Application of the SALI chaos detection method to accelerator mappings
| dc.creator | Bountis, T. | |
| dc.creator | Skokos, Ch. | |
| dc.date | 2005-12-13 | |
| dc.date.accessioned | 2026-07-07T10:47:02Z | |
| dc.date.available | 2026-07-07T10:47:02Z | |
| dc.description | We apply the Smaller ALignment Index (SALI) method to a 4--dimensional mapping of accelerator dynamics in order to distinguish rapidly, reliably and accurately between ordered and chaotic motion. The main advantage of this index is that it tends {\it exponentially} to zero in the case of chaotic orbits, while it fluctuates around non--zero values in the case of quasiperiodic trajectories. Thus, it avoids the notorious ambiguities concerning the eventual convergence of (maximum) Lyapunov exponents to (positive) non-zero values. Exploiting the different behavior of SALI in these two cases we produce phase space `charts' where regions of chaos and order are clearly identified. Evaluating the percentage of chaotic and escaping orbits as a function of the distance from the origin we are able to estimate rapidly and accurately the boundaries of the {\it dynamical aperture} of a proton beam, passing repeatedly through an array of magnetic focusing elements. | |
| dc.description | 7 pages, 6 figures, to appear in 'Nuclear Instruments and Methods in Physics Research - Section A' | |
| dc.identifier | https://arxiv.org/abs/physics/0512115 | |
| dc.identifier | http://arxiv.org/abs/physics/0512115 | |
| dc.identifier | Nucl.Instrum.Meth.A561:173-179,2006 | |
| dc.identifier | doi:10.1016/j.nima.2006.01.009 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/183433 | |
| dc.subject | Accelerator Physics | |
| dc.subject | Astrophysics | |
| dc.subject | Chaotic Dynamics | |
| dc.title | Application of the SALI chaos detection method to accelerator mappings | |
| dc.type | text |