Excitonic energy transfer in red algal Photosystem I reveals an evolutionary bridge between cyanobacteria and plants

M Mengyuan Cui (Department of Physics, School of Physical Science and Technology, Ningbo University) Z Zihui Liu (Department of Physics, School of Physical Science and Technology) M Miriam Izzo (Solar Fuels Laboratory, Center of New Technologies, University of Warsaw) J Junhua Zhou (Department of Physics, School of Physical Science and Technology) E Enhu He (Department of Physics, School of Physical Science and Technology, Ningbo University) V Vandana Tiwari P Petar H. Lambrev (Biological Research Centre) R R. J. Dwayne Miller (Departments of Chemistry and Physics, University of Toronto, 80 St. George Street, Toronto, ON M5S3H6, Canada) J Joanna Kargul (Solar Fuels Laboratory, Center of New Technologies, University of Warsaw) F Fulu Zheng (Department of Physics, School of Physical Science and Technology) A Ajay Jha (Rosalind Franklin Institute) H Hong-Guang Duan (Department of Physics, School of Physical Science and Technology)

Abstract

Photosystem I (PSI) converts light into chemical energy with near-unity quantum efficiency, yet its energy-transfer and charge-separation mechanisms remain debated. Evolution has diversified PSI architectures: Cyanobacterial PSI trimers confine red-shifted pigments to the core, whereas plant PSI-Light Harvesting Complex Isupercomplexes incorporate extensive peripheral red and charge-transfer states that reshape trapping. The unicellular red alga Cyanidioschyzon merolae exemplifies functional diversification across distinct evolutionary branches, combining a photosystem II and plant-like monomeric PSI core associated with a varying number of light harvesting antenna subunits, Light Harvesting Complexes from Red Lineage (LHCR). This hybrid organization functionally bridges mechanistic models across different lineages. We applied two-dimensional electronic spectroscopy at ultralow temperatures (8 and 80 K) to disentangle overlapping excitation pathways in C. merolae PSI. Cryogenic measurements suppressed thermal broadening, resolving five dynamical components: subpicosecond equilibration (0.3 to 0.8 ps) across the core–LHCR interface, subsequent population transfer (2.6 to 4 ps) into progressively lower-energy manifolds, and slower feeding (18 to 53 ps) into red pools distributed across both core and antenna. On the longest timescales (hundreds of ps), a persistent ground-state bleach signifies excitons stabilized in terminal sinks. Notably, comparison of 8 K and 80 K spectra reveals that excitations are heterogeneously partitioned among multiple sinks at low disorder, whereas modest thermal activation (kT ∼ 55 cm −1 ) promotes selective convergence into core-associated red chlorophylls. Atomistic excitonic modeling with time-nonlocal master equations supports these observations, revealing temperature-dependent energy redistribution. Overall, C. merolae PSI expands the kinetic funnel by distributing trapping sites, enhancing spectral coverage while maintaining high efficiency, which is an important functional diversification during evolution.

Article Details

Volume / Issue Vol. 123, Issue 30
Published July 28, 2026
ISSN 0027-8424
Publisher National Academy of Sciences

Authors (12)

M

Mengyuan Cui

Department of Physics, School of Physical Science and Technology, Ningbo University

Z

Zihui Liu

Department of Physics, School of Physical Science and Technology

M

Miriam Izzo

Solar Fuels Laboratory, Center of New Technologies, University of Warsaw

J

Junhua Zhou

Department of Physics, School of Physical Science and Technology

E

Enhu He

Department of Physics, School of Physical Science and Technology, Ningbo University

V

Vandana Tiwari

P

Petar H. Lambrev

Biological Research Centre

R

R. J. Dwayne Miller

Departments of Chemistry and Physics, University of Toronto, 80 St. George Street, Toronto, ON M5S3H6, Canada

J

Joanna Kargul

Solar Fuels Laboratory, Center of New Technologies, University of Warsaw

F

Fulu Zheng

Department of Physics, School of Physical Science and Technology

A

Ajay Jha

Rosalind Franklin Institute

H

Hong-Guang Duan

Department of Physics, School of Physical Science and Technology