Contents - Physical, Chemical and Earth Sciences ; Ebsco Academic Search ; Essential Science Indicators ; IF < 5 ; JCR ; SCOPUS ; Science Citation Index Expanded ; Web of Science Core Collection

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