Rapid Evolution of the Photosystem II Electronic Structure during Water Splitting
Katherine M. Davis (1), Brendan T. Sullivan (1), Mark Palenik (1),, Lifen Yan (1), Vatsal Purohit (1), Gregory Robison (1), Irina Kosheleva (2),, Robert W. Henning (2), Gerald T. Seidler (3), Yulia Pushkar (1) ((1), Department of Physics, Astronomy, Purdue University

TL;DR
This study uses time-resolved X-ray emission spectroscopy to observe rapid changes in the Photosystem II Mn4Ca cluster during water splitting, proposing a new mechanism involving MnIV=O formation that clarifies the O-O bond formation process.
Contribution
It introduces a novel spectroscopic approach and proposes a new mechanism for oxygen evolution involving MnIV=O formation in the S3 state, advancing understanding of water oxidation.
Findings
Rapid (within 50 μs) changes in Mn Kβ XES spectrum during oxygen evolution.
No oxidation of Mn4Ca core above MnIV state before O-O bond formation.
Proposed mechanism where O-O bond formation occurs before the final electron transfer.
Abstract
Photosynthetic water oxidation is a fundamental process that sustains the biosphere. A MnCa cluster embedded in the photosystem II protein environment is responsible for the production of atmospheric oxygen. Here, time-resolved x-ray emission spectroscopy (XES) was used to observe the process of oxygen formation in real time. These experiments reveal that the oxygen evolution step, initiated by three sequential laser flashes, is accompanied by rapid (within 50 s) changes to the Mn K XES spectrum. However, no oxidation of the MnCa core above the all Mn state was detected to precede O-O bond formation. A new mechanism featuring Mn=O formation in the S state is proposed to explain the spectroscopic results. This chemical formulation is consistent with the unique reactivity of the S state and explains facilitation of the…
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