2012
DOI: 10.1007/s10569-012-9418-y
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Diversity and validity of stable-unstable transitions in the algorithmic weak stability boundary

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Cited by 11 publications
(8 citation statements)
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“…Generally speaking, DEMR performs better than all of the algorithms except SHADE. Among the 25 test functions, DEMR is significantly better than CMA-ES, LBBO, GL-25, SaDE, MPEDE, and SHADE in 15,11,16,12,10, and 9 functions, respectively, while the numbers of functions where CMA-ES, LBBO, GL-25, SaDE, MPEDE, and SHADE perform significantly better are 6, 7, 6, 10, 8, and 13. And for the remaining functions, DEMR provides error values comparable to those of the compared algorithms.…”
Section: Experiments On Benchmarkmentioning
confidence: 96%
See 1 more Smart Citation
“…Generally speaking, DEMR performs better than all of the algorithms except SHADE. Among the 25 test functions, DEMR is significantly better than CMA-ES, LBBO, GL-25, SaDE, MPEDE, and SHADE in 15,11,16,12,10, and 9 functions, respectively, while the numbers of functions where CMA-ES, LBBO, GL-25, SaDE, MPEDE, and SHADE perform significantly better are 6, 7, 6, 10, 8, and 13. And for the remaining functions, DEMR provides error values comparable to those of the compared algorithms.…”
Section: Experiments On Benchmarkmentioning
confidence: 96%
“…This type of low-energy transfer trajectory is mainly achieved by taking advantage of the invariant manifold structures associated with the 3D halo orbits (or 2D Lyapunov orbits) in the vicinity of the libration points in the Sun-Earth system and Earth-Moon system and can be modelled as two coupled CR3BPs. In fact, the Japanese Hiten mission was a paradigmatic example for a class of low-energy Earth-to-Moon orbits obtained by considering the gravitational effects of the Earth, the Moon, and the Sun on the motion of the spacecraft simultaneously [8,9,14,15] and was later found to be related to the hyperbolic invariant manifolds of the CR3BP by employing the patched threebody approximation [5,16,17]. G贸mez et al [18] had also presented the use of the restricted three-body problem's invariant manifold structural to design the low-energy transfer orbit in detail.…”
Section: Introductionmentioning
confidence: 99%
“…Otherwise the point is redeemed as unstable. (Some of these ideas are also suggested in [11].) The main result of this paper is that the WSB points, which make the transition from the weakly stable to the weakly unstable regime, are the points on the stable manifold of the Lyapunov orbit for the corresponding energy level.…”
Section: Introductionmentioning
confidence: 94%
“…We remark that, since the stability/instability criteria, as described above, are concerned with the behavior of trajectories for finite time, they inherently introduce 'artifacts', i.e., points with very similar trajectories that are categorized differently with respect to these criteria. See [4,11].…”
Section: Introductionmentioning
confidence: 99%
“…The Weak Stability Boundary 鈭俉 can therefore be introduced: it identifies the separatrix between those points in the phase space leading to capture orbits and those leading to different behaviours, such as escape orbits. In order to identify an initial point on the WSB, a bisection method defined in polar coordinates has been here implemented, as discussed in Topputo and Belbruno (2009): the possible Cantor-like structure of the Stable Set, discussed in Sousa and Terra (2012), has been here neglected. This work is focused on the identification of the closure of both the Stable Set (i.e., the Weak Stability Boundary), and of the Unstable Set.…”
Section: Ballistic Capturementioning
confidence: 99%