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High-Pressure and Stark Hole-Burning Studies of Chlorosome Antennas from Chlorobium tepidum
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...
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Published in: | Biophysical journal 2000-09, Vol.79 (3), p.1561-1572 |
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Main Authors: | , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | 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 Q
y-band at 100
K and the lowest Q
y-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, ƒΔ
μ
=
0.35 D, where Δ
μ is the dipole moment change for the Q
y transition and ƒ is the local field correction factor. The data establish that Δ
μ is dominated by the matrix-induced contribution. The change in polarizability (Δ
α) for the Q
y transition of the BChl
c monomer is estimated at 19
Å
3, 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 10
5
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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ISSN: | 0006-3495 1542-0086 |
DOI: | 10.1016/S0006-3495(00)76407-1 |