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A Few More General Topics Thermodynamic Efficiency

A system receives energy and entropy from a pump and emits energy and entropy into surroundings at steady rates E, S, E, S, It also emits heat and performs work at steady rates Q, W. [Pg.55]

We first check that this formula for a thermodynamically maximal temperature yields the Carnot efficiency. As heat transfer is included explicitly in the formulae, we simply remove the sink (E = S =0) and associate a temperature T E E /S with ss PP P [Pg.55]

Next we take black-body radiation to be the pump, and regard black-body radiation as emitted, Then we may put [Pg.55]

Both limits are shared by the Carnot efficiency, but (between these limits) the new efficiency lies lower. It is still unrealistically high, however, [Pg.56]

A further reduction may be achieved by assuming radiation to pass in sequence through n ideal solar cells of decreasing band gaps so that longer wavelengths are absorbed later. At the same time each cell emits radiation to keep in a steady state and this is absorbed by the two neighbouring cells. This radiation becomes important as n - , since for many cells the photons [Pg.56]




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