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Biophys J, January 2000, p. 344-353, Vol. 78, No. 1

and
*Faculty of Sciences, Division of Physics and Astronomy and
Institute for Condensed Matter Physics and Spectroscopy, Vrije
Universiteit, 1081 HV Amsterdam, the Netherlands, and
Fakultät für Biologie, Universität
Konstanz, D-78457 Konstanz, Germany
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ABSTRACT |
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Time-resolved fluorescence anisotropy spectroscopy has
been used to study the chlorophyll a (Chl a) to
Chl a excitation energy transfer in the water-soluble
peridinin-chlorophyll a-protein (PCP) of the
dinoflagellate Amphidinium carterae. Monomeric PCP binds
eight peridinins and two Chl a. The trimeric structure of PCP, resolved at 2 Å (Hofmann et al., 1996
, Science.
272:1788-1791), allows accurate calculations of energy transfer times
by use of the Förster equation. The anisotropy decay time
constants of 6.8 ± 0.8 ps (
1) and 350 ± 15 ps (
2) are respectively assigned to intra- and
intermonomeric excitation equilibration times. Using the ratio
1/
2 and the amplitude of the anisotropy,
the best fit of the experimental data is achieved when the
Qy transition dipole moment is rotated by
2-7° with respect to the y axis in the plane of the Chl
a molecule. In contrast to the conclusion of Moog et al.
(1984
, Biochemistry. 23:1564-1571) that the refractive index (n) in the Förster equation should be equal to
that of the solvent, n can be estimated to be 1.6 ± 0.1, which is larger than that of the solvent (water). Based on our
observations we predict that the relatively slow intermonomeric energy
transfer in vivo is overruled by faster energy transfer from a PCP
monomer to, e.g., the light-harvesting a/c complex.
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INTRODUCTION |
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The dinoflagellate Amphidinium
carterae contains a water-soluble peridinin-chlorophyll
a-protein (PCP) that acts as an accessory photosynthetic
light-harvesting pigment-protein complex. The complex transfers its
excitation energy to photosystem II (PSII) (Mimuro et al., 1990
).
However, it is not known whether this transfer is directly to the PSII
antenna complex (Knoetzel and Rensing, 1990
) or via the membrane-bound
light-harvesting complex (LHCa/c) (Hofmann et al., 1996
).
The main light-absorbing pigment of PCP is peridinin, which absorbs in
the 470-550-nm region. Besides peridinin the complex binds chlorophyll
a (Chl a). The pigments are bound to a 30.2-kDa
protein and are organized into two clusters of pigments, each
consisting of four peridinins and one Chl a (see, e.g.,
Carbonera and Giacometti, 1995
). Singlet energy transfer from peridinin
to Chl a occurs with an efficiency close to 100% (Song et
al., 1976
; Koka and Song, 1977
) on a time scale of a few picoseconds
(Bautista et al., 1999
; Akimoto et al., 1996
).
Recently, the crystal structure of PCP was resolved at a resolution of
2.0 Å (Hofmann et al., 1996
), revealing a trimeric organization of the
complex. The protein mainly has an
-helical structure and forms a
cavity in which the two pigment clusters are located (Hofmann et al.,
1996
). The distance between the centers of the two Chl a in
one monomer is 17.4 Å, whereas the distance between two Chl
a bound to different monomers ranges from 40 to 54 Å (Hofmann et al., 1996
). All peridinins are organized in pairs with a
closest distance to each other of 4 Å, and they are in van der Waals
contact with the Chl a. The resolution is high enough to
distinguish the x and y axes of the Chl
a molecules, allowing a definition of the orientation of the
Qy transition dipole moment within the molecular
frame of Chl a in PCP. Therefore, PCP forms an excellent
system for the study of the Chl a to Chl a
excitation energy transfer in a relatively simple pigment-protein
complex and to test whether it can be modeled using the Förster
equation (Förster, 1965
).
A detailed test of the Förster equation was conducted before by
Debreczeny et al. (1995a
,b
) on another pigment-protein complex with a
known crystal structure (Schirmer et al., 1987
; Duerring et al., 1991
),
namely monomeric and trimeric C-phycocyanin (CPC) from
Synechococcus sp. The pigments responsible for light
harvesting in this complex are open-chain tetrapyrrole chromophores
(also called phycocyanobilins). The three pigments bound to each
monomer are relatively far apart; however, in the trimer two pigments bound to different monomers are relatively close. The energy transfer processes in the monomeric and trimeric complexes were studied using
time-resolved polarized fluorescence experiments by Gillbro et al.
