Evolution of the disrupted material around the NS. Panel a: Z component of the angular momentum with respect to the distance to the NS for selected times. Panel b: distribution of gas mass with respect to the distance to the NS for selected times. The distance at which the WD is disrupted is shown by the black dashed line. Panel c: rate in M_⊙ s⁻¹ at which mass is accreted onto the gravitationally softened volume.