activity
20052023
most citedRegular and chaotic orbits in barred galaxies - I. Applying the SALI/GALI method to explore their distribution in several models

55 citations · 300 across the 22 of their papers we have counts for

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Showing 2013Show all

5 papers · 1 filter

astro-ph.GA2013★ 32 cited

Chaos and dynamical trends in barred galaxies: bridging the gap between N-body simulations and time-dependent analytical models

T. Manos, Rubens E. G. Machado

Self-consistent N-body simulations are efficient tools to study galactic dynamics. However, using them to study individual trajectories (or ensembles) in detail can be challenging.…

nlin.CD2013★ 43 cited

Survey on the role of accelerator modes for anomalous diffusion: The case of the standard map

Thanos Manos, Marko Robnik

We perform an extensive and detailed analysis of the generalized diffusion processes in deterministic area preserving maps with noncompact phase space, exemplified by the standard…

nlin.CD2013★ 21 cited

The intermediate level statistics in dynamically localized chaotic eigenstates

Benjamin Batistić, Thanos Manos, Marko Robnik

We demonstrate that the energy or quasienergy level spacing distribution in dynamically localized chaotic eigenstates is excellently described by the Brody distribution, displaying…

nlin.CD2013

Dynamical localization in kicked rotator as a paradigm of other systems: spectral statistics and the localization measure

Thanos Manos, Marko Robnik

We study the intermediate statistics of the spectrum of quasi-energies and of the eigenfunctions in the kicked rotator, in the case when the corresponding system is fully chaotic w…

nlin.CD2013★ 38 cited

Dynamical localization in chaotic systems: spectral statistics and localization measure in the kicked rotator as a paradigm for time-dependent and time-independent systems

Thanos Manos, Marko Robnik

We study quantum kicked rotator in the classically fully chaotic regime, in the domain of the semiclassical behaviour. We use Izrailev's N-dimensional model for various N<=4000, wh…