“…The advantage of our scaling is that it yields an asymptotic description for solutions of order O(1) in L ∞ on macroscopic spacetime scales, in contrast to the setting of [1,17], in which the size of the solution varies as ε → 0. Another advantage is that this scaling puts us firmly in the regime of weakly nonlinear, semi-classical NLS with highly oscillatory periodic potentials, which have been extensively studied in, e.g., [5,6,7,8,19], albeit not for the case of honeycomb lattices. From the mathematical point of view, the present work will follow the ideas presented in [19] and adapt them to the current situation.…”