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Biophys J, September 2000, p. 1561-1572, Vol. 79, No. 3


*Department of Chemistry and Biochemistry, Arizona State
University, Tempe, Arizona 85287, and
Ames
Laboratory- U.S. Department of Energy and Department of Chemistry,
Iowa State University, Ames, Iowa 50011 USA
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ABSTRACT |
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Results from high-pressure and Stark hole-burning
experiments on isolated chlorosomes from the green sulfur bacterium
Chlorobium tepidum are presented, as well as Stark
hole-burning data for bacteriochlorophyll c (BChl
c) monomers in a poly(vinyl butyral) copolymer film.
Large linear pressure shift rates of
0.44 and
0.54
cm
1/MPa were observed for the chlorosome BChl
c Qy-band at 100 K and the lowest
Qy-exciton level at 12 K, respectively. It is argued that
approximately half of the latter shift rate is due to electron exchange
coupling between BChl c molecules. The similarity
between the above shift rates and those observed for the B875 and B850 BChl a rings of the light-harvesting complexes of purple
bacteria is emphasized. For BChl c monomer,

µ = 0.35 D, where
µ is the dipole moment change for
the Qy transition and
is the local field correction
factor. The data establish that
µ is dominated by the
matrix-induced contribution. The change in polarizability (
) for
the Qy transition of the BChl c monomer is
estimated at 19 Å3, which is essentially identical to that
of the Chl a monomer. Interestingly, no Stark effects
were observed for the lowest exciton level of the chlorosomes (maximum
Stark field of 105 V/cm). Possible explanations for this
are given, and these include consideration of structural models for the
chlorosome BChl c aggregates.
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INTRODUCTION |
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Green sulfur bacteria, such as
Chlorobium (Cb.) tepidum and Cb.
limicola, and green nonsulfur bacteria, such as
Chloroflexus (Cf.) aurantiacus, are
separated by a large evolutionary distance according to 16S rRNA
analysis (Woese, 1987
; Olsen et al., 1994
). Their distinctiveness is
reflected in the different types of reaction centers and membrane-bound
antenna complexes found in the two families, as well as their entirely
distinct metabolic and ecological characteristics (see Blankenship et
al., 1995
; Olson, 1998
, and references therein). Interestingly, they
both contain chlorosomes; an antenna complex of flattened ellipsoidal
shapes of ~100 × 30 × 10 nm3 for
the green nonsulfur bacteria and ~200 × 70 × 12 nm3 for the green sulfur bacteria. Chlorosomes
consist of up to ~10,000 aggregated bacteriochlorophyll (BChl)
c, d, or e molecules surrounded by a
monolayer lipid envelope and a relatively small amount of protein. BChl
a molecules are associated with the baseplate of the
chlorosomes (Blankenship et al., 1995
; Olson, 1998
), which serves as an
intermediate in the excitation energy transfer from the chlorosomes to
BChl a-containing antenna complexes in both types of
microorganisms: the B808-866 complex for the green nonsulfur bacteria
and the Fenna-Matthews-Olson (FMO) complex for the green sulfur
bacteria. Fig. 1 is a schematic of the
arrangement of photosynthetic complexes in green sulfur bacteria. The
molar ratio of BChl c (d or e) to BChl
a in the chlorosomes varies with species and growth
conditions. Molar ratios of 20:1 for chlorosomes from Cf. aurantiacus (Schmidt, 1980
) and 90:1 for those from Cb.
limicola (Gerola and Olson, 1986
) have been reported.
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Compared with other antenna complexes, chlorosomes have relatively low
protein to BChl c, d, or e ratios,
ranging from ~0.5 to ~2, depending on the species and growth
conditions (Cruden and Stanier, 1970
; Schmidt, 1980
; Feick and Fuller,
1984
; Chung et al., 1994
; Blankenship et al., 1995
). It is generally
accepted that pigment-pigment interactions within chlorosomes are
mainly responsible for the pigment organization, rather than
pigment-protein interactions, as is commonly found in other antenna
complexes. BChl c, d, or e can readily
form aggregates in nonpolar organic solvents (Bystrova et al., 1979
;
Smith et al., 1983
; Brune et al., 1987
; Olson and Pedersen, 1990
) or
aqueous lipid/detergent micelles (Hirota et al., 1992
; Miller et al.,
1993
; van Noort et al., 1997
) in vitro with spectroscopic properties
similar to those observed in chlorosomes. That is, the
Qy band of the BChl c monomers at
~670 nm is red-shifted to the ~720-760-nm region because of the
formation of aggregates. Based on resonance Raman, Fourier transform
infrared spectroscopy, and absorption studies, the BChl c
molecules are essentially pentacoordinated, and the 31 hydroxyl and 131 keto
groups are involved in the aggregation (Brune et al., 1988
; Lutz and
van Brakel, 1988
; Nozawa et al., 1990
; Hildebrandt et al., 1994
). It is
believed that the aggregated BChl c, d, or
e molecules form rods 5-10 nm in diameter within
chlorosomes, as was seen in freeze-fracture electron micrographs of
Cb. limicola and Cf. aurantiacus cells (Staehelin
et al., 1978
, 1980
; Golecki and Oelze, 1987
). Various pigment
aggregation models have been proposed for the chlorosome aggregates
that are based on antiparallel chains (Brune et al., 1988
; Nozawa et
al., 1994
; Minuro et al., 1995
), parallel stepped chains (Brune et al.,
1988
; Mizoguchi et al., 1998
), and cylindrical arrangements of BChl
molecules (Somsen et al., 1996
). Larger scale structural models for the rod elements, aided by quantum chemical calculations or molecular modeling, have also been proposed (Holzwarth and Schaffner, 1994
; Buck
and Struve, 1996
; Fetisova et al., 1996
).
