We have determined the marginal stability curve of convective instability i
n the usual Rayleigh-Benard configuration with radiative transfer and a fix
ed total heat flux at the boundaries instead of a fixed temperature. In the
Milne-Eddington approximation, radiative transfer introduces a new length
scale and breaks the invariance of the Boussinesq equations under an arbitr
ary temperature shift, which occurs when the heat flux is fixed at the boun
daries. The convergence to the limits where the non-radiative cases are exp
ected is studied in this approximation. Then, using a second-order perturba
tive calculation, we show that the presence of radiation can change qualita
tively the instability pattern: there is a range of optical parameters wher
e the Cahn-Hillard equation is not anymore the one appropriate to describe
the instability near the threshold. (C) 2001 Published by Elsevier Science
B.V.