“…Although the computation of the mLCE is the most widely used technique for characterizing the regular or chaotic nature of orbits, its computational drawbacks, like for example its slow convergence to its limiting value, led to the development of a number of other, efficient chaos detection techniques, which make use of the solutions of the variational equations, like for example the fast Lyapunov indicator (FLI) and its variants [79,80,81,82,83,84], the mean exponential growth of nearby orbits (MEGNO) [85,86,87], the relative Lyapunov indicator (RLI) [88,89,90], the smaller alignment index (SALI) [91,92,93] and its generalization, the GALI [74,75,76,94].…”