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Thermodynamic limits around M-dwarf stars: Improving antenna efficiency with an energetic ’funnel’by@photosynthesis

Thermodynamic limits around M-dwarf stars: Improving antenna efficiency with an energetic ’funnel’

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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]).

3.4 Lattice antenna model: Improving antenna efficiency with an energetic ’funnel’


This paper is available on arxiv under CC 4.0 license.