for power-law corrections.
For the sake of clarity in what follows we split the analysis
for the two classes of entropy corrections, but in this section we
will only consider perfect fluids assuming that the dominant energy
condition (DEC) holds true (i.e., ρ + P/c2 > 0) all along the
expansion. Then, in view of Eq. (13) the GSL is satisfied provided
F(H) is non-negative which occurs only for some values of the
parameter α. In all the cases the results of general relativity [18]
are recovered, as it should, by setting α = 0.