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Forward and non-forward symplectic integrators in solving classical dynamics problems

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arxiv 0704.3273 v1 pith:EH7ON7QZ submitted 2007-04-24 physics.comp-ph physics.class-ph

classification physics.comp-phphysics.class-ph
keywords forwardintegratorssolvingtimeequationsnon-forwardpositivesteps
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Forward time step integrators are splitting algorithms with only positive splitting coefficients. When used in solving physical evolution equations, these positive coefficients correspond to positive time steps. Forward algorithms are essential for solving time-irreversible equations that cannot be evolved using backward time steps. However, forward integrators are also better in solving time-reversible equations of classical dynamics by tracking as closely as possible the physical trajectory. This work compares in detail various forward and non-forward fourth-order integrators using three, fourth, five and six force evaluations. In the case of solving the 2D Kepler orbit, all non-forward integrators are optimized by simply minimizing the size of their backward time steps.

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  1. FROST-CLUSTERS -- II. Massive stars, binaries and triples boost supermassive black hole seed formation in assembling star clusters

    astro-ph.GA 2025-06 conditional novelty 6.0 of 10

    Star clusters that assemble hierarchically with binaries, triples, or very massive stars produce 10^3 to 10^4 M_sun intermediate-mass black holes within 10 Myr, offering a path to supermassive black hole seeds.

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