Over the past 20 years nonphotochemical hole-burning (NPHB)
spectroscopy has been applied to chromophores embedded in disordered host media whose optical spectra suffer from significant inhomogeneous broadening. Photosynthetic protein complexes with an inhomogeneous broadening contribution of ~100 cm
1 to the
absorption bandwidths are good candidates for NPHB spectroscopy, which
can improve spectral resolution by two to three orders of magnitude.
Information that is obtainable includes the inhomogeneity of the
protein complex, excited-state lifetimes, exciton-level structures, the
electron-phonon coupling strength of optical transitions and
frequencies, and Franck-Condon factors of chlorophyll (Chl) modes. For
general reviews covering NPHB and its applications, see Moerner (1988)
and Jankowiak et al. (1993)
. For reviews pertaining to NPHB studies of
photosynthetic complexes, see Johnson et al. (1991)
, Reddy et al.
(1992a)
, and Jankowiak and Small (1993)
.
Recently, NPHB, in combination with high pressure and electric (Stark)
fields, has been applied to several photosynthetic protein complexes.
The results obtained led to new insights into excitation energy
transfer dynamics and the Qy electronic
structures of Chl molecules. Of particular relevance to this study are
the high-pressure- and Stark-NPHB experiments of Reddy et al. (1996)
, Wu et al. (1996
, 1997a
, 1998
), and Rätsep et al. (1998a
,b
) on light-harvesting (LH) complexes from purple bacteria. Not only are the
results of those studies consistent with the structure of LH2 as
determined by x-ray crystallography; they also provide benchmarks for
electronic structure calculations by establishing that electron
exchange coupling between nearest-neighbor pigments and energy disorder
associated with the cyclic LH2 and LH1 rings cannot be ignored. This is
important because a firm understanding of the Qy
states of Chl molecules bound to the proteins of LH complexes is
essential for understanding their excitation energy transfer/relaxation
dynamics. The usefulness of the external field/NPHB combination (or
external field/optical spectroscopy combination in a broader sense) in
the study of dynamics, structures, interactions, and functions is not
limited to photosynthetic complexes. In principle, any system with a
probe is an ideal candidate for such a study. An example of a probe
intrinsic to the system is the heme group in hemoglobin, but artificial
labeling is also possible, such as the labeling of human serum albumin
with hypericinate ions (Falk and Meyer, 1994
). An example of an
external field/optical spectroscopy combination study that is
nonbiologically oriented is the photon echo investigation of optical
dephasing in pentacene-doped polymethyl methacrylate under high
pressure (Berg and Chronister, 1997
). The reader interested in the
effects of high pressure and Stark fields on the spectroscopic
properties of pigments bound to proteins is referred to the review
articles of Kohler et al. (1998)
and Fidy et al. (1998)
.
The chlorosome Qy bands of Cf.
aurantiacus and Cb. limicola, which have absorption
maxima at 742 and 751 nm, respectively, have been investigated by NPHB
in the fluorescence excitation mode at low temperature (Fetisova and
Mauring, 1992
, 1993
). The results were consistent with the chlorosome
pigments being excitonically coupled. The lowest exciton level of the
Qy band was characterized by zero-phonon hole
(ZPH) action spectroscopy and found to carry an inhomogeneous full
width at half-maximum (FWHM) of ~100 cm
1 with
a band center at ~752 nm for Cf. aurantiacus and ~774 nm for Cb. limicola. The ZPH action spectrum is generated by
burning a series of ZPHs across the absorption band with constant laser fluence and is a powerful method for obtaining the width, center, and
intensity of an inhomogeneously broadened distribution mixed with other
absorption contributions. An example of such a study on photosynthetic
antenna complexes is the identification of the lowest exciton level
(B870) of LH2 complex from Rhodopseudomonas acidophila (Wu
et al., 1997c
). Broad nonresonant holes resulting from fast
interexciton-level relaxation from the higher exciton components, which
carry most of the oscillator strength, were also observed. Recently,
ZPH action spectroscopy was applied in a study of the lowest exciton
level of chlorosomes of Cb. tepidum (Psencik et al., 1998
).
The lowest exciton level was found to lie in the range of 760-800 nm
and to be centered at ~780 nm. The fractional hole depth of the most
intense hole was 0.04 in the action spectrum. Different redox
conditions were also employed to examine their effects on hole widths,
as the excited-state lifetime of BChl c aggregates and
energy transfer to the baseplate were known to be regulated by the
redox potential for green sulfur bacteria. The ZPH width was 1.8 cm
1 under anaerobic conditions and 4.0 cm
1 under aerobic conditions and was
independent of wavelength and temperature up to 25 K. Psencik et al.