(1993)
and Debreczeny et al. (1995a
,b
). It was concluded by Debreczeny
et al. (1995a
,b
, 1993
) that the equilibration rates are in good
correspondence with those that can be calculated using the
Förster equation, with the refractive index (which is an important parameter in this equation) being that of the solvent, in
this case water (n = 1.33). It was argued before by
Moog et al. (1984)
that when the Förster equation is applied to
protein-chromophore complexes, the refractive index of the solvent
should be used.
In the present study we focus on the Chl a to Chl
a excitation energy transfer in PCP, using time-resolved
fluorescence anisotropy spectroscopy. We show that the experimental
equilibration rates and the rates calculated using the Förster
equation are in reasonable agreement when the Chl a
Qy transition dipole moments are oriented along the
molecular y axis. However, we find a better match when these
dipole moments are rotated by 2-7°. In contrast to the conclusion by
Moog et al. (1984)
, in the case of PCP the refractive index in the
Förster equation is larger than the refractive index of the
solvent, which is water, and it is estimated to be 1.60 ± 0.1.
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MATERIALS AND METHODS |
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Sample preparation
PCP was purified according to the method described by Hofmann et
al. (1996)
. Measurements were performed in a buffer containing 25 mM
Tris-HCl (pH 7.5), 3 mM NaN3, and 2 mM KCl.
Absorption and steady-state fluorescence emission spectroscopy
The absorption spectra were recorded on a Cary 219 spectrophotometer, using an optical bandwidth of 1 nm. Steady-state fluorescence emission spectra were recorded using a CCD camera (Chromex Chromcam 1) via a 1/2 m spectrograph (Chromex 500IS). Excitation light was provided by a tungsten-halogen lamp via a band-pass filter at 475 nm with a full width at half-maximum (FWHM) of 15 nm. The fluorescence emission spectra were corrected for the wavelength sensitivity of the detection system.
Time-resolved fluorescence anisotropy
The optical density of the sample was 0.2/cm at the excitation wavelength (660 nm) and 0.6/cm in the absorbance maximum at 670 nm. The sample was kept at room temperature in a spinning cell (light path of 0.22 cm, diameter 10 cm, frequency 15 Hz) refreshing the sample every few shots. The spinning cell was placed at an angle of 45° with respect to the excitation light. Comparison of the OD spectrum of the sample before and after the experiment showed that less than 10% of the absorption was lost after an experiment with a duration of several hours. The spectrum essentially did not change. Two independent series of experiments were performed.
Pulses of 150-200 fs at 660 nm with a FWHM of 7 nm were generated at a 100-kHz repetition rate, using a Ti:sapphire based oscillator (Coherent MIRA), a regenerative amplifier (Coherent REGA), and a double-pass optical parametric amplifier (OPA-9400; Coherent). The intensity was adjusted so that less than 1 photon/20 trimeric complexes was absorbed per laser shot. The polarization of the excitation light was adjusted with a Soleil Babinet compensator.
The fluorescence was detected at a right angle with respect to the
excitation beam through a sheet polarizer, using a Hamamatsu C5680
synchroscan streak camera equipped with a Chromex 250IS spectrograph
(4-nm spectral resolution, 3-ps time response). The streak images were
recorded on a Hamamatsu C4880 CCD camera, which was cooled to
55°C.
Streak images were recorded on two different time scales (200 ps and
2200 ps full range) and over a wavelength range of 315 nm, with the
detection polarizer oriented alternately parallel and perpendicular to
the vertically polarized excitation light. The polarization dependence
of the sensitivity of the apparatus was measured by recording streak
images, using horizontally polarized excitation light, with the
polarizer in the detection branch oriented both horizontally and
vertically, and is expressed in the so-called g factor.
Global analysis
The measurements on both time scales and with both polarizations
were fitted simultaneously, using a global analysis program (van
Stokkum et al., 1994
) for the wavelength region in which no scattering
of the exciting laser light was present. The two independent series of
experiments were fitted separately. Included in the fitting procedure
is the signal that is detected in the back sweep of the streak camera,
which is 6-8 ns after the excitation pulse. The experimentally
determined g factor was introduced into the fitting
procedure. In the model an initial anisotropy of 0.4 is assumed. The
amplitudes of the fitted kinetics are rather sensitive to small
variations in the g factor; however, the variation in the
corresponding time constants is limited. For both data sets we have
estimated the error margins for the amplitudes by examining the
consequences of small variations in the g factor.
