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Fig. 2.

image

Evolution of the the virial ratio −2K/U (top panel), the fluctuations of the total energy δE in units of the initial energy E0 (middle panel), and the norm of the total angular momentum δL (bottom panel) for the same isotropic Plummer initial conditions with N = 2 × 104 particles, evolved with the direct N-body code (black lines), the exact angular momentum preserving MPC scheme (light blue lines), and the faster MPC rotation with a random axis (purple lines). The initial conditions have a slight angular momentum due to the randomised initialisation procedure for stellar velocities.

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