(1998)
proposed that the ZPH width is due to the BChl
c-to-BChl c energy transfer. A width of 1.8 cm
1 corresponds to a BChl c-to-BChl
c energy transfer time (T1)
of 5.8 ps, whereas a width of 4.0 cm
1
corresponds to a transfer time of 2.7 ps. The shortening to 2.7 ps may
be due to an additional quenching mechanism, involving one or both of
the quinone molecules chlorobiumquinone and menaquinone-7 under
oxidizing conditions (Frigaard et al., 1997
).
Currently the exact structural arrangement of the pigments within the
chlorosomes is unknown, but models generally include J-aggregate-like
long chains arranged circularly to form the rod elements observed by
electron microscopy. The homogeneous line shift and broadening of
pseudoisocyanine (PIC) J-aggregates under pressure (<6.5 MPa) have
been investigated by hole-burning spectroscopy at 4.2 K (Hirschmann and
Friedrich, 1992
). The holes within the J-band were found to shift with
a linear rate of about
0.3 cm
1/MPa, which
depends on the burn frequency within the band. The hole broadening
induced by pressure was found to be surprisingly small. The largest
linear broadening rate observed was ~0.025 cm
1/MPa; a dependence on the burn frequency
(color effect) was observed. Hirschmann and Friedrich argued that the
low hole-broadening rate is the result of motional narrowing of
structural heterogeneity due to large exciton coherence lengths.
Before this study, Stark hole burning was applied to the J-band of
aggregated pseudoisocyanine iodide (PIC-I) at 2 K (Wendt and Friedrich,
1996
). The aggregation of PIC-I reduced the linear Stark effect by more
than two orders of magnitude compared to the monomer. At a field
strength of 300 kV/cm, the quadratic Stark effect was significant for
the J-aggregate (comparable to the linear contribution). The large
difference in the polarizability between the ground and excited states,
which is responsible for the quadratic Stark effect, was argued to be
due to the aggregation of PIC-I molecules on the basis of exciton
theory. Wendt and Friedrich argued that certain structural constraints
such as a helical pigment organization could explain the large
reduction in the linear Stark effect of the aggregates.
Recently, conventional Stark modulation spectroscopy at 77 K was used
in a study of chlorosomes from Cf. aurantiacus (in both wild-type and carotenoid-deficient cells) (Frese et al., 1997
). The
Stark spectrum of the Qy band resembles a
first-derivative-type lineshape, consistent with there being a large
difference in polarizability between the ground and excited states
(Tr(
) = 1650 ± 100 Å3/f2, where Tr(
)
denotes the trace of the polarizability difference tensor). The
second-derivative contribution to the Stark spectrum was found to be
negligible, which indicates that the dipole moment change between the
ground and excited states is very small. Frese et al. suggested that
the aggregated BChl c in chlorosomes adopt an antiparallel
structure, as opposed to various parallel models proposed by others
(Brune et al., 1988
; Alden et al., 1992
; Mizoguchi et al., 1998
).
We present here the results of high-pressure and Stark hole-burning experiments on isolated chlorosomes from BChl c containing Cb. tepidum, as well as Stark hole-burning results for BChl c monomers in a polymer film. The motivations for the experiments were to gain additional insights into the arrangement of BChl c molecules in chlorosomes and the exciton level structure of the aggregates (with emphasis on the lowest Qy exciton level) and to provide benchmarks for electronic structure calculations based on structural models for the BChl c aggregates.
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EXPERIMENTAL |
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Cb. tepidum cells were grown at ~40°C in a
90-liter clear plastic vessel in a modified version of the CH1 medium
reported by Olson et al. (1973)
and illuminated with four banks of
fluorescent tube lights (
60 µEinsteins m
2
s
1) over 3-4 days with gentle stirring. Cells
were harvested using a continuous flow centrifuge and used in the
preparation of chlorosomes.
Chlorosomes were isolated following the method of Gerola and Olson
(1986)
with minor revisions. Four grams of cell paste was mixed with 16 ml of chlorosome buffer (10 mM sodium phosphate (pH 7.4), 10 mM sodium
ascorbate, and 2 M sodium thiocyanate) until an even suspension was
achieved. Cells were broken by sonication in the presence of DNase I,
and the sonicate was centrifuged to remove cell debris. The dark green
supernatant was layered on top of a 20-50% continuous sucrose density
gradient. The sucrose gradient was spun at 45,000 rpm for 18 h at
4°C, and the chlorosome fraction was removed. Chlorosomes (FMO
depleted) equilibrate between 25% and 30% sucrose.
BChl c pigments used in the Stark hole-burning experiment
were extracted from whole cells of Cb. tepidum according to
the procedure described by van Noort et al. (1997)
. BChl c
was dissolved in methanol, which prevents the formation of aggregates,
and was added to poly(vinyl butyral-co-vinyl alcohol-co-vinyl acetate) (Aldrich, Milwaukee, WI)/dichloromethane solution (0.5 g of the polymer
with an average molecular weight of 90,000-120,000 in 15 ml
dichloromethane). The solution was dried overnight in a flat Petri dish
covered by a glass plate (to reduce the drying rate). The dried film
was kept in an oven under vacuum at 40°C for ~2 h to remove the
residual solvent. Typically the film separated from the Petri dish
after it was placed in a darkened closed box with a wet towel for ~2
days. The resulting OD and FWHM of the BChl c absorption
band at 667 nm at room temperature were 0.07 and
400 cm
1, respectively.
