Versuche zur Synthese ferrocendiylverbrückter Di(amido)-Chelatkomplexe von Gruppe-4-Metallen

Die Polymerisation von α-Olefinen mit Derivaten von Gruppe-4-Metallocenen ist von großem technologischen Interesse. In den letzten Jahren hat sich bei der Suche nach metallocenalternativen Präkatalysatoren u.a. aufgrund der theoretischen Arbeiten von Ziegler gezeigt, dass Di(amido)-Chelatkomplexe mit Gruppe-4-Metallen vielversprechende Spezies für die α-Olefinpolymerisation darstellen. Im Rahmen der vorliegenden Arbeit sollten die stereoelektronischen Eigenschaften solcher Komplexe durch Arylgruppen mit sterisch anspruchsvollen Alkylsubstituenten beeinflusst werden. Weitere interessante Eigenschaften sollten durch die die Stickstoffatome verbrückende Ferroceneinheit erzielt werden, da diese als molekulares Kugellager und redoxaktive Schaltereinheit fungieren kann. Die Di(arylamino)ferrocenligandvorstufen Fe[(C5H4)NHPh]2, Fe[(C5H4)NH(2,6-C6H3Me2)]2 und Fe[(C5H4)NH(2,4,6-i-Pr3C6H2)]2 konnten durch Hartwig-Buchwald-artige Kreuzkupplung von 1,1´-Diaminoferrocen mit dem jeweiligen Arylbromid erhalten werden. Dagegen misslangen über diese Syntheseroute zahlreiche Versuche zur Synthese von Derivaten mit Substituenten in meta-Position des Arylringes. Die Darstellung der Titan- und Zirkoniumchelatkomplexe gelang durch Metathesereaktion der Di(arylamino)ferrocene mit M(NMe2)4 bzw. M(CH2Ph)4 (M = Ti, Zr), die unter Eliminierung von 2 Äquivalenten HNMe2 bzw. Toluol ablaufen. Dabei zeigte sich, dass bei sterisch anspruchsvollen Di(arylamino)ferrocenligandsystemen keine Metathesereaktion mit Ti(NMe2)4 möglich ist, was auch für analoge Reaktionen mit Ti(CH2Ph)4 zu erwarten ist. Ganz anders sind dagegen die Verhältnisse in der Zirkoniumchemie. Hier konnten durch Umsetzung von Fe[(C5H4)NH(2,4,6-i-Pr3C6H2)]2 mit Zr(NMe2)4 bzw. Zr(CH2Ph)4 die Komplexe [{Fe[C5H4(NC6H2-2,4,6-i-Pr3)]2}Zr(NMe2)2] und [{Fe[C5H4(NC6H2-2,4,6-i-Pr3)]2}Zr(CH2Ph)2] dargestellt werden. Hier findet sich eine senkrechte Anordnung der Arylringe zur Chelatringebene, die die nach Ziegler günstige Orbitalüberlappung ermöglicht, die zu einer besonders hohen katalytischen Aktivität dieser Komplexe in der Ethylenpolymerisation führen sollte. Nach üblicher Aktivierung zeigen diese Komplexe jedoch nur niedrige Aktivitäten in der Ethylenpolymerisation. Ob strukturelle Parameter für dieses Ergebnis verantwortlich sind, oder sogar Defizite im Ziegler-Modell vorliegen, sollte Gegenstand zukünftiger Untersuchungen sein.

Dirac-Fock-Slater calculations for the elements Z = 100, fermium, to Z = 173

Listed here for the elements Z = 100, fermium, to Z = 173 are energy eigenvalues and total energies found from relativistic Dirac-Fock-Slater calculations. The effect of high ionization on the energy eigenvalues is presented for two exarnples. The use of these tables in connection with the energy levels of superheavy elements and molecular orbital (MO) x-ray transitions in superheavy quasiatoms, is discussed. In addition, abrief comparison between the results of the Dirac-Fock-Slater and Dirac-Fock calculations is given.

Reduced L_1 level width and Coster-Kronig yields by relaxation and continuum interactions in atomic zinc

Calculations of the level width \gamma( L_1) and the f_12 and f_13 Coster-Kronig yields for atomic zinc have been performed with Dirac-Fock wave functions. For \gamma(L_1), a large deviation between theory and evaluated data exists. We include the incomplete orthogonality of the electron orbitals as well as the interchannel interaction of the decaying states. Orbital relaxation reduces the total rates in all groups of the electron-emission spectrum by about 10-20 %. Different, however, is the effect of the continuum interaction. The L_1-L_23X Coster-Kronig part of the spectrum is definitely reduced in its intensity, whereas the MM and MN spectra are slightly enhanced. This results in a reduction of Coster-Kronig yields, where for medium and heavy elements considerable discrepancies have been found in comparison to relativistic theory. Briefly, we discuss the consequences of our calculations for heavier elements.

