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The wavelength of the incident light determines the primary charge separation pathway in Photosystem II

Charge separation is a key component of the reactions cascade of photosynthesis, by which solar energy is converted to chemical energy. From this photochemical reaction, two radicals of opposite charge are formed, a highly reducing anion and a highly oxidising cation. We have previously proposed tha...

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Autores principales: Pavlou, Andrea, Jacques, Julien, Ahmadova, Nigar, Mamedov, Fikret, Styring, Stenbjörn
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2018
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5809461/
https://www.ncbi.nlm.nih.gov/pubmed/29434283
http://dx.doi.org/10.1038/s41598-018-21101-w
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author Pavlou, Andrea
Jacques, Julien
Ahmadova, Nigar
Mamedov, Fikret
Styring, Stenbjörn
author_facet Pavlou, Andrea
Jacques, Julien
Ahmadova, Nigar
Mamedov, Fikret
Styring, Stenbjörn
author_sort Pavlou, Andrea
collection PubMed
description Charge separation is a key component of the reactions cascade of photosynthesis, by which solar energy is converted to chemical energy. From this photochemical reaction, two radicals of opposite charge are formed, a highly reducing anion and a highly oxidising cation. We have previously proposed that the cation after far-red light excitation is located on a component different from P(D1), which is the location of the primary electron hole after visible light excitation. Here, we attempt to provide further insight into the location of the primary charge separation upon far-red light excitation of PS II, using the EPR signal of the spin polarized (3)P(680) as a probe. We demonstrate that, under far-red light illumination, the spin polarized (3)P(680) is not formed, despite the primary charge separation still occurring at these conditions. We propose that this is because under far-red light excitation, the primary electron hole is localized on Chl(D1), rather than on P(D1). The fact that identical samples have demonstrated charge separation upon both far-red and visible light excitation supports our hypothesis that two pathways for primary charge separation exist in parallel in PS II reaction centres. These pathways are excited and activated dependent of the wavelength applied.
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spelling pubmed-58094612018-02-15 The wavelength of the incident light determines the primary charge separation pathway in Photosystem II Pavlou, Andrea Jacques, Julien Ahmadova, Nigar Mamedov, Fikret Styring, Stenbjörn Sci Rep Article Charge separation is a key component of the reactions cascade of photosynthesis, by which solar energy is converted to chemical energy. From this photochemical reaction, two radicals of opposite charge are formed, a highly reducing anion and a highly oxidising cation. We have previously proposed that the cation after far-red light excitation is located on a component different from P(D1), which is the location of the primary electron hole after visible light excitation. Here, we attempt to provide further insight into the location of the primary charge separation upon far-red light excitation of PS II, using the EPR signal of the spin polarized (3)P(680) as a probe. We demonstrate that, under far-red light illumination, the spin polarized (3)P(680) is not formed, despite the primary charge separation still occurring at these conditions. We propose that this is because under far-red light excitation, the primary electron hole is localized on Chl(D1), rather than on P(D1). The fact that identical samples have demonstrated charge separation upon both far-red and visible light excitation supports our hypothesis that two pathways for primary charge separation exist in parallel in PS II reaction centres. These pathways are excited and activated dependent of the wavelength applied. Nature Publishing Group UK 2018-02-12 /pmc/articles/PMC5809461/ /pubmed/29434283 http://dx.doi.org/10.1038/s41598-018-21101-w Text en © The Author(s) 2018 Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.
spellingShingle Article
Pavlou, Andrea
Jacques, Julien
Ahmadova, Nigar
Mamedov, Fikret
Styring, Stenbjörn
The wavelength of the incident light determines the primary charge separation pathway in Photosystem II
title The wavelength of the incident light determines the primary charge separation pathway in Photosystem II
title_full The wavelength of the incident light determines the primary charge separation pathway in Photosystem II
title_fullStr The wavelength of the incident light determines the primary charge separation pathway in Photosystem II
title_full_unstemmed The wavelength of the incident light determines the primary charge separation pathway in Photosystem II
title_short The wavelength of the incident light determines the primary charge separation pathway in Photosystem II
title_sort wavelength of the incident light determines the primary charge separation pathway in photosystem ii
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5809461/
https://www.ncbi.nlm.nih.gov/pubmed/29434283
http://dx.doi.org/10.1038/s41598-018-21101-w
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