Hole-burned spectra of chlorosomes were detected in the absorption mode
(Lyle et al., 1993
). A Ti:sapphire ring laser (model 899-21, linewidth
~0.07 cm
1; Coherent, Santa Clara, CA) pumped
by a Coherent 15-W argon ion laser was used to burn holes in the
Qy absorption band. The spectra before and after
burning were recorded with a Bruker IFS 120 HR Fourier transform
spectrometer (Bruker, Billerica, MA). Burn fluence and spectral reading
resolutions are given in the figure captions.
Because of the smaller ZPH width, spectral hole burning of BChl
c monomers was detected in the fluorescence excitation mode with an apparatus described by Reinot et al. (1996)
and Kim et al.
(1995)
. The burn and read laser was a Coherent 699-21 ring dye laser
(linewidth <30 MHz) pumped by a 6-W Coherent Innova 90 Ar ion laser
stabilized by a LS 100 power stabilizer (Cambridge Research and
Instrumentation, Cambridge, MA). Fluorescence was detected by a GaAs
photomultiplier tube (RCA C31034) and a photon counter (SR-400;
Stanford Research Systems, Sunnyvale, CA). Scattered laser light was
eliminated with cutoff filters at 750 nm. Laser intensities used for
hole burning were in the range of ~10 µW/cm2,
and hole depths were typically ~25%. For hole reading, the duration of which was ~300 s, the laser was attenuated by a factor of ~60.
High pressures of up to 1.5 GPa were generated by compressing helium
gas with a Unipress U11 three-stage compressor (Warsaw, Poland). The
sample was contained in a gelatin capsule and placed in a high-pressure
cell (rated for pressures less than 800 MPa) with two sapphire windows
installed. A custom-made liquid helium cryostat (Janis, Wilmington, MA)
was used to achieve low temperatures for the high-pressure hole-burning
experiments. For further details, see Reddy et al. (1995)
.
A Trek model 610 C dc high-voltage power supply (0 to ± 10 kV;
Trek, Medina, NY) was used to generate the Stark field. By changing the
polarity of the power supply, we were able to achieve a maximum Stark
field difference of 100 kV/cm for two copper electrodes separated by 2 mm. For the quadratic Stark effect, however, the highest field
achievable was 50 kV/cm, because the positive and negative polarities
of the power supply would result in the same effect. The gelatin
capsule containing the sample was allowed to soften at room temperature
for 5 min before being squeezed into the space between the electrodes
(optical path length ~6 mm). To avoid dielectric breakdown, all
measurements were performed at 1.8 K in a Janis 10 DT liquid helium
cryostat. This setup allowed for study of the Stark effect with varying
laser polarization relative to the external field. The interested
reader is referred to Rätsep et al. (1998a)
for further details.
The Stark cell used in the fluorescence excitation mode for the BChl
c monomer study consisted of two vertical Teflon walls and
two copper electrodes perpendicular to the walls (Milanovich et al.,
1998
). A separation distance of 5 mm between electrodes was maintained
by placing them in the grooves on the inside of the Teflon walls. A
slit was made in one of the Teflon walls to allow the laser access to
the sample. Fluorescence was collected at a 90° angle relative to the
incident laser light through an opening on the other Teflon wall in the
Stark cell. A polarizer placed in front of the Stark cell allowed for
control of the laser polarization relative to the applied field direction.
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RESULTS |
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Pressure-dependent studies of the Qy band and its lowest exciton level
Fig. 2 shows the near-IR absorption
spectrum of chlorosomes at 15 and 752 MPa (1 MPa
10 atm) at
100 K. A red shift of 320 cm
1 (from 13,250 ± 5 to 12,930 ± 5 cm
1) and a band
broadening of 95 cm
1 (from 550 ± 5 to
645 ± 5 cm
1) with increasing pressure are
observed. Fig. 3 plots the absorption band positions and widths versus pressure. Within the pressure range
employed, the red shift and broadening are reversible and linear
with pressure (see the regression lines in Fig. 3). The linear pressure
shift and broadening rates were
0.44 and 0.12 cm
1/MPa, respectively.
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|
As in the studies of LH2 and LH1 antenna complexes of purple bacteria
(Reddy et al., 1992b
, 1993
; Wu et al., 1997c
, 1998
), the lowest exciton
level of the chlorosome Qy band was studied by
means of ZPHs burned at the red edge of the band. This level was
determined by ZPH action spectroscopy at ambient pressure to have an
inhomogeneous distribution width (FWHM) of ~100 ± 10 cm
1 and was centered at ~12,900 ± 10 cm
1 (775 nm), consistent with the findings of
Psencik et al. (1998)
for Cb. tepidum. The pressure shifting
of the lowest exciton level of the Qy band at 12 K is shown in Fig. 4. Five ZPHs were
burned at 15 MPa in this spectral region, which shift to the red with increasing pressure. The inset of Fig. 2 shows the ZPHs burned at
12,862 cm
1 at 12 K and 15 MPa. The shifting and
broadening of that hole resulting from an increase in pressure to 34 MPa are also shown. Because of the solidification of the
pressure-transmitting medium, helium gas, at ~75 MPa at 12 K, as well
as rapid hole filling and broadening, no data were obtained beyond 57 MPa. As with the absorption band, the shift of ZPHs is linearly
dependent on the pressure (see the regression lines and their slopes in
Fig. 4) with an averaged linear pressure shift rate of
0.54
cm
1/MPa. Unlike the lowest exciton level (B870)
of B850 molecules of LH2 from Rps. acidophila and Rb.
sphaeroides (Wu et al., 1997a
), which exhibits an increase in
shift rate in going from the high-energy to low-energy sides of the
band, the shift rate of the lowest exciton level of the chlorosome
Qy band is essentially constant.
|
Stark-hole burning studies
The Stark shift of the optical transition frequency of the
absorber is given by
|
(1) |
is the local field correction factor and is taken to be a
scalar.
