Migration of Electronic Energy from Chlorophyll b to Chlorophyll a in Solutions
Absorption, emission, and fluorescence excitation spectra of pure solutions of chlorophyll a (Chl a) and chlorophyll b (Chl b) in diethyl ether and of equimolecular mixed solutions of the two pigments, were determined at room temperature as functions of concentration (in the range from 5 × 10 -6 M t...
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Veröffentlicht in: | Biophysical journal 1972-07, Vol.12 (7), p.731-745 |
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Sprache: | eng |
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Zusammenfassung: | Absorption, emission, and fluorescence excitation spectra of pure solutions of chlorophyll
a (Chl
a) and chlorophyll
b (Chl
b) in diethyl ether and of equimolecular mixed solutions of the two pigments, were determined at room temperature as functions of concentration (in the range from 5
×
10
-6 M to 4
×
10
-3 M) and of wavelength of the exciting light (in the regions 380–465 and 550–650 nm). The efficiency of energy transfer from Chl
b to Chl
a, derived from these data, was found to depend on the wavelength of exciting light. Furthermore, the transfer efficiency calculated from sensitization of Chl
a fluorescence by Chl
b was substantially smaller than that calculated from quenching of Chl
b fluorescence by Chl
a. Both these effects are tentatively explained as evidence of superposition of a “fast” energy transfer (taking place
before the Boltzmann distribution of vibrational energy had been reached) upon the “delayed” transfer, which takes place
after vibrational equilibration. The first-named mechanism is made possible by overlapping of the absorption bands of the two pigments; the second, by overlapping of the emission band of Chl
b and the absorption band of Chl
a. The first mechanism can lead to repeated transfer of excitation energy between pigment molecules, the second only to a one-time transfer from the donor to the acceptor. Both mechanisms could be of the same, second-order type, with the transfer rate proportional to
r
-6. An alternative is for the fast mechanism to be of the first order, with the transfer rate proportional to
r
-3, but spectroscopic evidence seems to make this alternative less probable. |
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ISSN: | 0006-3495 1542-0086 |
DOI: | 10.1016/S0006-3495(72)86117-4 |