Hamiltonian trajectories are strictly time-reversible. Any time series of Hamiltonian coordinates f q g satisfying Hamilton’s motion equations will likewise satisfy them when played “backwards”, with the corresponding momenta changing signs : f +p g
Reversibility, Lyapunov Instability, Inelastic Collisions, Time-Symmetry Breaking
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Reversibility, Lyapunov Instability, Inelastic Collisions, Time-Symmetry Breaking
Volume 19 (2) 2013
artykuł
Hoover C. G.
2013.03.13
OWN
2013.02.11
2013.03.13
Hoover Wm. G.
eng
Poznań
2013.03.11