Excited Electronic States Flashcards

1
Q

What are excited states important for?

A

UV-vis absorption

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2
Q

Why are UV-vis absorption peaks broad?

A

Because of various subsets achievable
(many vibrational energies available for each electronic energy level)

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3
Q

Adiabatic excitation energy

A

Excitation to the ground state of the electronically excited state
The threshold for the energy transition

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4
Q

Vertical excitation energy

A

The change in energy to the peak maximum
Computed by assuming ground-state nuclear positions

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5
Q

Where is Eupper (for delta E) computed at for vertical and adiabatic energy?

A

Ground state geometry for delta E vert.
Excited state geometry for delta E adiab.

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6
Q

When can ordinary methods (for calculating E (excited) used?

A

If excited state has different spin state or different orbital symmetry

Called the delta SCF approach (for SCF-only methods like HF or DFT)

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7
Q

Variational collapse problem

A

If electron is excited to a spin-orbital of the same symmetry it had in the ground state, then the excited orbital tends to optimize back to the ground-state orbital

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8
Q

How is variational collapse problem solved?

A

Matrix diagonalization methods are used, involving a CI matrix

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9
Q

CI Matrix

A

Has elements Eij = integral( Yi* H Yj dT)
where Yi and Yj are electronic states having different occupations but keeping the same ground state optimized orbitals, which give better state energies when diagnonalized

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10
Q

CI Singles Technique

A

(1) HF-SCF ground state orbitals (Y, Yi) obtained

(2) CI matrix elements (Eij’s) computed without re-optimizing orbitals, considering only single excitations (Yj’s)

(3) CI matrix is diagonalized, providing several excited-state energies at that molecular geometry (delta E vert, ground state geometry used). Each excited state represented by a linear combination of Slater determinants (just like ground state is in CISD and MCSCF)

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11
Q

Typical errors (CI singles technique)

A

0.07 eV or 70 kJ/mol
Best for qualitative exploring of excited states

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12
Q

General (more accurate) methods

A

Excited-state MCSCF
Time-dependent DFT

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13
Q

Excited-state MCSCF

A

Two modes:
Optimize orbitals for each excited state individually, great for delta E adiab
Hard to do if variational collapse is a threat

State-averaged opt:
Optimize orbitals for the best (lowest) average of several state energies, algorithm converges, generally more accurate than CI

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14
Q

Time-dependent DFT

A

Uses equations from oscillating electric-field theory to find ‘resonance’ corresponding to excited state energies, accurate for low-lying states

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15
Q

Solvatochromism

A

UV-vis spectral transitions of solutes, often require consideration of solvent effects

delta E is often increased by solvation (solvatochromism), treated by implicit solvation modelling with excited-state computation

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