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Related papers: Smaller alignment index (SALI): Determining the or…

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We use the Smaller Alignment Index (SALI) to distinguish rapidly and with certainty between ordered and chaotic motion in Hamiltonian flows. This distinction is based on the different behavior of the SALI for the two cases: the index…

Chaotic Dynamics · Physics 2008-11-26 Ch Skokos , Ch Antonopoulos , T C Bountis , M N Vrahatis

The Smaller Alignment Index (SALI) is a very useful and efficient indicator that can distinguish rapidly and with certainty between ordered and chaotic motion in Hamiltonian systems. This is based on the different behavior of the SALI in…

Chaotic Dynamics · Physics 2010-08-17 Ch. Antonopoulos , T. Manos , Ch. Skokos

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…

Accelerator Physics · Physics 2008-11-26 T. Bountis , Ch. Skokos

The ability of the Smaller Alignment Index (SALI) to distinguish chaotic from ordered motion, has been demonstrated recently in several publications.\cite{Sk01,GRACM} Basically it is observed that in chaotic regions the SALI goes to zero…

Chaotic Dynamics · Physics 2016-09-08 Ch. Skokos , Ch. Antonopoulos , T. C. Bountis , M. N. Vrahatis

We use the Smaller ALignment Index (SALI) method of chaos detection, to study the global dynamics of conservative dynamical systems described by differential or difference equations. In particular, we consider the well--known 2 and…

Chaotic Dynamics · Physics 2014-11-18 T. Manos , Ch. Skokos , E. Athanassoula , T. Bountis

We provide a concise presentation of the Smaller (SALI) and the Generalized Alignment Index (GALI) methods of chaos detection. These are efficient chaos indicators based on the evolution of two or more, initially distinct, deviation vectors…

Chaotic Dynamics · Physics 2015-06-02 Ch. Skokos , T. Manos

A very important issue in the area of galactic dynamics is the detection of chaotic and ordered motion inside galaxies. In order to achieve this target, we use the Smaller ALignment Index (SALI) method, which is a very suitable tool for…

Astrophysics · Physics 2007-05-23 T. Manos , E. Athanassoula

The chaotic or ordered character of orbits in galactic models is an important issue, since it can influence dynamical evolution. This distinction can be achieved with the help of the Smaller Alingment Index - (SALI). We describe here…

Astrophysics · Physics 2009-11-11 T. Manos , E. Athanassoula

We use a simple dynamical model in order to investigate the regular or chaotic character of orbits in a barred galaxy with a central, spherically symmetric, dense nucleus and a flat disk. In particular, we explore how the total orbital…

Astrophysics of Galaxies · Physics 2017-09-28 Euaggelos E. Zotos

We study the dynamics of 2D and 3D barred galaxy analytical models, focusing on the distinction between regular and chaotic orbits with the help of the Smaller ALigment Index (SALI), a very powerful tool for this kind of problems. We…

Astrophysics · Physics 2013-03-26 T. Manos , E. Athanassoula

The dynamical evolution of barred galaxies depends crucially on the fraction and their spacial distribution of chaotic orbits in them. In order to distinguish between the two kinds of orbits, we use the Smaller Alignment Index (SALI)…

Astrophysics · Physics 2007-05-23 T. Manos , E. Athanassoula

The distinction between chaotic and regular behavior of orbits in galactic models is an important issue and can help our understanding of galactic dynamical evolution. In this paper, we deal with this issue by applying the techniques of the…

Astrophysics of Galaxies · Physics 2015-05-27 T. Manos , E. Athanassoula

We present a new dynamical model describing 3D motion in non axially symmetric galaxies. The model covers a wide range of galaxies from a disk system to an elliptical galaxy by suitably choosing the dynamical parameters. We study the…

Astrophysics of Galaxies · Physics 2014-02-18 Euaggelos E. Zotos , Nicolaos D. Caranicolas

The regular or chaotic character of orbits of stars moving in the meridional plane (R,z) of an axially symmetric elliptical galaxy with a dense, massive spherical nucleus and a dark matter halo component is under investigation. In…

Astrophysics of Galaxies · Physics 2017-09-28 Euaggelos E. Zotos , Nicolaos D. Caranicolas , Efthimia G. Doni

The H\'{e}non-Heiles potential is undoubtedly one of the most simple, classical and characteristic Hamiltonian systems. The aim of this work is to reveal the influence of the value of the total orbital energy, which is the only parameter of…

Chaotic Dynamics · Physics 2017-09-28 Euaggelos E. Zotos

We introduce a new methodology for a fast and reliable discrimination between ordered and chaotic orbits in multidimensional Hamiltonian systems which we call the Linear Dependence Index (LDI). The new method is based on the recently…

Chaotic Dynamics · Physics 2007-11-05 Chris Antonopoulos , Tassos Bountis

We present and validate simple and efficient methods to estimate the chaoticity of orbits in low dimensional dynamical systems from computations of Lagrangian descriptors (LDs) on short time scales. Two quantities are proposed for…

As originally formulated, the Generalized Alignment Index (GALI) method of chaos detection has so far been applied to distinguish quasiperiodic from chaotic motion in conservative nonlinear dynamical systems. In this paper we extend its…

Chaotic Dynamics · Physics 2013-10-17 T. Manos , Ch. Skokos , Ch. Antonopoulos

Understanding the dynamics of multi--dimensional conservative dynamical systems (Hamiltonian flows or symplectic maps) is a fundamental issue of non-linear science. The Generalized ALignment Index (GALI), which was recently introduced and…

Chaotic Dynamics · Physics 2013-03-26 T. Manos , Ch. Skokos , T. Bountis

The case of the classical Hill problem is numerically investigated by performing a thorough and systematic classification of the initial conditions of the orbits. More precisely, the initial conditions of the orbits are classified into four…

Chaotic Dynamics · Physics 2017-07-07 Euaggelos E. Zotos
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