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RESULTS |
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Absorption and fluorescence
In Fig. 1 the absorption
(solid line) and fluorescence emission (dashed
line) spectra of PCP at room temperature are shown. The inset
shows the overall absorption spectrum of PCP at room temperature. The
absorption band at 670 nm is due to the Qy band of Chl a and has a FWHM of 14 nm. The absorption in the
450-600-nm region is due to peridinin, and the peak at 430 nm is due
to the Soret band of Chl a. The spectrum is very similar to
the absorption spectra of PCP reported before (Koka and Song, 1977
;
Carbonera et al., 1996
). In the time-resolved fluorescence emission
experiment the sample was excited at 660 nm (thick vertical
line in Fig. 1), and the anisotropy was calculated from the
fluorescence detected between 675 and 700 nm. The anisotropy decay was
independent of the detection wavelength. The absorption and
fluorescence emission spectra shown here were used for the calculation
of the Förster overlap integral (see Appendix 2).
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Time-resolved fluorescence anisotropy
In Fig. 2 the
F
(t) and F
(t)
components (polarization of the detection being parallel and
perpendicular to the vertical polarization of the excitation light,
respectively) of the fluorescence emission spectra are plotted on a
linear-logarithmic time scale for the 200-ps window (Fig. 2
A) and for the 2200-ps time window (Fig. 2 B).
The detection wavelength of these traces was 675 nm. At detection
wavelengths shorter than 675 nm, scattering of the excitation light
contributes at time scales on the order of the instrument response. The
anisotropy was independent of the detection wavelength; therefore the
675-700-nm region was fitted using a global analysis routine (van
Stokkum et al., 1994
). The solid lines in Fig. 2 show the result of a
simultaneous fit of the F
(t) and
F
(t) components in the two time domains. In
the fit procedure the anisotropy at t = 0 was fixed at
0.4. Two decay time constants were needed to fit the decay of the
anisotropy r(t):
|
(1) |
1 and
2
are tentatively interpreted as intra- and intermonomeric equilibration
times, respectively. The error margins are estimated on the basis of
the fits of two independent series of experiments. The estimated error
margin of the amplitude of the fast process (A1)
is 0.24 ± 0.02. The amplitude of the 350 ± 15-ps process
could be estimated very accurately to be 0.05, and the fitted amplitude
of the residual anisotropy is anticorrelated to the fitted amplitude of
the fast process. Therefore, the amplitude of the residual anisotropy
(r
) is 0.11 ± 0.02. On the time scale
of the fastest depolarization process hardly any depolarization due to
the slower process takes place. The anisotropy "after" the fast
depolarization process (r1) can be defined as
r1 = 0.4
A1 = 0.16 ± 0.02.
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Because the experiment is performed in water, one might expect a third
depolarization time constant caused by the rotational motion of the PCP
complex. The rotational depolarization time was reported to be 33 ns
(Koka and Song, 1977
). On the basis of the known size of the complex
one can calculate that the rotational depolarization time (Cantor and
Schimmel, 1980
), is ~48 ns for the PCP trimer and ~16 ns for the
monomer. Addition of an extra component with a depolarization time
constant of 16-48 ns in the global analysis procedure did not lead to
an improvement of the fit, and therefore the rotational depolarization
is negligible.
The isotropic fluorescence decay time constant was estimated to be
~4.2 ns, which is in reasonable agreement with the fluorescence lifetime of 4.6 ns reported by Koka and Song (1977)
.
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DISCUSSION |
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Calculation of Förster energy transfer rates based on the structure of PCP
For the application of the Förster equation two
prerequisites should be fulfilled: 1) the dipole interaction approach
should be justified and 2) the excitonic coupling between the pigments should be weak. In the case of PCP, the center-to-center distance between the interacting pigments is at least 17 Å, significantly larger than the conjugated part of the porphyrin, so that the dipole-dipole approximation is justified. The second constraint quantitatively implies that the coupling between the pigments is
smaller than the homogeneous width of the absorption bands. The Chl
a Qy band of PCP has a width of 300 cm
1, and the coupling between two Chl a in a
PCP monomer is on the order of 10 cm
1 (Kleima, 1999
), so
the second condition is also fulfilled.