µ0 is the molecular dipole
moment change, and 
0 is the
molecular polarizability difference tensor.
Eint is the matrix field
experienced by the absorber and the induced dipole moment
µind = 
Eint. The
first and second terms in the square brackets depend linearly and
quadratically on the Stark field Es,
respectively. As reviewed in Rätsep et al. (1998b)
106 V/cm (see also Kador et al., 1990
was enhanced because of
aggregation (Wendt and Friedrich, 1996Considering further the case of isolated molecules in glassy matrices
with the domination of the linear Stark effect, let
be the angle
between the molecular dipole moment difference vector
µo and the transition dipole vector
d. Linearly polarized light preferentially burns out
those molecules with d parallel to the
polarization vector eof the light. The experimentally observed dipole moment change can be written as
µ =
µo +
µind, where
µind is the matrix-induced
dipole moment change equal to

Eint. When
µo is dominant, photoselection enables one to probe molecules for which the angle between
µo and e is well
defined (shallow hole limit). As discussed by Meixner et al. (1986)
and
Gafert et al. (1995)
, Stark splitting of the hole can be observed for
an angle between e and
Es, which depends on the value
of
. For example, for
= 0 or
, Stark splitting occurs
for parallel polarization, while symmetrical broadening occurs for
perpendicular polarization. The situation is reversed for
= ±
/2. However, when
µind is
dominant, only Stark broadening is expected for both polarizations.
This is because the orientation of
µind relative to d
or e is random for a glassy matrix, i.e., the matrix
field varies significantly from site to site.
The assumption of random orientations for
µind for Chl molecules in
photosynthetic complexes is questionable because the structure of the
protein around these chromophores is well defined, although the
Qy absorption bands do suffer from significant inhomogeneous broadening. For example, Gafert et al. (1995)
observed Stark hole splitting for two of the three sites of mesoporphyrin substituted in horseradish peroxidase. For the same molecule in a
glass, only Stark broadening was observed for both laser polarizations. Gafert et al. introduced the notion of random and nonrandom protein contributions to
µind, i.e.,
µind(random) and
µind(nonrandom). Recently, Rätsep et
al. observed Stark splitting and broadening with parallel and
perpendicular laser polarizations, respectively, for the lowest exciton
level of the FMO complex (Rätsep et al., 1998a
). However, for the
B800 and B870 bands of the LH2 complex and B896 of the LH1 complex,
Stark broadening of the ZPH was observed for both parallel and
perpendicular laser polarizations (Rätsep et al., 1998a
,b
).
Stark hole-burning studies of the Qy band of BChl c monomers
Fig. 5 shows the Stark broadening of a ZPH burned at 670.2 nm (14921 cm
1) into the
Qy absorption band of BChl c monomers
in a poly(vinyl butyral) copolymer film at 1.8 K for laser polarization
perpendicular to the Stark field. (Hole broadening was also observed
for laser polarization parallel to the Stark field.) The FWHM of the
hole at zero field is 1.1 GHz (0.036 cm
1) and
increases symmetrically to 1.7 GHz (0.058 cm
1)
at 4 kV/cm. Fig. 6 shows the
dependence of the FWHM of the hole burned at 670.2 nm on electric field
(diamonds) and the theoretical fit (solid curve)
obtained using the theory of Kador et al. (1987)
µ for the Qy
transition based on the symmetrical hole-broadening fit is 0.35 ± 0.03 D near the absorption band maximum (670.2 nm). It increases to
0.48 ± 0.05 D at the red side of the band (677 nm) (results not
shown). Changing the laser polarization did not affect the broadening rate and hole shape.
|
|
Stark hole-burning studies of chlorosomes
Stark hole-burning experiments on the lowest exciton level of the chlorosome Qy band were conducted at 1.8 K. The widths of the ZPH at zero field were ~2 cm
1, as
detected in the absorption mode (results not shown). This width, if
interpreted in terms of energy transfer from the lowest exciton level
to the baseplate, corresponds to a transfer time (T1) of 5 ps. However, the possibility
that the width is due to pure dephasing from exciton-defect scattering
cannot be excluded. However, no Stark effect (i.e., broadening,
splitting, or shift) was observed. Possible reasons for the
absence of Stark effects will be discussed in the following section.
| |
DISCUSSION |
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|
|
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Absorption spectra
Compared with the 4.2 K absorption bands of other photosynthetic
antenna complexes such as B800 (FWHM = 125 cm
1) and B850 of LH2 (FWHM = 200 cm
1) of purple bacteria and the three partially
resolved Qy bands (FWHM
100 cm
1) of the FMO complex, the chlorosome
Qy band is considerably broader (FWHM
550 cm
1) and clearly asymmetrical (Fig. 2). Given
that the inhomogeneous broadening of the lowest exciton level of the
chlorosome is only ~100 cm
1, a significant
fraction of the 550 cm
1 width is most likely
due to higher energy exciton levels. These levels are inhomogeneously
and homogeneously broadened because of structural heterogeneity
and downward interexciton level relaxation, as proposed in the
earlier hole-burning papers discussed in the Introduction.
