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Related papers: Narrow rings: a scattering billiard model

200 papers

Rings and gaps have been observed in a wide range of protoplanetary discs, from young systems like HLTau to older discs like TW Hydra. Recent disc simulations have shown that magnetohydrodynamic (MHD) turbulence (in the ideal or non-ideal…

Earth and Planetary Astrophysics · Physics 2019-05-29 A. Riols , G. Lesur

Rings are ubiquitous around giant planets in our Solar System. They evolve jointly with the nearby satellite system. They could form either during the giant planet formation process or much later, as a result of large scale dynamical…

Earth and Planetary Astrophysics · Physics 2018-12-05 Sébastien Charnoz , Aurélien Crida , Ryuki Hyodo

We investigate the dynamics of no-slip billiards, a model in which small rotating disks may exchange linear and angular momentum at collisions with the boundary. We give new results on periodicity and boundedness of orbits which suggest…

Dynamical Systems · Mathematics 2016-02-05 Chris Cox , Renato Feres

We investigate chaotic scattering on an attractive step potential with a quadrupolar deformation. The phase space features of the bound billiard are studied by using the notion of symmetry lines to find periodic orbits. We show that the…

chao-dyn · Physics 2009-10-30 Vincent J. Daniels , Michel Vallieres , Jian Min Yuan

The dynamics of chaotic billiards is significantly influenced by coexisting regions of regular motion. Here we investigate the prevalence of a different fundamental structure, which is formed by marginally unstable periodic orbits and…

Chaotic Dynamics · Physics 2008-01-24 E. G. Altmann , T. Friedrich , A. E. Motter , H. Kantz , A. Richter

The purpose of this paper is to compare a classical non-holonomic system---a sphere rolling against the inner surface of a vertical cylinder under gravity---and a class of discrete dynamical systems known as no-slip billiards in similar…

Dynamical Systems · Mathematics 2020-03-19 Timothy Chumley , Scott Cook , Christopher Cox , Renato Feres

We use global bifurcation techniques to establish the existence of arbitrarily many geometrically distinct nonplanar embedded smooth minimal 2-spheres in sufficiently elongated 3-dimensional ellipsoids of revolution. More precisely, we…

Differential Geometry · Mathematics 2025-11-05 Renato G. Bettiol , Paolo Piccione

We apply periodic orbit theory to a two-dimensional non-integrable billiard system whose boundary is varied smoothly from a circular to an equilateral triangular shape. Although the classical dynamics becomes chaotic with increasing…

Chaotic Dynamics · Physics 2008-11-26 Ken-ichiro Arita , Matthias Brack

In an ordinary billiard trajectories of a Hamiltonian system are elastically reflected after a collision with a hypersurface (scatterer). If the scatterer is a submanifold of codimension more than one, we say that the billiard is…

Dynamical Systems · Mathematics 2017-03-08 Sergey Bolotin

I propose a scenario for the formation of double-ring systems, as observed in some planetary nebulae and in the outer rings of SN 1987A. In this scenario, two jets, one jet on each side of the equatorial plane, expand into a thin, dense…

Astrophysics · Physics 2009-11-07 Noam Soker

We present a study of the spiral responses in a stable disc galaxy model to co-orbiting perturbing masses that are evenly spaced around rings. The amplitudes of the responses, or wakes, are proportional to the masses of the perturbations,…

Astrophysics of Galaxies · Physics 2021-09-01 J. A. Sellwood , R. G. Carlberg

Polygonal billiards constitute a special class of models. Though they have zero Lyapunov exponent their classical and quantum properties are involved due to scattering on singular vertices. It is demonstrated that in the semiclassical limit…

Quantum Physics · Physics 2019-02-07 Eugene Bogomolny

In billiard systems with a flux line semiclassical approximations for the density of states contain contributions from periodic orbits as well as from diffractive orbits that are scattered on the flux line. We derive a semiclassical…

chao-dyn · Physics 2010-03-09 Martin Sieber

We present a novel mechanism for resolving the mechanical rigidity of nanoscopic circular polymers that flow in a complex environment. The emergence of a regime of negative differential mobility induced by topological interactions between…

Soft Condensed Matter · Physics 2018-11-21 Stefano Iubini , Enzo Orlandini , Davide Michieletto , Marco Baiesi

(Abridged) A simple and general description of the dynamics of a narrow eccentric ring is presented.We view an eccentric ring which precesses uniformly at a slow rate as exhibiting a global $m=1$ mode originating from a standing wave…

Astrophysics · Physics 2009-11-10 J. C. B. Papaloizou , M. D. Melita

The phase-space volume of regions of regular or trapped motion, for bounded or scattering systems with two degrees of freedom respectively, displays universal properties. In particular, drastic reductions in the volume (gaps) are observed…

Chaotic Dynamics · Physics 2008-01-14 L. Benet , O. Merlo

A Roche model for describing uniformly rotating rings is presented and the results are compared with numerical solutions to the full problem for polytropic rings. In the thin ring limit, the surfaces of constant pressure including the…

Astrophysics · Physics 2009-01-13 Stefan Horatschek , David Petroff

Shadows and spirals seem to be common features of transition discs. Among the spiral-triggering mechanisms proposed, only one establishes a causal link between shadows and spirals so far. In fact, provided the presence of shadows in the…

Earth and Planetary Astrophysics · Physics 2018-01-24 Matías Montesinos , Nicolás Cuello

Collective organisation of patterns into ring-like configurations has been well-studied when patterns are subject to either weak or semi-strong interactions. However, little is known numerically or analytically about their formation when…

Dynamical Systems · Mathematics 2024-03-06 Dan J. Hill , Jason J. Bramburger , David J. B. Lloyd

Recent experiments have shown that many species of microorganisms leave a solid surface at a fixed angle determined by steric interactions and near-field hydrodynamics. This angle is completely independent of the incoming angle. For several…

Soft Condensed Matter · Physics 2016-06-14 Madison S. Krieger