On the basis of the crystal structure of PCP, the excitation energy
transfer rates can now be calculated using the Förster equation
(Förster, 1965
):
|
(2) |
|
(3) |
1) is the rate of
transfer from donor (D) to acceptor (A),
is
an orientation factor which is given below, n is the
refractive index, R is the distance between the centers of
the interacting pigments in nm, and krD is
the radiative rate of the donor molecule (ps
1). The
integral reflects the overlap between the fluorescence spectrum of the
donor normalized to area unity and the absorption spectrum of the
acceptor scaled to the value of the extinction coefficient
(M
1 · cm
1) in the absorption
maximum, both on a frequency scale (cm
1). The orientation
factor
is given by
|
(4) |
1 and
2 are the
normalized transition dipole moment vectors and
12 is the normalized vector between the
centers of pigments 1 (donor) and 2 (acceptor). The center of the Chl a molecule is taken to be the center of gravity of the four
nitrogen atoms in the molecular structure of Chl a (see Fig.
3, inset). In the literature
one often encounters the Förster radius
(R0), which is related to C via
R06 =
2 · C/krD.
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In Fig. 3 the positions of the six Chl a molecules in
trimeric PCP are shown (Hofmann et al., 1996
). Pigments 1 and 2 are the
interacting pigments in a monomer. On the basis of the trimeric structure, two energy equilibration processes can be expected: within
the monomer and within the trimer, respectively. From linear dichroism
and absorption spectroscopy experiments at room temperature (Kleima, 1999
) it is concluded that the two Chl a
molecules that are bound per monomeric unit are essentially
isoenergetic, which is reasonable because the two pigments are located
in very similar environments.
Because the pigments are isoenergetic at room temperature, the
intramonomeric equilibration rate (keqM) is
twice the excitation energy transfer rate
(keqM = k12 + k21 = 2k12 = 1/
eqM, where knm is the
transfer rate from pigment n to pigment m and
eqM is the time constant for equilibration within the
monomer). The intermonomeric equilibration rate
(keqT) is calculated as follows:
|
(5) |
eqT is the time constant for equilibration within the
trimer. Because the equilibration within the monomer is fast, the
transfer rate from monomer 12 to monomer 34 (k12
34) is the sum of the average transfer
rates from, respectively, pigment 1 to pigments 3 and 4 and from
pigment 2 to pigments 3 and 4. The equilibration rate within a trimer
is three times the rate for transfer between two monomeric subunits
(see, e.g., Causgrove et al., 1988Detailed comparison of experimentally determined and calculated transfer rates
To discuss the transfer processes in terms of the Förster
equation in detail, accurate knowledge of the Qy
transition dipole moment within the porphyrin plane is required. To a
first approximation the dipole is often taken to be along the
y axis (see Fig. 3), but this is not entirely correct (see,
e.g., van Zandvoort et al., 1995
, and Appendix 1). In Fig. 3 the angle
is defined, which corresponds to the angle between the
Qy transition dipole moment and the x
axis of the molecular frame of Chl a. (Note that the
y axis corresponds to the NB-ND axis of the Chl a
molecule, whereas the x axis is perpendicular to the
y axis). Assuming that the preparation exclusively contains
trimers, there are three experimentally determined parameters available
that depend on the choice of
, which will be discussed below: 1) the
amount of anisotropy (r1) that remains after
equilibration within the monomer, 2) the residual anisotropy
(r
) that remains after equilibration within
the trimer, and 3) the ratio
1/
2 of the equilibration within the monomer and trimer, respectively. However, a
complicating factor is the fact that the preparation does not only
contain trimers. Using ultracentrifugation techniques, it was shown
that the percentage of PCP trimers present in a preparation depends on
the PCP concentration, and, at the concentration applied in our
experiments, one expects the presence of both monomers and trimers
(Hofmann et al., unpublished results). Because biochemical separation
of the monomers and trimers affects the monomer/trimer equilibrium, the
exact percentages of monomers and trimers at a certain initial PCP
concentration are hard to give. As a consequence, r1 provides the most unambiguous information
about
because this term is independent of the state of
oligomerization (assuming that the relative orientations of the Chl
molecules within the monomer are the same in all cases).
