2001
DOI: 10.1002/1521-3757(20010417)113:8<1465::aid-ange1465>3.0.co;2-j
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Die Renaissance der Edelgaschemie

Karl O. Christe

Abstract: Obwohl stabile Edelgasverbindungen mindestens seit 1902 vorausgesagt worden waren, lieûen erfolglose Syntheseversuche die weit verbreitete Ansicht entstehen, dass sich Edelgase chemisch nicht nur edel, sondern völlig inert verhalten. [1] Diese Einschätzung wurde dogmaartig in fast allen Lehrbüchern vertreten und entmutigte über eine lange Zeit Forscher auf diesem Gebiet zu arbeiten. Dies änderte sich erst 1962, als Bartlett in Kanada [2] die erste stabile Edelgasverbindung, XePtF 6 , entdeckte. Diese Endeckung… Show more

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Cited by 23 publications
(3 citation statements)
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“…Recent attempts to synthesize compounds that contain noble gases have been remarkably successful 13. However, so far no stable compound containing helium has been synthesized, except for structures where helium atoms are physically trapped inside fullerene cages 4.…”
Section: Introductionmentioning
confidence: 99%
“…Recent attempts to synthesize compounds that contain noble gases have been remarkably successful 13. However, so far no stable compound containing helium has been synthesized, except for structures where helium atoms are physically trapped inside fullerene cages 4.…”
Section: Introductionmentioning
confidence: 99%
“…Inzwischen wurden auch Verbindungen des Argons mit kovalenten Ar-Heteroatom-Bindungen bei tiefen Temperaturen im HArF [29] nachgewiesen. Erst 1962 gelang die Synthese stabiler Edelgasverbindungen.…”
Section: Eigenschaftenunclassified
“…The discovery of actinide–noble‐gas bonding adds to the recent renaissance in noble‐gas chemistry,7, 8 including the HArF molecule of Räsänen and co‐workers,9 which is kinetically stable in solid argon, and the [AuXe 4 ] 2+ ion of Seidel and Seppelt,10 which is stable enough to be characterized by X‐ray crystallography. The UNg bonds in the CUO(Ng) n complexes are weak: The UNg binding energy ranges from about 4 kcal mol −1 for Ar to about 7 kcal mol −1 for Xe, values that are at the threshold of what can be called a bond.…”
Section: Infrared Absorptions For Uo2+ In Various Solid Noble‐gas Envmentioning
confidence: 99%