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The high nuclear charges of the heaviest elements influence their electronic structure and hence their chemical properties. [1][2][3][4][5] The experimental results so far obtained for the heaviest chemically investigated elements reveal that seaborgium, [6,7] bohrium, [8] and hassium [9] behave as typical representatives of the corresponding Group 6, 7, and 8 of the periodic table. Apparently, relativistic effects do not introduce a perceptible destabilization of the highest oxidation states of these elements in the chemical environments they have been studied in. An even stronger increase of relativistic effects is predicted for the transactinides of Groups 12-18. [1][2][3] Element 112, a representative of Group 12 of the periodic table, has a predicted closed-shell electronic ground-state configuration of [Rn]5f 14 6d 10 7s 2 , rendering this element one of the key elements regarding relativistic effects in the electronic structure. [3,5,10] Recently, our gas chromatography experiments with only two observed atoms of element 112 revealed evidence for a metallic adsorption interaction with the stationary gold surface. [11] Here we present new experimental results with an increased number of observed atoms that confirm these observations and improve their statistical significance. From the complete data set, thermochemical and physical data are deduced for element 112 and compared to the corresponding properties of its homologues in Group 12: Zn, Cd, and Hg. The increased stabilization of the atomic state of element 112 reveals a further enhancement of the relativistic effects with increasing atomic number Z in Group 12.For element 112 a noble-metallic character was predicted from empirical extrapolations. [12,13] Relativistic atomic calculations revealed a contraction of the spherical 7s orbitals, leading to the prediction of an enhanced stability of the elemental atomic state for element 112. Accordingly, a noblegas-like behavior was postulated. [14] Modern calculation methods confirmed a stronger binding of the 7s orbitals. [3] However, the spin-orbit coupling of the 6d orbitals is predicted to lead to an electronic ground state configuration with a 6d 5/2 orbital that is similar energetically and spatially to the 7s orbital, indicating that element 112 could be a noble transition metal [5,15] or even a semiconductor. [16] Based on these strongly differing predictions, it is decisive for experimentalists to be able to distinguish in chemical experiments whether element 112 behaves more as a noble metal or as a noble gas. Therefore, investigation of gas adsorption properties of element 112 on metal surfaces has been suggested. [17] In such studies the energy content of the adsorption bond between element 112 and the metallic stationary phase, the standard adsorption enthalpy at zero surface coverage (DH ads Au ), is determined. This quantity differentiates between metal-bond formation and weak van der Waals physisorption interaction. The semiempirical macroscopic adsorption model based on the Miedema approach ...
The high nuclear charges of the heaviest elements influence their electronic structure and hence their chemical properties. [1][2][3][4][5] The experimental results so far obtained for the heaviest chemically investigated elements reveal that seaborgium, [6,7] bohrium, [8] and hassium [9] behave as typical representatives of the corresponding Group 6, 7, and 8 of the periodic table. Apparently, relativistic effects do not introduce a perceptible destabilization of the highest oxidation states of these elements in the chemical environments they have been studied in. An even stronger increase of relativistic effects is predicted for the transactinides of Groups 12-18. [1][2][3] Element 112, a representative of Group 12 of the periodic table, has a predicted closed-shell electronic ground-state configuration of [Rn]5f 14 6d 10 7s 2 , rendering this element one of the key elements regarding relativistic effects in the electronic structure. [3,5,10] Recently, our gas chromatography experiments with only two observed atoms of element 112 revealed evidence for a metallic adsorption interaction with the stationary gold surface. [11] Here we present new experimental results with an increased number of observed atoms that confirm these observations and improve their statistical significance. From the complete data set, thermochemical and physical data are deduced for element 112 and compared to the corresponding properties of its homologues in Group 12: Zn, Cd, and Hg. The increased stabilization of the atomic state of element 112 reveals a further enhancement of the relativistic effects with increasing atomic number Z in Group 12.For element 112 a noble-metallic character was predicted from empirical extrapolations. [12,13] Relativistic atomic calculations revealed a contraction of the spherical 7s orbitals, leading to the prediction of an enhanced stability of the elemental atomic state for element 112. Accordingly, a noblegas-like behavior was postulated. [14] Modern calculation methods confirmed a stronger binding of the 7s orbitals. [3] However, the spin-orbit coupling of the 6d orbitals is predicted to lead to an electronic ground state configuration with a 6d 5/2 orbital that is similar energetically and spatially to the 7s orbital, indicating that element 112 could be a noble transition metal [5,15] or even a semiconductor. [16] Based on these strongly differing predictions, it is decisive for experimentalists to be able to distinguish in chemical experiments whether element 112 behaves more as a noble metal or as a noble gas. Therefore, investigation of gas adsorption properties of element 112 on metal surfaces has been suggested. [17] In such studies the energy content of the adsorption bond between element 112 and the metallic stationary phase, the standard adsorption enthalpy at zero surface coverage (DH ads Au ), is determined. This quantity differentiates between metal-bond formation and weak van der Waals physisorption interaction. The semiempirical macroscopic adsorption model based on the Miedema approach ...
Jedes Atom zählt: Neue Daten zum adsorptionschromatographischen Verhalten einzelner Atome des Elements 112 bestätigen dessen metallischen Charakter in der Wechselwirkung mit einer Goldoberfläche ähnlich zu seinen Homologen Zn, Cd und Hg. Den experimentellen Resultaten zufolge hat Element 112 eine deutlich höhere Flüchtigkeit als die leichteren Homologen der Gruppe 12 des Periodensystems.
The chemical nature and aggregate state of superheavy copernicium (Cn) have been subject of speculation for many years.W hile strong relativistic effects render Cn chemically inert, which led Pitzer to suggest an oble-gas-like behavior in 1975, Eichler and co-workers in 2008 reported substantial interactions with ag old surface in atom-at-a-time experiments,s uggesting am etallic character and as olid aggregate state.H erein, we explore the physicochemical properties of Cn by means of first-principles free-energy calculations,w hichc onfirm Pitzerso riginal hypothesis:W ith predicted melting and boiling points of 283 AE 11 Ka nd 340 AE 10 K, Cn is indeed avolatile liquid and exhibits adensity very similar to that of mercury.H owever,i ns tark contrast to mercury and the lighter Group 12 metals,wefind bulk Cn to be bound by dispersion and to exhibit alarge band gap of 6.4 eV, which is consistent with an oble-gas-like character.T his nongroup-conforming behavior is eventually traced backtostrong scalar-relativistic effects,a nd in the non-relativistic limit, Cn appears as ac ommon Group 12 metal.Supportinginformation and the ORCID identification number(s) for the author(s) of this article can be found under: https://doi.org/10.
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