The expected anisotropy after equilibration within the monomer
(reqM) can be calculated using
reqM = 0.5(0.4 + r1
2) with r1
2 = 0.2 (3cos2
12
1), where
r1
2 is the anisotropy after 100% energy transfer from pigment 1 to pigment 2 and
12 is the angle
between the relevant transition dipole moments of the interacting
pigments (see Fig. 3). The angle
12 depends on the
orientation of the transition dipole moment within the molecular frame
of the chlorophyll molecule. In Fig. 4
A reqM is plotted as a function of
. The vertical dashed line shows the value of reqM in
the case where the transition dipole moments are not rotated (
is
90°, parallel to the y axis). The horizontal dotted line
shows the experimentally determined anisotropy after equilibration
within the monomer, and the gray area reflects the error margin
(r1 = 0.16 ± 0.02). Clearly, a value
of
= 89-94° leads to a good correspondence between
experiment and calculation. Other regions where the experimental and
calculated anisotropy are in agreement are 9-15°, 57-63°, and
158-163°. However, we do not expect that the transition dipole moment has an orientation differing that much from the y
axis, because in, e.g., BChl a bound to protein,
is also
close to 90°, as can be concluded from modeling studies on LH2
(Koolhaas et al., 1998
) and the FMO complex (Louwe et al., 1997
; Vulto
et al., 1999
).
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Subsequently, the expected residual anisotropy in the case of trimers
(reqT) for
= 89-94° can be
calculated, assuming that in our sample all PCP is trimeric. A value
ranging between 0.04 and 0.05 is found for reqT,
which is lower than the experimentally determined residual anisotropy
(r
= 0.11 ± 0.02). A similar, relatively high value was found in steady-state anisotropy measurements performed both at room temperature and 4 K (unpublished results). This
shows that the assumption that the preparation exclusively contains
trimers is not correct. On the other hand, if the preparation would
contain only monomers, we would not observe a slow depolarization time.
Moreover, the linear dichroism spectrum would be completely different
(Kleima, 1999
). Obviously, the preparation consists of a mixture, which
is in line with the results of the ultracentrifugation experiments (see
above). For instance, assuming that 50% of the total amount of Chl
a is bound to trimers and 50% is bound to monomers would
explain the experimental residual anisotropy. However, if trimers and
monomers are present and the aggregation is not entirely cooperative,
the presence of dimers cannot be excluded, although there are no
biochemical indications that these indeed exist.
The ratio
1/
2 is the third experimental
parameter that provides information about the energy transfer in PCP.
This ratio is not influenced by the presence of monomers, although it
is affected by the possible presence of dimers (see below). At first, we will neglect the possible fraction of dimers. In Fig. 4 B
the calculated ratio
eqM/
eqT is shown as
a function of
. The asymptotes correspond to the case where
for
the intramonomer equilibration rate becomes zero (
eqM
). The value for
can be positive or negative, depending on
the direction of the transition dipole moment; however, because the
transfer rate is proportional to
2, the period is
180°. The dashed line shows the ratio
eqM/
eqT, which is 0.038 for unrotated
transition dipole moments (
is 90°, parallel to the y
axis). The dotted line shows the average value for the experimentally
determined ratio (
1/
2 = 0.019 ± 0.003), and the gray area reflects the error margin. Correspondence
between the experimentally determined and calculated values is found
for
= 97-105°. Other regions are 60-65°, 139-142°,
and 164-169°. However, as discussed above, these values are not realistic.
The discussion in the preceding paragraphs concerning trimers (or
monomers and trimers) is summarized in Fig.
5 A, where the amplitude of
the anisotropy reqM (dashed, right y
axis), the residual anisotropy reqT
(dotted, right y axis), and the ratio
eqM/
eqT (solid, left y axis)
are shown for
ranging from 80° to 110°. The ranges of
values (represented by gray areas) corresponding to the
experimental parameters r1 and
1/
2 do not overlap. The highest value for
based on the experimentally determined value for
r1 is
= 94°, whereas the lowest value
for
based on
1/
2 is
= 97°.
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Alternatively, if we assume that the preparation contains only dimers
(or dimers and monomers), which are organized like trimers missing one
monomeric unit, we can define the residual anisotropy in the dimer
(reqD) and the ratio
eqM/
eqD, where
eqD is the equilibration time constant within the dimer (
eqD = 1.5 ×
eqT). Fig. 5 B is similar to Fig.