Before discussing the spectral heterogeneity of chlorosomes, it is
useful to discuss the exciton level structure of a J-aggregate. For a
linear chain of N identical molecules, the Hamiltonian in the absence of energy disorder is (Fidder et al., 1991
; Alden et al.,
1992
)
|
(2) |

label the states in which molecule
(
= 1, 2, ... N) is excited and all others are in the ground
state. e is the excitation energy of the chromophore, and
V
is the coupling energy between molecules
and
. Under the nearest-neighbor coupling approximation
V
,
+1 ± V
,
1 =
V, the
Hamiltonian can be diagonalized exactly to give the eigenfunctions and
eigenenergies as
|
(3) |
|
(4) |
is found to be
(Fidder et al., 1991
|
(5) |
|
(6) |
For J-aggregates, the coupling energy
V between the
nearest neighbors must be negative. As a result, the lowest exciton
level (j = 1) carries most of the transition dipole
strength in the absence of energy disorder. However, the J-aggregate
picture is inconsistent with NPHB studies of chlorosomes which
establish that the lowest exciton level is only weakly allowed (see
Results and Fetisova and Mauring, 1992
, 1993
, and Psencik et al.,
1998
). Buck and Struve (1996)
proposed that this issue can be resolved by introducing a tubular arrangement of J-aggregates and diagonal energy disorder to explain the exciton level structure of chlorosomes. Their tubular arrangement leads to the lowest exciton level being forbidden in the absence of energy disorder. Energy disorder endows this level with some intensity stolen from the allowed levels. This
situation is similar to those of B870 of LH2 and B896 of LH1 of purple
bacteria (Reddy et al., 1992b
, 1993
; Wu et al., 1997b
,c
; Wu and Small,
1997
, 1998
). The picture that emerges is that the broad and
asymmetrical Qy band of chlorosomes is a
superposition of exciton levels carrying different absorption
intensities and, possibly, bandwidths. However, the tailing on the blue
side of the Qy absorption band seen in Fig. 2 may
be contributed to by weak intramolecular vibronic transitions of the
BChl c molecules (Cherepy et al., 1996
).
Spectral equilibration among different components of chlorosome BChl
c molecules of Cb. tepidum was observed in the
femtosecond pump-probe experiments of Savikhin et al. (1995)
. A red
shift in the absorption difference spectrum was observed upon 720-nm excitation. The one-color and two-color isotropic data also confirmed the existence of spectral heterogeneity within the chlorosome absorption band. Similar results have been obtained for chlorosomes from BChl e-containing Cb. phaeovibrioides and
BChl c- and d-containing Cb.
vibrioforme by picosecond pump-probe laser spectroscopy (van Noort
et al., 1994
). Interestingly, chlorosomes from Cf.
aurantiacus, which contain BChl c and trace quantities
of BChl d molecules, do not show such downhill energy
transfer within BChl aggregates. At room temperature, the FWHM of the
chlorosome Qy band of Cb. tepidum and
Cf. aurantiacus is 800 and 530 cm
1,
respectively, suggesting greater heterogeneity for Cb.
tepidum. As mentioned in the Introduction, the chlorosomes from
green sulfur bacteria such as Cb. tepidum are larger in size
and have higher BChl c/BChl a ratios than those
of green nonsulfur bacteria such as Cf. aurantiacus. This,
together with the spectral equilibration data obtained by Savikhin et
al. (1995)
, suggests that more than one pool of BChl aggregates exists
in green sulfur bacteria such as Cb. tepidum to compensate
for the lower energy transfer efficiency to the baseplate due to larger
chlorosome sizes and lower amounts of BChl a molecules. The
different pools of BChl aggregates may be due to variations in the size
of the rod elements and/or the relative numbers of BChl c,
d, and e molecules and their homologs.
High-pressure studies
Pressure shifting of the Qy band
According to earlier high-pressure studies on isolated chromophore systems and protein complexes, it was found that a pressure shift rate larger than ~0.2 cm
1/MPa is an indication of
strong interactions between pigments (Reddy et al., 1996
1 and negligible electron exchange coupling
permit use of the Laird-Skinner theory. That is, the pressure shifting
appears to be dominated by attractive pigment-protein interactions, as
required by the theory.
