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相关论文: A symplectic integrator for the symmetry reduced a…

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In this work we propose a new numerical approach to distinguish between regular and chaotic orbits in Hamiltonian systems, based on the simultaneous integration of both the orbit and the deviation vectors using a symplectic scheme, hereby…

混沌动力学 · 物理学 2015-03-17 Anne-Sophie Libert , Charles Hubaux , Timoteo Carletti

We propose to use the properties of the Lie algebra of the angular momentum to build symplectic integrators dedicated to the Hamiltonian of the free rigid body. By introducing a dependence of the coefficients of integrators on the moments…

天体物理仪器与方法 · 物理学 2019-05-07 J. Laskar , T. Vaillant

We suggest a numerical integration procedure for solving the equations of motion of certain classical spin systems which preserves the underlying symplectic structure of the phase space. Such symplectic integrators have been successfully…

统计力学 · 物理学 2007-05-23 Robin Steinigeweg , Heinz-Jürgen Schmidt

We present a symplectic integrator, based on the canonical midpoint rule, for classical spin systems in which each spin is a unit vector in $\mathbb{R}^3$. Unlike splitting methods, it is defined for all Hamiltonians, and is…

数学物理 · 物理学 2023-03-20 Robert I. McLachlan , Klas Modin , Olivier Verdier

We construct a symplectic, globally defined, minimal-coordinate, equivariant integrator on products of 2-spheres. Examples of corresponding Hamiltonian systems, called spin systems, include the reduced free rigid body, the motion of point…

数学物理 · 物理学 2017-05-19 Robert I. McLachlan , Klas Modin , Olivier Verdier

The dynamic equation of mass point in rotating coordinates is governed by Coriolis and centrifugal force, besides a corotating potential relative to frame. Such a system is no longer a canonical Hamiltonian system so that the construction…

天体物理仪器与方法 · 物理学 2022-02-09 Xiongbiao Tu , Qiao Wang , Yifa Tang

The kinetic term of the $N$-body Hamiltonian system defined on the surface of the sphere is non-separable. As a result, standard explicit symplectic integrators are inapplicable. We exploit an underlying hierarchy in the structure of the…

数值分析 · 数学 2021-04-23 Ana Silva , Eitan Ben Av , Efi Efrati

We present a new symplectic integrator designed for collisional gravitational $N$-body problems which makes use of Kepler solvers. The integrator is also reversible and conserves 9 integrals of motion of the $N$-body problem to machine…

天体物理仪器与方法 · 物理学 2017-03-03 David M. Hernandez , Edmund Bertschinger

Symplectic integration algorithms are well-suited for long-term integrations of Hamiltonian systems because they preserve the geometric structure of the Hamiltonian flow. However, this desirable property is generally lost when adaptive…

天体物理学 · 物理学 2025-10-20 Miguel Preto , Scott Tremaine

Dependable numerical results from long-time simulations require stable numerical integration schemes. For Hamiltonian systems, this is achieved with symplectic integrators, which conserve the symplectic condition and exactly solve for the…

等离子体物理 · 物理学 2015-06-17 Stephen D. Webb

We develop Lie-Poisson integrators for general Hamiltonian systems on $\mathbf{R}^{3}$ equipped with the rigid body bracket. The method uses symplectic realisation of $\mathbf{R}^{3}$ on $T^{*}\mathbf{R}^{2}$ and application of symplectic…

数值分析 · 数学 2015-04-09 Robert McLachlan , Klas Modin , Olivier Verdier

The gravitational $N$-body problem, which is fundamentally important in astrophysics to predict the motion of $N$ celestial bodies under the mutual gravity of each other, is usually solved numerically because there is no known general…

计算物理 · 物理学 2021-12-10 Maxwell X. Cai , Simon Portegies Zwart , Damian Podareanu

A method for deriving superintegrable Hamiltonians with a spin orbital interaction is presented. The method is applied to obtain a new superintegrable system in Euclidean space $\mathbb{E}_3$ with the following properties. It describes a…

数学物理 · 物理学 2015-06-18 D. Riglioni , O. Gingras , P. Winternitz

We present a class of symplectic integrators adapted for the integration of perturbed Hamiltonian systems of the form $H=A+\epsilon B$. We give a constructive proof that for all integer $p$, there exists an integrator with positive steps…

天体物理学 · 物理学 2023-07-19 J. Laskar , P. Robutel

The 3-body problem in $\mathbb{R}^4$ has 24 dimensions and is invariant under translations and rotations. We do the full symplectic symmetry reduction and obtain a reduced Hamiltonian in local symplectic coordinates on a reduced phase space…

动力系统 · 数学 2020-09-07 Holger R. Dullin , Jürgen Scheurle

It is well known that symplectic integrators lose their near energy preservation properties when variable step sizes are used. The most common approach to combine adaptive step sizes and symplectic integrators involves the Poincar\'e…

数值分析 · 数学 2021-06-25 Valentin Duruisseaux , Jeremy Schmitt , Melvin Leok

We show that symplectic Runge-Kutta methods provide effective symplectic integrators for Hamiltonian systems with index one constraints. These include the Hamiltonian description of variational problems subject to position and velocity…

数值分析 · 数学 2014-02-28 Robert I McLachlan , Klas Modin , Olivier Verdier , Matt Wilkins

We consider periodic and quasi-periodic solutions of the three-body problem with homogeneous potential from the point of view of the equivariant calculus of variations. First, we show that symmetry groups of the Lagrangian action functional…

动力系统 · 数学 2008-06-11 Vivina Barutello , Davide L. Ferrario , Susanna Terracini

We introduce a novel numerical method to integrate partial differential equations representing the Hamiltonian dynamics of field theories. It is a multi-symplectic integrator that locally conserves the stress-energy tensor with an excellent…

数值分析 · 数学 2017-02-23 Hugo Ricateau , Leticia F. Cugliandolo

Symplectic integrators that preserve the geometric structure of Hamiltonian flows and do not exhibit secular growth in energy errors are suitable for the long-term integration of N-body Hamiltonian systems in the solar system. However, the…

广义相对论与量子宇宙学 · 物理学 2021-02-02 Ying Wang , Wei Sun , Fuyao Liu , Xin Wu
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