5 A, but represents the case of dimers. In this case there
is horizontal overlap of the gray areas for
= 92-94°. The
residual anisotropy ranges from 0.075 to 0.09, which is in reasonable
agreement with the measured residual anisotropy. It should be noted
that trimers containing a Chl a that does not transfer
properly will also show a depolarization behavior between those of
dimers and trimers.
Summarizing, the data indicate that we do not have only monomers (or
trimers), and the data can be explained by the exclusive presence of
dimers, but this is in disagreement with biochemical experiments. We
are probably dealing with a mixture of monomers, dimers, and trimers.
Assuming dimers (or dimers and monomers) implies that
= 92°-94°, the simultaneous presence of trimers tends to favor the
slightly larger values of
.
It has been concluded by van Zandvoort et al. (1995)
that
differs
for absorption and emission. This is, in principle, due to
"solvent" relaxation, but it is demonstrated in Appendix 1 that for
Förster transfer between isoenergetic pigments one cannot simply
use different values for
in the case of absorption and emission,
because this leads to a conflict with the laws of thermodynamics. Nevertheless, in the event of transfer between isoenergetic pigments the value of
may in principle vary as a function of the
absorption/emission wavelength. If the variation exists, then the
values estimated above should be considered an effective (average) orientation.
Estimation of the refractive index
In the previous paragraph we have estimated, using the
experimentally determined values for the anisotropy
r1 and the ratio
1/
2, the values of
that lead to
agreement between the experimental data and the calculations using the
PCP structure. With this information about
, the calculated time
constants
eqM and
eqT (and/or
eqD) can be scaled to "real" time constants, using
the refractive index, krD and the overlap
integral, together forming the constant part (C) of the
Förster equation. In Appendix 2 this factor (C) is
determined. The radiative lifetime is estimated from literature values
for the fluorescence quantum yield and the fluorescence lifetime of Chl
a (Seely and Conolly, 1986
), leading to C = 42/n4 ps
1 nm6 for
rD = 18.5 ns (for details see Appendix 2). The
refractive index can be used for the actual scaling of the calculated
time constants to "real" time constants.
In Table 1 the results are shown. We have
examined the consequences for the refractive index for both scaling to
1 (upper half of Table 1) and scaling to
2 (lower half of Table 1). The first column shows
whether we assume trimers (and monomers) or dimers (and monomers), the
second column gives the upper and lower limits of
as determined in
the previous paragraph, the third column gives the calculated ratio
1/
2 (for that particular
and the
assumed composition of the preparation), and the fourth column gives
the experimentally determined upper and lower values of
1. The column with heading
2 presents the
time constants resulting from the values for the ratio and
1 in the same row. In the next column the corresponding
scaling factor is shown. The last column shows the resulting values for
n. The lower part of Table 1 is the same as the upper part,
but in this case
2 represents the experimentally
determined value.
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Clearly, the refractive indices required for proper scaling of the time
constants in the case where the preparation is assumed to consist of
trimers (and monomers) are higher than those in the case of dimers (and
monomers). The average refractive index is 1.6 ± 0.1, where the
error margins reflect the standard deviation. This value is
significantly higher than the refractive index of the medium, which is
water in this case (n = 1.33). It was suggested by Moog
et al. (1984)
that the refractive index in the Förster equation
should be interpreted as that of the bulk solution. Our data are
clearly not in agreement with that statement, and the effect of the
protein and/or the peridinins should be taken into account. By very
different methods, the refractive indices of, for example, LH2 and CP47
have been determined to be 1.63 (Andersson et al., 1991
) and 1.51 (Renge et al., 1996
), respectively.
To illustrate the dependence of the transfer rates between individual
pigments (numbering according to Fig. 3) on the value of
, these
rates are shown in Table 2 for
= 92° and for
= 97°, using C = 42/n6 ps
1 nm6 and the
average value of n (= 1.6). In addition, the corresponding factors
2/R6 and the time
constants are shown. The equilibration time constant in the case of
dimers with
= 92° is 438 ps, whereas in the case of trimers
with
= 97° we find 269 ps. Note that the discrepancy with
the experimental value is due to the strong dependence of the transfer
rates on n (see Table 1).