Despite the success of the Laird-Skinner theory in accounting for the
pressure shift rates of the above systems, it is inapplicable to
strongly coupled BChl in chlorosomes that exhibit a pressure shift rate
of ~
0.5 cm
1/MPa. Currently there is
no microscopic theory for pressure shifting of strongly exciton-coupled
systems. Thus, in what follows, we use the simple analysis procedure
developed for the B850 band of LH2 and the B875 band of LH1 (Wu et al.,
1998
/
p is
|
(7) |
is the compressibility. Based on the red shift of ~1400 cm
1 for the
aggregated BChl c in chlorosomes relative to monomeric BChl
c, the value of V is ~700
cm
1. This value has been used in theoretical
calculations and modeling of chlorosomes (Buck and Struve, 1996
1 (Kopainsky et al., 1981
1 (Wu et al., 1998
1 and
= 0.1 GPa
1 (Perepechko, 1980
0.14
cm
1/MPa. For the pressure shift rate of
chlorosomes, the total contribution of
0.14
cm
1/MPa from electrostatic couplings and
0.1
cm
1/MPa from dispersion interactions (Wu et
al., 1998
0.50
cm
1/MPa by
0.26
cm
1/MPa. Thus, as in the case of the strongly
coupled B850 and B875 molecules of LH2 and LH1, it appears that
electron exchange interactions between the aggregated BChl c
molecules in chlorosomes should not be neglected in the analysis. We
note that electron exchange coupling leads to charge transfer states
that interact with the 
* states.
The contribution of electron exchange (EE) interactions to the pressure
shift rate is approximately given by
|
(8) |
VEE/
REE =
A for
REE < ± 0.1 Å.
VEE is the change in coupling due
to a change in
REE. Utilization of
Eq. 8 requires a value for REE that,
in the absence of a x-ray structure of chlorosomes, cannot be
estimated, although it may correspond to the interplanar separation
between neighboring BChl c molecules. For the B850 molecules
of LH2, REE was taken to be 3.5 Å,
based on the x-ray structure (Freer et al., 1996
= 0.1 GPa
1, an
A value of 110 cm
1/0.1 Å is
obtained from Eq. 8 to account for the discrepancy of
0.26
cm
1/MPa in the pressure shift rate mentioned
above. Using the same method and REE = 3.5 Å, an A value of 85 cm
1/0.1 Å for the B850 molecules of the LH2 complex and 126 cm
1/0.1 Å for the B875 molecules of the LH1
complex of purple bacteria were obtained (Wu et al., 1998Pressure broadening of the Qy band
As summarized in table 1 of Wu et al. (1997a)
1/MPa,
depending on the species. For the Qy band of
isolated chlorosomes, the broadening rate is 0.12 cm
1/MPa (Fig. 3). Pressure broadening can be
qualitatively understood in terms of the underlying exciton level
structure and the pressure shifting rates of the levels. Different
exciton levels may shift at different rates, and the rates can have
different signs, leading, therefore, to pressure broadening. This
reasoning is supported by the observation that the shift rate of
0.54
cm
1/MPa for the lowest exciton level is larger
than the shift rate of
0.44 cm
1/MPa for the
origin absorption band of the chlorosome Qy
transition, as determined from the band maximum. One can view the shift
rate of the entire absorption band to the red as the average of the larger rate of the lowest exciton level and smaller rates of other levels that contribute to the Qy band. That the
exciton level lying lowest in energy tends to shift faster can be
qualitatively understood in terms of perturbative arguments involving
dispersion interactions, electrostatic and electron-exchange
interactions, and energy disorder. Support for this line of argument is
also provided by the observation that the broadening rate for the P960 special pair band of Rps. viridis, to which only one exciton
level contributes, is small, 0.02 cm
1/MPa
(Reddy et al., 1996Stark hole-burning studies
Stark hole burning of BChl c monomers in polymer films
That the hole broadening for BChl c monomers is independent of laser polarization suggests that the random contribution from the amorphous polymer matrix is the dominating factor in determining the BChl c Stark effect. The absence of a hole shift or asymmetrical hole broadening suggests that the quadratic Stark effect is negligible for the BChl c monomers. Using the theory of Kador et al. (1987)
µ at the center of the
absorption band is 0.35 D, which, within experimental uncertainty, is
equal to the value of 0.33 D for Chl a monomers obtained by
Stark hole-burning (Altmann et al., 1993
µ value of 0.6 D for Chl a monomers was
obtained by Small and co-workers (Rätsep et al., 2000
µ values for weakly coupled Chl a molecules
in photosynthetic complexes are ~0.6 D.
