Exciton quenching by oxidized chlorophyll Z across the two adjacent monomers in a photosystem II core dimer

被引:1
|
作者
Mohamed, Ahmed [1 ,2 ]
Nishi, Shunsuke [3 ]
Kawakami, Keisuke [4 ]
Shen, Jian-Ren [5 ,6 ]
Itoh, Shigeru [3 ]
Fukumura, Hiroshi [1 ,7 ]
Shibata, Yutaka [1 ]
机构
[1] Tohoku Univ, Grad Sch Sci, Dept Chem, Aoba Ku, Sendai, Miyagi 9808578, Japan
[2] Inst Natl Rech Sci, Ctr Energie Mat Telecommun, 1650 Boul Lionel Boulet, Varennes, PQ J3X 1S2, Canada
[3] Nagoya Univ, Grad Sch Sci, Div Mat Sci Phys, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan
[4] RIKEN Spring 8 Ctr, Biostruct Mech Lab, Mikazuki, Hyogo 6795148, Japan
[5] Okayama Univ, Res Inst Interdisciplinary Sci, Okayama 7008530, Japan
[6] Okayama Univ, Grad Sch Nat Sci & Technol, Okayama 7008530, Japan
[7] Katholieke Univ Leuven, Dept Chem, Celestijnenlaan 200F, B-3001 Leuven, Belgium
关键词
Light harvesting; Temperature dependence; Time-resolved fluorescence spectroscopy; ANTENNA PROTEIN COMPLEX; LOWEST ELECTRONIC STATES; ENERGY-DISSIPATION; REACTION CENTERS; FLUORESCENCE; CP47; PHOTOOXIDATION; EXCITATIONS; RESOLUTION; MECHANISM;
D O I
10.1007/s11120-022-00948-1
中图分类号
Q94 [植物学];
学科分类号
071001 ;
摘要
This study aimed to clarify (1) which pigment in a photosystem II (PSII) core complex is responsible for the 695-nm emission at 77 K and (2) the molecular basis for the oxidation-induced fluorescence quenching in PSII. Picosecond time-resolved fluorescence dynamics was compared between the dimeric and monomeric PSII with and without addition of an oxidant. The results indicated that the excitation-energy flow to the 695-nm-emitting chlorophyll (Chl) at 36 K and 77 K was hindered upon monomerization, clearly demonstrating significant exciton migration from the Chls on one monomer to the 695-nm-emitting pigment on the adjacent monomer. Oxidation of the redox-active Chl, which is named Chl(Z) caused almost equal quenching of the 684-nm and 695-nm emission bands in the dimer, and lower quenching of the 695-nm band in the monomer. These results suggested two possible scenarios responsible for the 695-nm emission band: (A) Chl11-13 pair and the oxidized Chl(Z)D1 work as the 695-nm emitting Chl and the quenching site, respectively, and (B) Chl29 and the oxidized Chl(Z)D2 work as the 695-nm emitting Chl and the quenching site, respectively.
引用
收藏
页码:277 / 289
页数:13
相关论文
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