Geometric explanation of strong trajectory separation
Determine whether strong separation of neighboring fluid trajectories in the pressure-induced effective curved space arises from a local alignment of the velocity vector with an eigenvector of the Riemann curvature tensor, such that the particle closely shadows a particular geodesic while neighboring particles do not.
References
Building upon this picture, strong separation may arise from a parallelism effect. When the local velocity vector aligns with an eigenvector of the Riemann tensor, the particle closely shadows a particular geodesic, so that its deviation from that geodesic is reduced, whereas neighboring particles do not. As a result, the relative separation between them is enhanced. Such an interpretive conjecture is consistent with the observation of \citet{haller2012geodesic} that the locally most compressing or most shearing material lines are closely shadowed by least-stretching geodesics of the metric induced by the Cauchy-Green strain tensor.