The polarizability change of BChl c can be estimated using
the following empirical formula, which was arrived at on the basis of
Stark hole-burning and solvent shift data for 11
-electron chromophores isolated in poly(vinyl butyral) (Altmann et al., 1993
|
(9) |

is
Å3. For Cb. tepidum, the two major
BChl c homologs found in the chlorosomes both have an ethyl
group at the 12 position, and each has a n-propyl and ethyl
group at the 18 position. The average molecular weight for these two
homologs is 608. We assume that the measured f
µ of 0.35 D contains only the matrix-induced component, because the laser
polarization-independent and symmetrical hole broadening suggests
little contribution from
µ0. With
f = 1.5 and MW = 608, Eq. 9 yields 
= 19 ± 2 Å3 for monomeric BChl c
molecules, which essentially is the same as the Chl a value
of 18 Å3 obtained by Altmann et al. (1993)Stark hole burning of isolated chlorosomes from Cb. tepidum
In contrast to BChl c monomers, no Stark effect was detected for the lowest exciton level of the chlorosome Qy band at the maximum field strength of 100 kV/cm. It should be emphasized that the relatively shallow saturated hole depths (usually less than ~0.05 fractional depth) and broad holewidths observed in chlorosomes (~2 cm
1,
compared with ~0.04 cm
1 for the BChl
c monomer) would hinder the observation of small Stark
effects. Previous studies by Blankenship and co-workers (Causgrove et
al., 1990
1 at 775 nm; results not shown). Experiments
were performed on whole cells of Cb. tepidum in the presence
of dithionite, but the results (holewidth = 1.6 cm
1 and fractional hole depth
0.04 at
777 nm) are similar to those of isolated chlorosome complexes. As for
the difficulties in obtaining deeper ZPHs in chlorosomes, there was
evidence (results not shown) suggesting that this may be due to partial
hole filling induced by the white light of the Fourier transform
spectrometer employed in the experiments. Holes with a fractional hole
depth of 0.1 have been reported for the lowest exciton level of
Cb. limicola detected in the fluorescence excitation mode
(Fetisova and Mauring, 1993
µ. Under the reasonable assumption that a minimum symmetrical hole broadening of 0.3 cm
1 is
necessary for the observation of the linear Stark effect at 100 kV/cm
on a hole with an initial holewidth of 2 cm
1,
f
µ must be less than 0.3 D (based on equation 15 of
Kador et al., 1987
µind, because Stark splitting was not
observed for laser polarization parallel or perpendicular to the
electric field Es; i.e.,
the molecular contribution f
µ0 to
0.35 D is small. It follows from exciton theory that
f
µ0 for the BChl c
aggregate cannot be larger than that of the monomer (Wu and Small,
1998
µ0. This possibility is
suggested by the paper of Wendt and Friedrich (1996)
µ0 of the J-aggregate relative to that of the monomer. It follows that a helical type structure could
also lead to a reduction in the value of

µind(nonrandom).
This brings us to the question of why

µind is no greater than ~0.3 D, given
that Frese et al. (1997)
2Tr(
) for chlorosomes is
1600 Å3 on the basis of classical Stark
modulation experiments at 77 K. With
Eint = 106 V/cm,
which is close to the values measured for polystyrene and n-hexane crystals (Kador et al., 1990
µind
5 D, which is a factor of ~10
greater than the upper limit determined above. An

µind of 5 D would have been easily
detected in our experiments. One explanation for this discrepancy is
that
µind is dominated by the nonrandom
contribution and that structural constraints, such as a helical
structure or a tubular arrangement (Buck and Struve, 1996
µ
signal was not observed in their Stark spectra. A second explanation
suggested in that work is that Eint is
small because of the low amount of protein residues near the BChl
c aggregate. A value of
Eint
105 V/cm would explain the absence of a linear
Stark effect in our experiments. Such a small value, however, seems
difficult to reconcile, given that it is an order of magnitude smaller
than those of polystyrene and n-hexane. A third possibility
is that 
of the lowest and weakly allowed exciton level probed by
Stark hole-burning is much smaller than those of the strongly allowed
levels, which dominate the optical responses in classical Stark
modulation spectroscopy. This possibility can be investigated using the
theory of Somsen et al. (1998)
|
(10) |
µ0 is small relative to
µind, which, given our results for BChl
c monomer, is a reasonable assumption. The above condition is not satisfied with Eint = 106 V/cm, because our maximum
Es value was 50 kV/cm (a value close to 1.5 is often used for
). Furthermore, it may not be satisfied even if Eint is as small as
105 V/cm.
| |
SUMMARY |
|---|
|
|
|---|
The strongly coupled nature of BChl c molecules in
chlorosomes was confirmed by the large linear pressure shift rate of
the Qy band (
0.44
cm
1/MPa) and the lowest exciton level (
0.54
cm
1/MPa) at low temperature. According to the
analysis presented, about half of the contribution to the shift rate is
from electron exchange interactions, which require a rather compact
arrangement of pigments. This important finding serves as a guideline
for electronic structure calculations of the chlorosome in the absence of knowing its exact structural arrangement of pigments.
The dipole moment change (f
µ) and polarizability change
(
) for the Qy transition of BChl
c monomers in a polymer film were determined to be 0.35 D
and 19 Å3, respectively.
µ is dominated by
the matrix-induced contribution. The absence of any Stark effect in the
lowest exciton level of chlorosomes led us to conclude that pigments in
chlorosomes possibly adopt certain structural constraints to attain
small dipole moments and polarizability changes. The basic tubular
models put forth by Buck and Struve (1996)
and Somsen et al. (1996)
, as
well as the helical structure proposed by Wendt and Friedrich (1996)
, are all in agreement with the Stark hole-burning results, as long as
the orientations of the pigments result in the reduction of
µ0 and 
ind.
| |
ACKNOWLEDGMENTS |
|---|
The authors thank Prof. Arvi Freiberg for critical comments on the manuscript.
Research at the Ames Laboratory was supported by the Division of Chemical Sciences, Office of Basic Energy Sciences, U.S. Department of Energy (USDOE). Ames Laboratory is operated for the USDOE by Iowa State University under contract W-7405-Eng82. Research at Arizona State University was supported by grant DE-FG03-97ER20267 from the Energy Biosciences program of the USDOE. Partial support for H-MW was provided by the Provost's Office at Arizona State University.
| |
FOOTNOTES |
|---|
Received for publication 10 January 2000 and in final form 1 June 2000.
Address reprint requests to Dr. Gerry J. Small, Department of Chemistry, Iowa State University, Ames, IA 50011. Tel.: 515-294-3859; Fax: 515-294-1699; E-mail: gsmall{at}ameslab.gov.
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REFERENCES |
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