The same circular orbit at

PHYSICS · Multi-part · Fermi University Physics · Mathematical Methods for Physics · Computational Physics · Simulating classical dynamical systems

Computational Physics, Ch An orbit that must not drift

Problem

The same circular orbit at a=1 AUa=1\,\mathrm{AU}, integrated at Δt=10−3 yr\Delta t = 10^{-3}\,\mathrm{yr} for 100100 years, gives these fractional energy drifts ΔE/∣E0∣\Delta E/|E_0|: Euler +0.66+0.66 (still rising), Euler-Cromer bounded within 3.9×10−53.9\times10^{-5}, Verlet bounded within 3.9×10−103.9\times10^{-10}, and Runge-Kutta −1.7×10−10-1.7\times10^{-10} (a loss, still falling steadily). A bounded method's error stays within the same fixed band forever, however long the run; a method whose error is a steady loss accumulates that loss in rough proportion to the elapsed time. ((a)) Predict the size of the Runge-Kutta drift after 10410^4 years (a hundred times longer), assuming the loss continues to accumulate in proportion to elapsed time. ((b)) Give the new ranking of the four methods by ∣ΔE/∣E0∣∣\big|\Delta E/|E_0|\big| at 10410^4 years, smallest first, and say which pair of methods has swapped places compared with the 100100-year ranking (Runge-Kutta smallest, then Verlet, then Euler-Cromer, then Euler). ((c)) State in one sentence why the 100100-year ranking is not a safe guide to which method is best for a much longer run.

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