Casazza Anna Paola, Szczepaniak Malwina, Müller Marc G, Zucchelli Giuseppe, Holzwarth Alfred R
CNR-Istituto di Biofisica, Dipartimento di Biologia, Universita; degli Studi di Milano, Milan, Italy.
Biochim Biophys Acta. 2010 Sep;1797(9):1606-16. doi: 10.1016/j.bbabio.2010.05.008. Epub 2010 May 19.
The energy equilibration and transfer processes in the isolated core antenna complexes CP43 and CP47 of photosystem II have been studied by steady-state and ultrafast (femto- to nanosecond) time-resolved spectroscopy at room temperature. The annihilation-free femtosecond absorption data can be described by surprisingly simple sequential kinetic models, in which the excitation energy transfer between blue and red states in both antenna complexes is dominated by sub-picosecond processes and is completed in less than 2ps. The slowest energy transfer steps with lifetimes in the range of 1-2ps are assigned to transfer steps between the chlorophyll layers located on the stromal and lumenal sides. We conclude that these ultrafast intra-antenna energy transfer steps do not represent a bottleneck in the rate of the primary processes in intact photosystem II. Since the experimental energy equilibration rates are up to a factor of 3-5 higher than concluded previously, our results challenge the conclusions drawn from theoretical modeling.
通过在室温下的稳态和超快(飞秒至纳秒)时间分辨光谱,对光系统II中分离的核心天线复合物CP43和CP47的能量平衡和转移过程进行了研究。无湮灭飞秒吸收数据可以用令人惊讶的简单顺序动力学模型来描述,其中两个天线复合物中蓝色和红色状态之间的激发能量转移由亚皮秒过程主导,并在不到2皮秒内完成。寿命在1 - 2皮秒范围内最慢的能量转移步骤被归因于位于基质侧和腔侧的叶绿素层之间的转移步骤。我们得出结论,这些超快的天线内能量转移步骤并不代表完整光系统II初级过程速率的瓶颈。由于实验测得的能量平衡速率比之前推断的高出3 - 5倍,我们的结果对从理论建模得出的结论提出了挑战。