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33645911925
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Calculations with larger basis sets such as 6-31++G**, 6-31++G*, or 6-311++G** could not be completed with GAUSSIAN98 as the largest MO coefficient eventually exceeds the computational threshold of the program. Large coefficients arise for those unoccupied orbitals with strong contributions of diffuse basis functions. These orbitals have Rydberg characteristics and are of highly oscillatory form because of the orthogonality constraint to the manifold of lower lying orbitals.
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Calculations with larger basis sets such as 6-31++G**, 6-31++G*, or 6-311++G** could not be completed with GAUSSIAN98 as the largest MO coefficient eventually exceeds the computational threshold of the program. Large coefficients arise for those unoccupied orbitals with strong contributions of diffuse basis functions. These orbitals have Rydberg characteristics and are of highly oscillatory form because of the orthogonality constraint to the manifold of lower lying orbitals.
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33645913074
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Since the HOMO and LUMO are localized in different parts of the molecule, i.e., in the pyrrolic ring and in the pyrroleninic ring and methine bridge, respectively, the transition moment and, hence, the oscillator strength are large for the HOMO -LUMO transition.
-
Since the HOMO and LUMO are localized in different parts of the molecule, i.e., in the pyrrolic ring and in the pyrroleninic ring and methine bridge, respectively, the transition moment and, hence, the oscillator strength are large for the HOMO -LUMO transition.
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Compared to the B3LYP MOs, the BP86 MOs are raised in energy, however, the shifts are more pronounced for the HOMO -1 and HOMO - 2 compared to the HOMO so that the energy differences between these orbitals are reduced, which in turn may promote mixing of these MOs in the excited states.
-
Compared to the B3LYP MOs, the BP86 MOs are raised in energy, however, the shifts are more pronounced for the HOMO -1 and HOMO - 2 compared to the HOMO so that the energy differences between these orbitals are reduced, which in turn may promote mixing of these MOs in the excited states.
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33645941928
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For the HF/6-31G* ground state geometry HOMO-2 and HOMO-1 are inverted compared to B3LYP, BP86, and CNDO/S calculations based on the B3LYP/6-31G* geometry.
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For the HF/6-31G* ground state geometry HOMO-2 and HOMO-1 are inverted compared to B3LYP, BP86, and CNDO/S calculations based on the B3LYP/6-31G* geometry.
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