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* Dipartimento di Chimica, Università di Roma "La Sapienza", 00185 Rome, Italy;
Dipartimento di Chimica, Ingegneria Chimica e Materiali, Università de l'Aquila, 67010 l'Aquila, Italy;
Dipartimento di Chimica-Fisica, Università di Padova, 35131 Padua, Italy; and
Dipartimento di Scienze e Tecnologie Chimiche, Università di Roma "Tor Vergata", 00133 Rome, Italy
Correspondence: Address reprint requests to Dr. A. Amadei, Tel.: +39-06-72594905; Fax: +39-0672594328; E-mail: andrea.amadei{at}uniroma2.it.
| ABSTRACT |
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| INTRODUCTION |
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| METHODS |
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2 of both histidines and the magnesium atom of the Chl a is 4 Å). A water molecule, which is on one side hydrogen-bonded to these residues, provides the fifth coordination site.
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1 and N
2, respectively. All the crystallographic water molecules close to the subsystem considered were included. The simulation was performed in the NVT ensemble, using the GROMACS simulation software packages (van der Spoel et al., 1995
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SCF), and the method based on the Koopmans' theorem, i.e., the energy of the highest energy electron in the molecular orbitals. To estimate the binding energy, Deq, of the water molecule to the magnesium atom of the chlorophyll ring, HF/SCF calculations with a double
-basis set including first polarization functions (3-21G*) (Pietro et al., 1982
132 kJ/mol allowed us to consider, in the 300 K MD simulation, the water molecule as covalently bound to the Chl a. All these ground-state calculations were done using GAMESS US package (Schmidt et al., 1993
Mixed calculations
To obtain the electronic properties of the Chl a into the protein environment during the simulation, we modeled the protein perturbation as an electric field, changing according to the protein's motions and acting on the Chl a system. The electric potential felt by the Chl a molecule can be expanded around the chromophore geometrical center. If a first order expansion of the electric potential is used, for an uncharged chromophore, the protein's perturbation reduces simply to the effect of a homogeneous electric field interacting with the dipole operator (we disregard the magnetic interactions). Such a perturbing electric field was assumed to be independent of the chromophore; hence any polarization of the atomic electronic density due to the chromophore interaction and excitation was neglected. It would be possible, in principle, to include these higher order effects, but in this paper where we deal with a large and complex system we disregard them, i.e., we assume that at least the chromophore excitation energy is basically independent of these effects. The electric field acting on the chromophore was approximated using the GROMOS87 atomic charges. Note that the interaction between the Chl a and bulk SPC water molecules was not included in the calculations, as their effect on the electric field acting on the chromophore, calculated as large as 110% of the protein electric field, was negligible during the simulation. By the use of the PMM method, given the unperturbed energies, dipoles, and transition dipoles, it is possible to calculate the electronic properties of the perturbed system during the simulation, i.e., for each stored configuration of the MD simulation. The method is based on the matrix expression of the time-independent Schroedinger's equation, that is for a perturbed system:
![]() | (1) |
, ci is the ith eigenvector of the perturbed Hamiltonian matrix
,
is the corresponding Hamiltonian eigenvalue,
is the unperturbed Hamiltonian matrix, and
is the perturbation energy matrix. By expressing the Hamiltonian matrix and its eigenvectors in the basis set defined by the unperturbed Hamiltonian matrix eigenvectors, the generic element l,l' of the Hamiltonian matrix is:
![]() | (2) |
l0 is the lth eigenfunction of the unperturbed Hamiltonian operator,
the corresponding energy eigenvalue,
l,l' the Kroenecker's delta, and
the perturbation energy operator. To obtain the eigenvectors and eigenvalues, and hence any needed property, of the perturbed Hamiltonian matrix, we have only to diagonalize the matrix
. For a system interacting with an external electric field, we can express in general the perturbation operator in Eq.2 in terms of the electric potential V (Spezia et al., 2002
![]() | (3) |
![]() |
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![]() | (4) |
![]() | (5) |
![]() | (6) |
![]() | (7) |
![]() | (8) |
![]() | (9) |
![]() | (10) |
From the last equations, it is evident that a second order expansion of the electric potential, able to describe electric fields up to linear behavior over the molecular size, requires the knowledge of the total charge and the unperturbed dipoles and quadrupoles. Higher order expansions can be in principle worked out in the same way but would require information on higher order multipoles, which are typically very difficult to obtain. Moreover, it is rather unusual that an applied electric field, at least evaluated from the Coulombic part of a usual molecular force field, is beyond the linear approximation over a molecular size. This was actually verified in our simulation, where the electric field, due to the Coulombic interactions, was for most of the configurations obtained by the MD simulation virtually constant over the chlorophyll. However, it is worth noting that such approximation does not hold in general for short-range atomic interactions, typically described in MD force field by the Lennard-Jones potential, which may modify significantly the electric field over a single atom. However, these interactions can be assumed, as far as the valence excited states are considered, to be basically independent of the Hamiltonian eigenstates, providing only an additive constant for the diagonal elements of the perturbation matrix. Hence the excitation energy may be well evaluated using only the Coulombic interactions. In the present paper, we used the Born-Oppenheimer approximation to describe the chromophore, i.e., its unperturbed eigenfunctions are purely electronic, and we disregard any perturbation effect beyond the dipolar term in Eq. 8. The previous equations could be in principle exact and general only if infinite dimensional matrices and vectors are involved. However, if we focus our attention on the ground and first excited states, the use of a finite dimensional matrix can provide an accurate approximation (Aschi et al., 2001
). To build up the matrix
defined by Eq. 9, we need the chromophore unperturbed eigenstates, i.e., the unperturbed energies of a finite set of eigenstates, and the corresponding electric dipoles and the transition electric dipoles. Provided that the chromophore remains basically rigid during the simulation, it is possible to use the unperturbed states calculated at CIS level of theory at a given reference configuration, and build for each stored configuration of the trajectory a perturbed matrix to be diagonalized. Note that the use of the PMM method is possible also in the presence of flexible molecules, although in this case the unperturbed eigenstates should be calculated over a set of different configurations. From each diagonalization of the perturbed matrix, constructed on the unperturbed ground and first 10 excited states, i.e., an 11 x 11 matrix, we obtained the perturbed eigenvalues and eigenvectors. The difference between the ground and the first excited eigenvalues gives us the energy of the first (vertical) electronic transition and therefore the corresponding wavelength.