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We have shown here that the Chl a to Chl a
excitation energy transfer in PCP can very well be modeled using the
Förster equation. The crystal structure, in which the molecular
frames of the Chl a molecules were resolved, enabled us to
estimate the orientation of the Qy transition
dipole moments and conclude that
= 94.5 ± 2.5°. By
using this value of
, the experimentally determined excitation
equilibration time constants of 6.8 ± 0.8 ps and 350 ± 15 ps can be assigned to equilibration times within the monomer and within
the trimer/dimer, respectively.
What can be said about the in vivo functioning of PCP?
Because of the relatively slow energy transfer from one monomer to
the next within the PCP complex, one could wonder whether this transfer
will actually occur in vivo, because other transfer processes might be
faster. When two trimeric PCP complexes are oriented favorably with
respect to each other, PCP-to-PCP transfer can be faster than the
intermonomeric transfer within one trimeric complex (Hofmann,
manuscript in preparation). However, it is not very likely that larger
in vivo aggregates of PCP complexes are formed, as suggested by
Knoetzel and Rensing (1990)
, because such aggregates have not been
isolated and are not formed upon crystallization. The probably more
important energy transfer processes that might compete with those
within the PCP complex are the transfer processes to the membrane-bound
PSII complex. However, it is not known whether this transfer occurs via
the LHCa/c complex (Hofmann et al., 1996
), via the CP43 or
CP47 complexes (Mimuro et al., 1990
), or directly to the PSII core
complex (Knoetzel and Rensing, 1990
). Because the LHCa/c
complex is to some extent similar to the LHCII complex of green plants
(Hiller et al., 1995
), it might be modeled on the basis of the crystal
structure of LHCII (Kühlbrandt et al., 1994
; Hofmann, unpublished
results), and therefore it forms the "easiest" candidate for some
tentative calculations. The PCP
LHCa/c transfer can be
calculated by using this model, the assignment of Chl a
according to Kühlbrandt et al. (1994)
, and the orientations of
transition dipole moments according to Gradinaru et al. (1998)
, n = 1.6 and C = 42/n6. If
the trimer axis of PCP and LHCa/c are aligned, the
orientation (in terms of rotation along the trimer axis) is as
favorable as possible, PCP and LHCa/c are as close as
possible, and PCP is located on the luminal side, the shortest transfer
time from a PCP Chl a to a LHCa/c Chl
a is ~140 ps (Hofmann, manuscript in preparation). This is
shorter than the transfer time between two PCP monomers (~1 ns).
Including the (unfavorable) transfer from the other Chl a in
the PCP monomer and the transfer to other LHCa/c Chl
a molecules, an average transfer time of ~150 ps is found in this specific case. We thus might speculate that some transfer to
the LHCa/c complex competes with transfer between monomers, although it should be emphasized that the numbers given here
strongly depend on the modeling parameters.
| |
APPENDIX 1: ROTATION OF TRANSITION DIPOLE MOMENTS |
|---|
|
|
|---|
It was concluded from angle-resolved fluorescence depolarization
experiments on Chl a oriented in nitrocellulose film that the transition dipole moments for absorption and emission are not
oriented parallel to each other, but are at an angle of 17-19° with
respect to each other (van Zandvoort et al., 1995
). The transition dipole moment for absorption was found to be parallel to the
Qy axis (
= 90°) of the Chl molecule,
while the transition dipole moment for emission is oriented at
is
107-109° in the plane of the Chl molecule (see inset of
Fig. 3). The time scale of this rotation could easily be on the order
of a few picoseconds because it might be related to solvent (protein)
relaxation processes that have been shown to occur on such time scales
in the case of Chl b (Oksanen et al., 1998
) and therefore
could be of importance in photosynthetic complexes. Below we will
examine the consequences for Förster excitation energy transfer.
In Fig. 6 three imaginary photosynthetic
complexes are shown. The pigments are isoenergetic, and the transition
dipole moments of each pigment for absorption and emission are,
respectively, µA and µE. In Fig. 6
A two pigments are placed at rotationally symmetrical
positions with respect to the axis perpendicular to the plane of the
paper. For excitation energy transfer from pigment 1 to 2 the
transition dipole moments µ1E and µ2A are
involved, while for transfer from 2 to 1 µ2E and
µ1A are involved. Because of the symmetrical position of
the pigments with respect to each other,
1
22
equals
2
12, so that back and forward excitation
energy transfer rates are the same. In Fig. 6 B an
asymmetrical dimer is shown. Because in this case the angle between
µ3E and µ4A is not the same as the angle
between µ4E and µ3A, it follows that
3
42 is not equal to
4
32.
