Figure shows the coherence distributions for k0 = 30 au at the corresponding time steps. As shown in Figures , 4B and 4E, all investigated methods produce highly accurate results in the short-time dynamics. After the WPs pass through the second interaction region (see Figures and), the oscillating phases of the coherence distribution by FSSH-wf are slightly shifted compared to those in the quantum reference, while the amplitudes show more significant deviations. In contrast, both BCSH-wf and BCSH-as are capable of predicting the same oscillating phases as the quantum reference due to the consideration of phase correction. Notably, BCSH-as also produces more accurate oscillating amplitudes as expected.