Relativistic Dirac-Fock-Slater program to calculate potential-energy curves for diatomic molecules

A LCAO-MO (linear combination of atomic orbitals - molecular orbitals) relativistic Dirac-Fock-Slater program is presented, which allows one to calculate accurate total energies for diatomic molecules. Numerical atomic Dirac-Fock-Slater wave functions are used as basis functions. All integrations as well as the solution of the Poisson equation are done fully numerical, with a relative accuracy of 10{^-5} - 10{^-6}. The details of the method as well as first results are presented here.

Ground state correlation energy of the Be-sequence for Z = 4-20 in MCDF approximation

The ground state (J = 0) electronic correlation energy of the 4-electron Be-sequence is calculated in the Multi-Configuration Dirac-Fock approximation for Z = 4-20. The 4 electrons were distributed over the configurations arising from the 1s, 2s, 2p, 3s, 3p and 3d orbitals. Theoretical values obtained here are in good agreement with experimental correlation energies.

Ionization potentials and radii of atoms and ions of element 104 (unnilquadium) and of hafnium (2+) derived from multiconfiguration Dirac-Fock calculations

Multiconfiguration relativistic Dirac-Fock (MCDF) values have been computed for the first four ionization potentials (IPs) of element 104 (unnilquadium) and of the other group 4 elements (Ti, Zr, and Hf). Factors were calculated that allowed correction of the systematic errors between the MCDF IPs and the experimental IPs. Single "experimental" IPs evaluated in eV (to ± 0.1 eV) for element 104 are: [104(0),6.5]; [104( 1 + ),14.8]; [104(2 + ),23.8]; [104(3 + ),31.9]. Multiple experimental IPs evaluated in eV for element 104 are: [(0-2+ ),21.2±0.2]; [(0-3+ ),45.1 ±0.2]; [(0-4+ ),76.8±0.3].Our MCDF results track 11 of the 12 experimental single IPs studied for group 4 atoms and ions. The exception is Hf( 2 + ). We submit our calculated IP of 22.4 ± 0.2 eV as much more accurate than the value of 23.3 eV derived from experiment.

Test for basis-set errors in relativistic Dirac-Fock-Slater calculations with a numerical AO-DFS-basis

A fully relativistic four-component Dirac-Fock-Slater program for diatomics, with numerically given AO's as basis functions is presented. We discuss the problem of the errors due to the finite basis-set, and due to the influence of the negative energy solutions of the Dirac Hamiltonian. The negative continuum contributions are found to be very small.

Solution of the time dependent Dirac-Fock-Slater equation for many-electron collisions systems using a time window method

We present a new scheme to solve the time dependent Dirac-Fock-Slater equation (TDDFS) for heavy many electron ion-atom collision systems. Up to now time independent self consistent molecular orbitals have been used to expand the time dependent wavefunction and rather complicated potential coupling matrix elements have been neglected. Our idea is to minimize the potential coupling by using the time dependent electronic density to generate molecular basis functions. We present the first results for 16 MeV S{^16+} on Ar.

Ionization potentials and radii of atoms and ions of element 105 (unnilpentium) and ions of tantalum derived from multiconfiguration Dirac-Fock calculations

Multiconfiguration relativistic Dirac-Fock (MCDF) values were calculated for the first five ionization potentials of element 105 (unnilpentium) and of the other group 5b elements (V, Nb, and Ta). Some of these ionization potentials in electron volts (eV) with uncertainties are: 105(0), 7.4±0.4; 105(1 +), 16.3 ±0.2; 105(2 +), 24.3 ± 0.2; 105(3 + ), 34.9 ± 0.5; and 105(4 + ), 44.9 ± 0.1. Ionization potentials for Ta(1+), Ta(2 +), and Ta(3 + ) were also calculated. Accurate experimental values for these ionization potentials are not available. Ionic radii are presented for the 2+, 3+, 4 +, and 5+ ions of element 105 and for the + 2 ions of vanadium and niobium. These radii for vanadium and niobium are not available elsewhere. The ionization potentials and ionic radii obtained are used to determine some standard electrode potentials for element 105. Born-Haber cycles and a form of the Born equation for the Gibbs free energy of hydration of ions were used to calculate the standard electrode potentials.