Therefore, in equilibrium relatively more excitations would be located
on pigment 3 than on pigment 4, although the pigments are isoenergetic.
In Fig. 6 C a symmetrical trimeric structure is shown. In
the trimer the pigments 5 and 6 are at the same positions with respect
to each other as the pigments 3 and 4. As a consequence, the transfer
from pigment 6 to 5 is faster than that from pigment 5 to 6, and the
same holds for the pigment pairs 5-7 and 7-6. In other words, in the
case of three isoenergetic pigments with different orientations of the
transition dipole moments for absorption and emission, the excitation
would continuously circle around, which seems counterintuitive.
|
In the case of isoenergetic pigments in the asymmetrical dimer, the
unidirectionality of transfer is thermodynamically impossible. Apparently, rotation of the transition dipole moment in the excited state cannot occur without affecting the energy of the excited state.
In other words, it is no longer correct to assume that the energy of
the pigment in the excited state and the orientation of the transition
dipole moment are independent properties. An explanation for this
feature is that the rotation of the transition dipole moment might be
caused by solvent reorganization effects, in general leading to a
lowering of the energy of the excited state. Förster excitation
energy transfer only takes place when the corresponding instantaneous
donor and acceptor transition energies are the same. As a consequence,
formally the orientation factor in the Förster equation becomes
energy dependent and therefore has to be included in the overlap
integral:
|
with respect to the molecular frame. The value for
is taken to be the same for all pigments. Thus the angle should be
considered as an effective "average" angle.
| |
APPENDIX 2 |
|---|
|
|
|---|
Below the constant factor in the Förster equation, consisting of the overlap integral and the radiative rate, is calculated.
To calculate the overlap integral in the Förster equation, the
extinction coefficient of PCP in the Chl a Qy
band has to be estimated. To that end the absorption spectrum of the
Qy band in PCP has been compared to that of Chl
a in different solvents with known extinction coefficients.
The FWHM of the Qy band in the OD spectrum of
PCP is 14 nm (see Fig. 1). The extinction coefficients and FWHMs of the
Qy band of Chl a are 90.25 mM
1 cm
1 in ether (FWHM 17 nm;
Lichtenthaler, 1987
), 79.6 mM
1 cm
1 in 100%
methanol (FWHM 22 nm; Eijckelhoff and Dekker, 1995
), and 86 mM
1 cm
1 in aqueous acetone (FWHM 20 nm;
Eijckelhoff and Dekker, 1995
) (Lichtenthaler, 1987
; Porra et al.,
1989
). Assuming that the dipole strengths of Chl a in PCP
and in these solvents are the same, we have normalized the areas of the
absorption spectra with respect to each other in the
Qy region and thus estimated the extinction coefficient of Chl a in PCP to be ~110 mM
1
cm
1.
The radiative rate in the Förster equation is estimated by using
krD =
f/
f,
where
f is the fluorescence lifetime and
f is the quantum yield for fluorescence. Using
literature values for
f and
f for Chl
a in methanol and in ether, we find an average radiative
lifetime of 18.5 ns (Seely and Conolly, 1986
). So for C we
find a value of 42/n4 ps
1
nm6.
| |
ACKNOWLEDGMENTS |
|---|
The authors thank Dr. Marc van Zandvoort and Drs. Markus Wendling for useful discussions and Dr. Roger Hiller for providing us with the unpurified PCP material.
This work was supported by a Dutch Science Foundation FOM grant to HvA and RvG.
| |
FOOTNOTES |
|---|
Received for publication 3 June 1999 and in final form 2 September 1999.
Address reprint requests to Dr. Foske J. Kleima, Division of Physics and Astronomy, Faculty of Sciences, Vrije Universiteit, De Boelelaan 1081, 1081 HV Amsterdam, the Netherlands. Tel.: 31-20-444-7941; Fax: 31-20-444-7999; E-mail: foske{at}nat.vu.nl.
| |
REFERENCES |
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-carotene and pheophytin a in solution and in green plant photosystem II.
J. Photochem. Photobiol.
96:109-121
Biophys J, January 2000, p. 344-353, Vol. 78, No. 1
© 2000 by the Biophysical Society 0006-3495/00/01/344/10 $2.00
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