Time evolution of the individual accretion rate (first and second row) and the relative precession phase between the disc and the binary (ϖ = ϖ_d − ϖ_b; third and last row) for the equal mass circular case e = 0, q = 1 (left column); e = 0.45, q = 0.7 (middle column); and the equal mass highly eccentric one e = 0.9, q = 1 (right column). The first two rows show the accretion onto the primary (green line) and the secondary (pink line) black hole over the last 400 and 200 orbits for the equal and unequal mass cases, respectively. The upper row shows the results of simulations without the radiation pressure, while the second row includes the radiation pressure. The third and last row display the evolution of the relative precession phase over the radius. The third row shows results without radiation pressure, and the last row includes it.