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. 2009 Oct 29;113(43):11685-92.
doi: 10.1021/jp902754p.

Color tuning in short wavelength-sensitive human and mouse visual pigments: ab initio quantum mechanics/molecular mechanics studies

Affiliations

Color tuning in short wavelength-sensitive human and mouse visual pigments: ab initio quantum mechanics/molecular mechanics studies

Ahmet Altun et al. J Phys Chem A. .

Abstract

We have investigated the protonation state and photoabsorption spectrum of Schiff-base (SB) nitrogen bound 11-cis-retinal in human blue and mouse UV cone visual pigments as well as in bovine rhodopsin by hybrid quantum mechanical/molecular mechanical (QM/MM) calculations. We have employed both multireference (MRCISD+Q, MR-SORCI+Q, and MR-DDCI2+Q) and single reference (TD-B3LYP and RI-CC2) QM methods. The calculated ground-state and vertical excitation energies show that UV-sensitive pigments have deprotonated SB nitrogen, while violet-sensitive pigments have protonated SB nitrogen, in agreement with some indirect experimental evidence. A significant blue shift of the absorption maxima of violet-sensitive pigments relative to rhodopsins arises from the increase in bond length alternation of the polyene chain of 11-cis-retinal induced by polarizing fields of these pigments. The main counterion is Glu113 in both violet-sensitive vertebrate pigments and bovine rhodopsin. Neither Glu113 nor the remaining pigment has a significant influence on the first excitation energy of 11-cis-retinal in the UV-sensitive pigments that have deprotonated SB nitrogen. There is no charge transfer between the SB and beta-ionone terminals of 11-cis-retinal in the ground and first excited states.

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Figures

Figure 1
Figure 1
QM models, R1 and R2, and atom numbering of PSBR. SBR corresponds to removing the circled hydrogen (gas phase) or transferring it to Glu113 carboxylic oxygen.
Figure 2
Figure 2
Calculated bond length alternation along the polyene chain of the SB and PSB 11-cis-retinal chromophore for RH, HB, and MUV. Average BLA is also given.
Figure 3
Figure 3
HOMO and LUMO of the SB and PSB 11-cis-retinals calculated at the CASSCF level in the gas phase (labeled as QM-none) and at the CASSCF/AMBER level with RH, HB, and MUV pigment environments. Average BLA is given in parentheses.
Figure 4
Figure 4
B3LYP and B3LYP/MM ground-state energies (kcal/mol) of PSBR relative to SBR [QM model: (a) R2 and (b) R2 + Wat2b] in the gas phase and in RH, HB, and MUV pigment environments at the ONIOM-EE structures optimized with R1.
Figure 5
Figure 5
Some important amino acid sites around SB nitrogen. Coordinates taken from RH.
Figure 6
Figure 6
Amino acids that show strong polarization effect on the S1 excitation energy of HB. PSBR and Lys296 bound covalently to each other are shown in green.

References

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