2019
DOI: 10.1021/acs.jpca.9b01947
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Solid Oganesson via a Many-Body Interaction Expansion Based on Relativistic Coupled-Cluster Theory and from Plane-Wave Relativistic Density Functional Theory

Abstract: Many-body potentials up to fourth order are constructed using nonrelativistic, scalar-relativistic, and relativistic coupled-cluster theory to accurately describe the interaction between superheavy oganesson atoms. The obtained distance-dependent energy values were fitted to extended two-body Lennard-Jones and three-body Axilrod− Teller−Muto potentials, with the fourth-order term treated through a classical long-range Drude dipole interaction model. From these interaction potentials, spectroscopic constants fo… Show more

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Cited by 28 publications
(65 citation statements)
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“…In this respect, Cn is much more similar to the noble gas Rn (band gap 7.1 eV) than to its lighter congeners, and even more similar to Rn than oganesson (Og) as the actual Group 18 member of the seventh period (band gap 1.5 eV, see Figure c) . Together with the smaller cohesive energy of Cn (0.38 eV vs. 0.45 eV), this suggests that Cn is more noble‐gas‐like than Og.…”
Section: Resultsmentioning
confidence: 70%
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“…In this respect, Cn is much more similar to the noble gas Rn (band gap 7.1 eV) than to its lighter congeners, and even more similar to Rn than oganesson (Og) as the actual Group 18 member of the seventh period (band gap 1.5 eV, see Figure c) . Together with the smaller cohesive energy of Cn (0.38 eV vs. 0.45 eV), this suggests that Cn is more noble‐gas‐like than Og.…”
Section: Resultsmentioning
confidence: 70%
“…However, the relatively strong interaction with the gold surface may as well be due to strong dispersion interactions. Also considering the distinctly larger cohesive energy of the superheavy “noble gas” oganesson (Og) of −0.45 eV, Cn appears to lean towards the noble gases rather than towards its lighter metallic congeners.…”
Section: Figurementioning
confidence: 99%
“…Experimental structures were used for Ne to Xe, and for Rn and Og high‐level computational structures were employed (cf. Table SII, Supporting Information) . The core region was modeled using the projector‐augmented wave (PAW) approach of Joubert and Kresse with the potentials for He to Rn taken from the VASP library .…”
Section: Figurementioning
confidence: 99%
“…[16],w ew ill focus here on the evolution of DE, O g ,a nd E g with increasing atomic number.B ys imple extrapolation based on Figure 2, one would anticipate aneardegeneracyofthe three at about 7eVfor Rn, and values just above 4eVf or Og, placing the latter at the borderline between insulators and semiconductors.H owever,s uch as imple extrapolation disregards that the close resemblance between atomic and bulk properties may break in the heavier noble gases which are larger,m ore polarizable and thus interact more strongly.This is reflected in the cohesive energy (E coh ,b inding energy of the solid per atom, red line in Figure 2), which increases continuously to 0.23 eV for Rn, and jumps to 0.45 eV for Og. [19,20] Hence,O gi sb yf ar the least noble of the noble gases,l ess noble even than superheavy copernicium (Cn, E coh = 0.38 eV) [22][23][24] and thus presumably also as olid at ambient conditions.A ccordingly,e xcitons in solid Og and perhaps also Rn may exhibit adelocalization and stabilization compared to the respective excited states of the atoms,w hich could cause O g and E g to fall well below DE, breaking with the periodic trends and rendering Og as emiconductor.…”
mentioning
confidence: 99%
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