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Related papers: Renormalization and forcing of horseshoe orbits

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We introduce a new equivalence relation on the set of all polygonal billiards. We say that two billiards (or polygons) are order equivalent if each of the billiards has an orbit whose footpoints are dense in the boundary and the two…

Dynamical Systems · Mathematics 2012-01-19 Jozef Bobok , Serge Troubetzkoy

In this note, we extend the renormalization horseshoe we have recently constructed with N. Goncharuk for analytic diffeomorphisms of the circle to their small two-dimensional perturbations. As one consequence, Herman rings with rotation…

Dynamical Systems · Mathematics 2021-06-10 Michael Yampolsky

Motivated by a certain type of unfolding of a Hopf-Hopf singularity, we consider a one-parameter family $(f_\gamma)_{\gamma\geq0}$ of $C^3$--vector fields in $\mathbb{R}^4$ whose flows exhibit a heteroclinic cycle associated to two periodic…

Dynamical Systems · Mathematics 2025-05-01 Santiago Ibáñez , Alexandre A. P. Rodrigues

We study bifurcations of homoclinic orbits to hyperbolic saddle equilibria in a class of four-dimensional systems which may be Hamiltonian or not. Only one parameter is enough to treat these types of bifurcations in Hamiltonian systems but…

Dynamical Systems · Mathematics 2010-09-08 David Blazquez-Sanz , Kazuyuki Yagasaki

We consider a system of four one-dimensional inelastic hard spheres evolving on the real line $\mathbb{R}$, and colliding according to a scattering law characterized by a fixed restitution coefficient $r$. We study the possible orders of…

Dynamical Systems · Mathematics 2026-02-17 Roberto Castorrini , Théophile Dolmaire

We study the renormalization operator of circle homeomorphisms with a break point and show that it possesses a hyperbolic horseshoe attractor.

Dynamical Systems · Mathematics 2014-04-29 Konstantin Khanin , Michael Yampolsky

Co-orbital systems contain two or more bodies sharing the same orbit around a planet or star. The best-known flavors of co-orbital systems are tadpoles (in which two bodies' angular separations oscillate about the L4/L5 Lagrange points…

Earth and Planetary Astrophysics · Physics 2023-04-20 Sean N. Raymond , Dimitri Veras , Matthew S. Clement , Andre Izidoro , David Kipping , Victoria Meadows

The solvability in Sobolev spaces is proved for divergence form complex-valued higher order parabolic systems in the whole space, on a half space, and on a Reifenberg flat domain. The leading coefficients are assumed to be merely measurable…

Analysis of PDEs · Mathematics 2012-02-02 Hongjie Dong , Doyoon Kim

An analytic reversible Hamiltonian system with two degrees of freedom is studied in a neighborhood of its symmetric heteroclinic connection made up of a symmetric saddle-center, a symmetric orientable saddle periodic orbit lying in the same…

Dynamical Systems · Mathematics 2021-02-24 L. M. Lerman , K. N. Trifonov

A tight binding representation of the kicked Harper model is used to obtain an integrable semiclassical Hamiltonian consisting of degenerate "quantized" orbits. New orbits appear when renormalized Harper parameters cross integer multiples…

chao-dyn · Physics 2009-10-31 Indubala I. Satija , Bala Sundaram

We study the one-dimensional two-orbital Hubbard model with general local interactions including a pair-hopping term. The model might be realized in one-dimensional transition-metal nanowires. Phase diagrams at T=0 are obtained by numerical…

Strongly Correlated Electrons · Physics 2014-12-15 Jun-ichi Okamoto , A. J. Millis

Motivated by knot theory, it is natural to define the orientation-reversal of a quandle orbit by inverting all the translations given by elements of that orbit. In this short note we observe that this natural notion is unsuited to medial…

Geometric Topology · Mathematics 2025-11-24 Lorenzo Traldi

In this paper decomposition of periodic orbits in bifurcation diagrams are derived in unidimensional dynamics system $x_{n+1}=f(x_{n};r)$, being $f$ an unimodal function. We proof a theorem which states the necessary and sufficient…

We consider a superexchange Hamiltonian, $H=-\sum_{<i,j>}(2{\bf S}_i\cdot {\bf S}_j-\frac 12)(2{\bf T}_i\cdot {\bf T}_j-\frac 12)$, which describes systems with orbital degeneracy and strong electron-phonon coupling in the limit of large…

Strongly Correlated Electrons · Physics 2013-01-24 Guang-Ming Zhang , Shun-Qing Shen

Chaotic dynamics can be effectively studied by continuation from an anti-integrable limit. Using the Henon map as an example, we obtain a simple analytical bound on the domain of existence of the horseshoe that is equivalent to the…

chao-dyn · Physics 2020-06-02 D. G. Sterling , J. D. Meiss

We have recently presented strong evidence that chaotic orbits that obey one isolating integral besides energy exist in a toy Hamiltonian model with three degrees of freedom and are bounded by regular orbits that isolate them from the…

Astrophysics of Galaxies · Physics 2017-12-06 J. C. Muzzio

In this paper, we consider a smooth arc of diffeomorphisms which has a saddle-node bifurcation inside a nontrivial invariant set which is a deformation of a horseshoe. We show that this saddle-node bifurcation is isolated, that is, its…

Dynamical Systems · Mathematics 2007-05-23 Yongluo Cao , Shin Kiriki

Working with a general class of linear Hamiltonian systems with at least one singular boundary condition, we show that renormalized oscillation results can be obtained in a natural way through consideration of the Maslov index associated…

Classical Analysis and ODEs · Mathematics 2020-09-23 Peter Howard , Alim Sukhtayev

We show that, near periodic orbits, a class of hybrid models can be reduced to or approximated by smooth continuous-time dynamical systems. Specifically, near an exponentially stable periodic orbit undergoing isolated transitions in a…

Dynamical Systems · Mathematics 2015-01-09 Samuel A. Burden , Shai Revzen , S. Shankar Sastry

Orbits in the principal planes of triaxial potentials are known to be prone to unstable motion normal to those planes, so that three dimensional investigations of those orbits are needed even though they are two dimensional. We present here…

Astrophysics of Galaxies · Physics 2015-06-03 Daniel D. Carpintero , Juan C. Muzzio