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Superheavy Element Flerovium (Element 114) Is a Volatile Metal

A. YakushevInstitut für Radiochemie, TU Munich, 85748 Garching, GermanyJ. M. GatesInstitut für Radiochemie, TU Munich, 85748 Garching, GermanyΑ. TürlerInstitut für Radiochemie, TU Munich, 85748 Garching, GermanyM. SchädelGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyCh. E. DüllmannSektion SHE Chemie, Helmholtz Institute Mainz, 55099 Mainz, GermanyD. AckermannGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyLiselotte AnderssonDepartment of Physics, University of Liverpool, L69 7ZE Liverpool, U.KM. BlockGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyW. BrüchleGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyJ. DvořákNuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720-8169, United StatesKlaus EberhardtInstitut für Kernchemie, Johannes Gutenberg University Mainz, 55099 Mainz, GermanyH.G. EsselGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyJ. EvenInstitut für Kernchemie, Johannes Gutenberg University Mainz, 55099 Mainz, GermanyU. ForsbergNuclear physicsA. V. GorshkovInstitut für Radiochemie, TU Munich, 85748 Garching, GermanyR. GraegerInstitut für Radiochemie, TU Munich, 85748 Garching, GermanyΚ. Ε. GregorichNuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720-8169, United StatesW. HartmannGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyR.-D. HerzbergDepartment of Physics, University of Liverpool, L69 7ZE Liverpool, U.KF. P. HeßbergerGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyD. HildInstitut für Kernchemie, Johannes Gutenberg University Mainz, 55099 Mainz, GermanyA. HübnerGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyE. JägerGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyJ. KhuyagbaatarHelmholtz Institute MainzB. KindlerGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyJens Volker KratzInstitut für Kernchemie, Johannes Gutenberg University Mainz, 55099 Mainz, GermanyJ. KrierGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyN. KurzGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyB. LommelGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyLorenz NiewischInstitut für Kernchemie, Johannes Gutenberg University Mainz, 55099 Mainz, GermanyH. NitscheNuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720-8169, United StatesJ. P. OmtvedtDepartment of Chemistry, University of Oslo, 0315 Oslo, NorwayE. ParrDepartment of Physics, University of Liverpool, L69 7ZE Liverpool, U.KZhi QinInstitute of Modern Physics, 730000 Lanzhou, People’s Republic of ChinaD. RudolphNuclear physicsJ. RunkeGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyΒ. SchaustenGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyE. SchimpfGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyA. SemchenkovDepartment of Chemistry, University of Oslo, 0315 Oslo, NorwayJ. SteinerGSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, GermanyP. Thörle-PospiechInstitut für Kernchemie, Johannes Gutenberg University Mainz, 55099 Mainz, GermanyJ. UusitaloDepartment of Physics, University of Jyväskylä, 40014 Jyväskylä, FinlandM. WęgrzeckiInstitute of Electron Technology, 02-668 Warsaw, PolandNorbert WiehlInstitut für Kernchemie, Johannes Gutenberg University Mainz, 55099 Mainz, Germany
Inorganic Chemistryjournal2014en
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The electron shell structure of superheavy elements, i.e., elements with atomic number Z ≥ 104, is influenced by strong relativistic effects caused by the high Z. Early atomic calculations on element 112 (copernicium, Cn) and element 114 (flerovium, Fl) having closed and quasi-closed electron shell configurations of 6d(10)7s(2) and 6d(10)7s(2)7p1/2(2), respectively, predicted them to be noble-gas-like due to very strong relativistic effects on the 7s and 7p1/2 valence orbitals. Recent fully relativistic calculations studying Cn and Fl in different environments suggest them to be less reactive compared to their lighter homologues in the groups, but still exhibiting a metallic character. Experimental gas-solid chromatography studies on Cn have, indeed, revealed a metal-metal bond formation with Au. In contrast to this, for Fl, the formation of a weak bond upon physisorption on a Au surface was inferred from first experiments. Here, we report on a gas-solid chromatography study of the adsorption of Fl on a Au surface. Fl was produced in the nuclear fusion reaction (244)Pu((48)Ca, 3-4n)(288,289)Fl and was isolated in-flight from the primary (48)Ca beam in a physical recoil separator. The adsorption behavior of Fl, its nuclear α-decay product Cn, their lighter homologues in groups 14 and 12, i.e., Pb and Hg, and the noble gas Rn were studied simultaneously by isothermal gas chromatography and thermochromatography. Two Fl atoms were detected. They adsorbed on a Au surface at room temperature in the first, isothermal part, but not as readily as Pb and Hg. The observed adsorption behavior of Fl points to a higher inertness compared to its nearest homologue in the group, Pb. However, the measured lower limit for the adsorption enthalpy of Fl on a Au surface points to the formation of a metal-metal bond of Fl with Au. Fl is the least reactive element in the group, but still a metal.

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