| RESULTS AND DISCUSSION |
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-helices, as usual in protein dynamics (Ceruso et al., 1999
atoms are shown. As expected, the first eigenvalues provide a large part of the overall fluctuations. The motion was projected on the first and second eigenvectors separately as well as on the plane of the first two eigenvectors (Fig. 5). The atomic motions associated with the first two eigenvectors, described in Fig. 6, correspond to a motion of the loop connecting the two helices N4 (from residue 56 to 70) and N5 (from residue 82 to 97) and a tilting of the helices N2 (from residue 22 to 34), N3 (from residue 37 to 53), and N7 (from residue 119 to 125). The loop motion is the largest in both eigenvectors. In the first eigenvector, the helix N2 has a lager amplitude motion than the helix N7 and the helix N3, whereas in the second eigenvector, the helix N3 has a larger displacement than the helix N2 and the helix N7 has only a small displacement. Note that such large amplitude motions are not probably associated to any unfolding process or instability of the monomer used, as already shown by the stability of the secondary structures and radius of gyration. Panels A and B of the Fig. 5 show the typical large amplitude and slow motion of essential coordinates (Amadei et al., 1993
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SCF IP and the Koopmans' theorem IP (5.47 eV and 6.15 eV, respectively) are close to the values reported for Bchl a by Sakuma et al. (1997)
), calculated from the energy difference between the first excited and ground perturbed eigenvalues, was obtained for each configuration of the trajectory. In Fig. 7 A, the transition wavelengths calculated in the simulation (solid line) and the corresponding unperturbed one (dashed line) are reported. The effect of the environment is a blue shift with an average absorption wavelength of 604 nm with a standard deviation of 8 nm. In Fig. 7 B, we report the unnormalized distribution of the perturbed
calculated in the equilibrated trajectory. Note that the distribution is not symmetric and hence the maximum, located between 610 and 611 nm, does not coincide with the average
. Moreover, this dispersion of the
-values is due only to the flexibility of the surrounding protein, as the inhomogeneous and vibronic contributions to the spectral broadening are not taken into account in this kind of calculations. To evaluate the role played respectively by the protein and Per chromophores in the perturbation and transition energy fluctuation (water molecules are too far and DGDG is a basically apolar molecule), we calculated the effect of the field produced only by the Pers. The average absorption wavelength, and its standard deviation and error, were calculated as a function of the position along the first eigenvector. In Fig. 8 (panel A), we show the absorption (average)
due to the overall electric field (solid line) and due to the Per electric field (dashed line) as a function of the position along the first eigenvector. In panel B, we also show the corresponding
standard deviation, provided by the other coordinates fluctuations. It is evident that only in a well-defined range of the protein first eigenvector coordinate, the Per chromophores have a relevant influence on the absorption spectrum. Consistently, the standard deviation of the wavelength due to the Per electric field shows the same behavior. From a more detailed analysis of the MD simulation, we noted that the above behavior corresponds to a translational motion of the three Pers (Per1, Per2, Per3). The absorption wavelength due to the overall electric field is clearly dependent on the first eigenvector coordinate whereas its standard deviation seems to be rather constant. This shows that the essential motions in the protein are important in modulating the photochemical activity of a chromophore. It is worth noting that the average absorption wavelengths evaluated at each position along the first eigenvector are likely to be not fully converged as the motion of the other essential coordinates is characterized by a slow diffusive kinetics (Amadei et al., 1999a
, we also evaluated the average
fixing the first two eigenvectors positions. This is likely to provide better converged
-values as they are averaged on faster relaxing coordinates. The results are reported in Fig. 9, which shows again a clear dependence of the average
on the first two eigenvectors coordinates.
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| CONCLUSIONS |
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| ACKNOWLEDGEMENTS |
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We acknowledge the Italian Ministry for University and Scientific and Technological Research (PRIN "Structure and Dynamics of Redox Proteins" 2001) and CNR Agenzia2000 for financial support.
Submitted on July 24, 2002; accepted for publication December 17, 2002.
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