2009
DOI: 10.1088/1751-8113/42/37/375207
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Spatial chaos of an extensible conducting rod in a uniform magnetic field

Abstract: Abstract. The equilibrium equations for the isotropic Kirchhoff rod are known to form an integrable system. It is also known that the effects of extensibility and shearability of the rod do not break the integrable structure. Nor, as we have shown in a previous paper does the effect of a magnetic field on a conducting rod. Here we show, by means of Mel'nikov analysis, that, remarkably, the combined effects do destroy integrability; that is, the governing equations for an extensible current-carrying rod in a un… Show more

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Cited by 8 publications
(5 citation statements)
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“…The equilibrium equations for an extensible and shearable rod in a uniform magnetic field were derived in [17]. The equations were obtained by reduction of a nine-dimensional system in Lie-Poisson form with three Casimirs to a six-dimensional canonical Hamiltonian system in terms of three Euler angles (θ, ψ, φ) and their canonical momenta (p θ , p ψ , p φ ), similar to the reduction of the isotropic elastic rod [20] or the symmetric heavy top [5].…”
Section: Hamiltonian For An Extensible Rod In a Uniform Magnetic Fieldmentioning
confidence: 99%
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“…The equilibrium equations for an extensible and shearable rod in a uniform magnetic field were derived in [17]. The equations were obtained by reduction of a nine-dimensional system in Lie-Poisson form with three Casimirs to a six-dimensional canonical Hamiltonian system in terms of three Euler angles (θ, ψ, φ) and their canonical momenta (p θ , p ψ , p φ ), similar to the reduction of the isotropic elastic rod [20] or the symmetric heavy top [5].…”
Section: Hamiltonian For An Extensible Rod In a Uniform Magnetic Fieldmentioning
confidence: 99%
“…where T u > 0 is a constant, L s is a 2 × 4 matrix consisting of row eigenvectors corresponding to eigenvalues with negative real parts of the Jacobian matrix J D 2 H(ξ 0 ) and ξ u 0 is a point on W u (ξ 0 ). Thus, we solve the boundary value problem (15) and (17) and continue the solution in ξ u 0 to compute W u (ξ 0 ) numerically. Similarly, to compute W s (ξ 0 ), we solve the boundary value problem (15) and…”
Section: Numerical Analysismentioning
confidence: 99%
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“…In classical problems of elastic stability (like Euler buckling), the system is subject to conservative loads and stability of a static solution against infinitesimally small perturbations depends on second variations of an energy functional. Non-conservative forces like a follower load (Langthjem and Sugiyama, 2000), magnetic forces (Sinden and van der Heijden, 2009) or sliding friction can be treated either via an extended energy approach or by direct analysis of the equations of motion. The loss of elastic stability plays a key role in many processes related to biological growth, which is subject of the theory of morpho-elasticity (Goriely, 2017).…”
Section: Introductionmentioning
confidence: 99%