The solar cell equation is derived (Section 2) in terms of transition
probabilities and this leads to a consideration of the principle of de
tailed balance, and also of the extent to which it is justifiable to a
ssume that the transition probabilities involved are excitation-indepe
ndent. A fuller discussion, with some applications, is then given of d
etailed balance (Section 3). If it cannot be applied, it may still be
justifiable to adopt the weaker steady-state assumption, backed up by
the hypothesis of quasi-Fermi levels. This can lead (Section 4) to pho
ton distributions with a non-zero chemical potential (which is imposed
on the photons by the fermions). A more general discussion of some st
atistical mechanical principles is also given (Section 5).