“…Simultaneously, simulations have been performed for a large variety of samples with different models. These can be based on rate equations for the electron densities, 3,4 Monte-Carlo simulations of the Boltzmann equation for the occupations of the k-states in the individual subbands, [5][6][7][8] density matrix calculations, [9][10][11][12][13] which have been also done k-resolved, 7,14,15 as well as nonequilibrium Green's functions (NEGF). [16][17][18][19][20] While the published results from either scheme typically agree well with experimental data, it is not clear how the choices of parameters (in particular, interface roughness (IFR) distributions and band offsets), specific approximations (such as screening models or various model-specific assumptions as subband temperatures), or model complexity affect the results.…”