  We study the influence of black-hole evaporation on light propagation. The
framework employed is based on the non-linear QED effective action at one-loop
level. We show that the light-cone condition is modified for low-energy
radiation due to black-hole evaporation. We discuss conditions under which the
phase velocity of this low-energy radiation is greater than $c$. We also
compute the modified light-deflection angle, which turns out to be
significantly different from the standard GR value for black-hole masses in the
range $M_\text{Pl} \ll M \lesssim 10^{19}\;M_\text{Pl}$.
