Justification for using effective radiation temperature Ty in Carnot efficiency and Boltzmann factor
Establish a rigorous justification for substituting the wavelength-dependent, non-equilibrium effective radiation temperature Ty(1) into the Carnot efficiency formula nmax = 1 − Tout/Ty(1) and into the Boltzmann factor exp(−ΔE/kBTy(2)) when analyzing photosynthetic light-powered systems, or determine the precise conditions under which these substitutions are valid, given that Ty(1) does not correspond to an equilibrium temperature.
References
Although this effective temperature has been widely used in the physicochemical analysis of the theoretical efficiency of photosynthesis, certain questions and critical discussions remain unresolved [17-21, 26-33]. These questions [21,24,27,33] stem mainly from the fact that this temperature Ty (1), which is not in equilibrium (i.e., not a true temperature), is automatically applied to Carnot efficiency and Boltzmann factor formulae, as nmax = 1 -Tout/Ty(1) and exp(-AE/kBTy(2)), respectively, without proper justification.