Cluster surface tension, σ (top panel), proton fraction in the dense phase, $y_p^I$ (middle panel), and global proton fraction, y_p (bottom panel) in the inner crust at T = 1 MeV as a function of the total baryon density, ρ, obtained for β-equilibrated matter (thick lines) and matter with fixed proton fraction y_p = 0.3 (thin lines in the top and middle panels) for all models considered in this work. The results are obtained without the translational term and the surface parameters are obtained from the fit to the mass table AME2016 (Audi et al. 2017).