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Thermodynamic Limits Around M-dwarf Stars: Increasing the Size of a “flat” Antenna in Limited PAR by@photosynthesis

Thermodynamic Limits Around M-dwarf Stars: Increasing the Size of a “flat” Antenna in Limited PAR

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In this study, researchers explore the feasibility and potential characteristics of photosynthetic light-harvesting on exo-planets.
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(1) Samir Chitnavis, School of Biological and Behavioural Sciences, Queen Mary University of London, Mile End, London E1 4NS, UK & Digital Environment Research Institute, Queen Mary University of London, Empire House, Whitechapel E1 1HH, UK; (2) Thomas J. Haworth, Astronomy Unit, Queen Mary University of London, Mile End Road, London E1 4NS, UK; (3) Edward Gillen, Astronomy Unit, Queen Mary University of London, Mile End Road, London E1 4NS, UK; (4) Conrad W. Mullineaux, School of Biological and Behavioural Sciences, Queen Mary University of London, Mile End, London E1 4NS, UK;

(5) Christopher D. P. Duffy, School of Biological and Behavioural Sciences, Queen Mary University of London, Mile End, London E1 4NS, UK & Digital Environment Research Institute, Queen Mary University of London, Empire House, Whitechapel E1 1HH, UK (Email: [email protected]).

3.3 Lattice antenna model: Increasing the size of a “flat” antenna in limited PAR


This paper is under CC 4.0 license.


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