Thermodynamic Limits Around M-dwarf Stars: Acknowledgements

Table of Links

• Abstract and Introduction
• 2 Methodology
• 2.1 Local spectral irradiance as a function of stellar temperature
• 2.2 Thermodynamic model of an oxygenic light-harvesting system
• 2.3 Lattice model of an oxygenic light-harvesting system
• 3 Results
• 3.1 Orbital distances and incident spectral fluxes
• 3.2 Thermodynamic antenna model: Increasing antenna size in limited PAR
• 3.3 Lattice antenna model: Increasing the size of a “flat” antenna in limited PAR
• 3.4 Lattice antenna model: Improving antenna efficiency with an energetic ’funnel’
• 4 Discussion
• Acknowledgements, Author Contribution Statement, Authors disclosure statement and References

5 Acknowledgements

CDPD and SC would like to acknowledge support from the BBSRC London Interdisciplinary Bioscience PhD Consortium (LIDo). Additionally, CDPD would like to acknowledge support from BBSRC for funding work (grant BB/T000023/1) that developed the key ideas in this work. TJH is funded by a Royal Society Dorothy Hodgkin Fellowship. EG gratefully acknowledges support from the UK Science and Technology Facilities Council (STFC; project reference ST/W001047/1).

6 Author Contribution Statement

CDPD, TJH and in discussion with EG and CWM, devised the project. TJH and EG provided stellar spectral data. Light-harvesting model development and simulations were carried out by CDPD and SC. TJH, EG and CWM provided additional interpretation of results. All authors were involved in Manuscript drafting.

7 Authors disclosure statement

There are no conflicts of interest to disclose.

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