In the following, a short survey of the theory of optical spectra is given. For a detailed discussion, we refer to refs (3, 18, 30, and 31). The theory is based on a standard Hamiltonian Hppc for the pigment–protein complex that describes the pigments as coupled two-level systems interacting with vibrational degrees of freedom of the pigments and the protein.3 It is composed of three parts, Hppc = Hex + Hex–vib + Hvib. The exciton part Hex includes the site energies Em of the pigments, defined as the optical transition energies at the equilibrium position of nuclei in the electronic ground state, and the excitation energy transfer couplings Vmn. The exciton–vibrational part Hex–vib describes the modulation of site energies and excitonic couplings by the vibrations. In the spirit of a NMA,17 it is assumed that the site energies and excitonic couplings depend linearly on the displacements of the vibrational coordinates from their equilibrium values. The vibrational part Hvib describes uncoupled harmonic oscillators.
For the calculation of optical spectra, the Hamiltonian of the PPC is transformed to the basis of delocalized exciton states |M⟩ which are given as linear combinations of local excited states |m⟩.
The exciton coefficients cm(M) and
excitation energies
, are
obtained from the solution of the
eigenvalue problem
of the exciton Hamiltonian Hex. The
absolute square of the exciton coefficient cm(M) describes the probability
that the mth pigment is excited when the PPC is in
the Mth exciton state. The exciton–vibrational
Hamiltonian Hex–vib contains diagonal
elements, which lead to vibrational sidebands and off-diagonal elements,
which cause lifetime broadening of the optical lines.18
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