PI-ASTERISK MOLECULAR-ORBITAL CROSSING A(2)(CHI) B(1)(PSI) IN 1,10-PHENANTHROLINE DERIVATIVES - AB-INITIO CALCULATIONS AND EPR/ENDOR STUDIES OF THE 4,7-DIAZA-1,10-PHENANTHROLINE RADICAL-ANION AND ITS M(CO)(4) COMPLEXES (M=CR, MO, W)/
S. Ernst et al., PI-ASTERISK MOLECULAR-ORBITAL CROSSING A(2)(CHI) B(1)(PSI) IN 1,10-PHENANTHROLINE DERIVATIVES - AB-INITIO CALCULATIONS AND EPR/ENDOR STUDIES OF THE 4,7-DIAZA-1,10-PHENANTHROLINE RADICAL-ANION AND ITS M(CO)(4) COMPLEXES (M=CR, MO, W)/, Inorganic chemistry, 35(5), 1996, pp. 1295-1300
Ab initio, semiempirical, and HMO perturbation calculations were emplo
yed to assess the relative positioning of the closely situated low-lyi
ng unoccupied pi MOs a(2)(chi) and b(1)(psi) in 1,10-phenanthroline (
phen) and its 3,4,7,8-tetramethyl (tmphen) and four symmetrical diaza
derivatives (n,m-dap). Compared to a(2)(chi), the b(1)(psi) pi MO is d
istinguished by markedly higher MO coefficients at the chelating nitro
gen pi centers in 1,10-positions; eventually, a higher Coulomb integra
l value at those positions will thus always favor the lowering of b(1)
beyond a(2). Using the Coulomb integral parameter at the chelating 1,
10-nitrogen pi centers as the HMO perturbation variable, the crossing
of both energy levels in terms of decreasing preference for the a(2)(c
hi) over the b(1)(psi) orbital as the lowest unoccupied MO follows the
sequence 5,6-dap > 2,9-dap > 4,7-dap, phen > 3,8-dap. The calculation
s reveal a(2)(chi) as the LUMO in 5,6-dap for all reasonable perturbat
ion parameters, in agreement with previous observations for ruthenium(
II) complexes which reveal a discrepancy between the lowest-lying ''re
dox pi orbital'' (a(2)) and the ''optical pi* MO'' (b(1)) to which th
e most intense low-energy MLCT transition occurs. According to the HMO
calculations, the situation is more ambiguous for the 4,7-dap analogu
e, yet EPR/ENDOR studies clearly show that the one-electron-reduced li
gand and its tetracarbonylmetal(0) complexes (Cr, Mo, W) have the b(1)
(psi) orbital singly occupied. Only ab initio calculations with double
-zeta basis and inclusion of d polarization functions reproduced corre
ctly the experimentally observed orbital ordering for tmphen (a(2) < b
(1)) and for phen and 4,7-dap (b(1) < a(2)).