2003
DOI: 10.1002/zaac.200300226
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Metal‐Xenon Complexes

Abstract: Long after the first isolation of a xenon compound in 1962 the first compounds with metal‐xenon bonds are prepared. The metal atoms are so far Au and Hg. The most stable metal xenon compounds decompose under loss of xenon slightly above room temperature. They can only exist if solvents and counter ions are weaker bases than atomic xenon. Solvents and counter ions used so far are HF, (SbF6)—, and (Sb2F11)—.

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Cited by 47 publications
(24 citation statements)
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“…Among metal hexafluoroantimonates coordinated with HF the compound [Hg(HF)](SbF 6 ) 2 should be mentioned [17] [18]. The distance Au-F(HF) is 213.5(3) pm [19] and is comparable with Au-F(Sb) distance of 212.6(3) pm.…”
Section: Synthesis and Structures Of Other Coordination Compounds Witmentioning
confidence: 97%
“…Among metal hexafluoroantimonates coordinated with HF the compound [Hg(HF)](SbF 6 ) 2 should be mentioned [17] [18]. The distance Au-F(HF) is 213.5(3) pm [19] and is comparable with Au-F(Sb) distance of 212.6(3) pm.…”
Section: Synthesis and Structures Of Other Coordination Compounds Witmentioning
confidence: 97%
“…+ , [5,6] [Ag(S 8 ) 2 ] + , [1] [Au(Xe) 4 ] + , [14] [AgA C H T U N G T R E N N U N G (P 3 N 3 Cl 6 ) n ] + , [3] [AgA C H T U N G T R E N N U N G (C 2 H 2 ) n ] + , [15] {[AgA C H T U N G T R E N N U N G {Cp*Fe(P 5 )} 2 ] + ) 1 , [4] or [AgA C H T U N G T R E N N U N G (C 2 H 4 ) n ]…”
Section: A C H T U N G T R E N N U N G (P 4 S 3 ) N ] + (N = 1-3) Andmentioning
confidence: 99%
“…Hence, Xe in complex 3 is shielded in the region of 719-1,044 ppm compared with an unbound Xe atom, and the known chemical-shift range for 129 Xe has been increased by Ϸ800 ppm (or nearly 10%) to Ϸ8,400 ppm (32). Smaller shifts to high field (up to 50 ppm) have been observed for gaseous Xe trapped in Cu ϩ -or Ag ϩ -exchanged NaX or NaY zeolites (35), for which it is postulated that the increased shielding is caused by back donation from the d 10 Cu or Ag centers that occurs in transient interactions with the Xe. Theoretical calculations on Cu ϩ -Xe and Ag ϩ -Xe species predict these upfield shifts and show their source to be a mixing of the filled metal d shell with the 5p, 4p, and 3p orbitals on the Xe (36).…”
Section: Nmr Studies At Low Temperature In Lxementioning
confidence: 99%
“…The great majority of this noble gas chemistry has resulted from interaction of Kr and Xe with electron-deficient, highly oxidizing reagents to create compounds containing the noble gas in positive oxidation states (6). More recently, the occurrence of atomic Xe as a discrete ligand in a selection of cationic gold and mercury inorganic complexes has been demonstrated, with the bonding occurring through a lone pair of electrons on the Xe (7)(8)(9)(10). Theoretical studies had previously predicted high stability of such cationic gold complexes (11).…”
mentioning
confidence: 99%