SPECTRAL EQUILIBRATION AND PRIMARY PHOTOCHEMISTRY IN HELIOBACILLUS-MOBILIS AT CRYOGENIC TEMPERATURE

Citation
U. Liebl et al., SPECTRAL EQUILIBRATION AND PRIMARY PHOTOCHEMISTRY IN HELIOBACILLUS-MOBILIS AT CRYOGENIC TEMPERATURE, Biochemistry, 36(19), 1997, pp. 5912-5920
Citations number
46
Categorie Soggetti
Biology
Journal title
ISSN journal
00062960
Volume
36
Issue
19
Year of publication
1997
Pages
5912 - 5920
Database
ISI
SICI code
0006-2960(1997)36:19<5912:SEAPPI>2.0.ZU;2-I
Abstract
We performed multicolor femtosecond transient absorption measurements on membranes of the photosynthetic bacterium Heliobacillus mobilis at 20 K, by selective excitation at either the red or the blue extreme of the bacteriochlorophyll g Q(y) band, which is split in three spectral forms (Bchl g 778, 793, and 808) at low temperature. In contrast to r oom temperature, there is no observable uphill energy transfer upon ex citation at the red extreme. This provides a direct experimental confi rmation of the expected strong temperature dependence of uphill energy transfer in multichromophore systems. Upon excitation at the blue edg e, downhill energy transfer is observed on time ranges varying over 2 orders of magnitude and is discussed in terms of four distinct energy transfer processes: Bchl g 778 --> Bchl g 793* (similar to 50 fs);Bch l g 778 --> Bchl g 808* (similar to 400 fs); Bchl g 793* --> Bchl g 8 08 (similar to 1.4 ps); and within Bchl g 808* (similar to 7 ps). Sur prisingly, the amount of oxidized primary donor P798(+) formed on the time scale of picoseconds and tens of picoseconds was found to depend on the excitation conditions: trapping occurs mainly in similar to 80 ps and slower from directly excited Bchl g 808 and can additionally o ccur in a few picoseconds from Bchl g 778 and Bchl g 793* upon blue e xcitation. This finding implies that spectral equilibration is not com plete prior to charge separation and furthermore is inconsistent with a funnel model, in which P798 is surrounded by long-wavelength pigment s. More generally, we discuss to what extent our data bring constraint s on the spatial distribution of the different spectral forms of the p igments.