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Regular dynamics of canonical post-Newtonian Hamiltonian for spinning compact binaries with next-to-leading order spin-orbit interactions

机译:正负后牛顿哈密顿量的正则动力学,用于旋转紧随其后的自旋轨道相互作用的紧致二元

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摘要

This paper shows that a conservative canonical post-Newtonian Hamiltonian formulation of spinning compact binaries with a pure orbital part up to third post-Newtonian order and spin-orbit contributions at the next-to-leading post-Newtonian order is explicitly integrable and regular because there are 5 independent exact isolating integrals in the 10-dimensional phase space. With the help of symplectic integrators and the fast Lyapunov indicators of two nearby trajectories, numerical investigations also support the absence of chaos.
机译:本文表明,一个保守的规范的后牛顿哈密顿量公式,其旋转的紧致二元具有纯轨道部分,直到第三牛顿后阶,并且自旋轨道贡献位于紧随其后的牛顿阶之后,这显然是可积的和规则的,因为在10维相空间中有5个独立的精确隔离积分。借助辛积分器和两个附近轨迹的快速Lyapunov指标,数值研究也支持不存在混沌。

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