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handle: 2117/415428
We construct $C^{\infty}$ time-periodic fluctuating surfaces in $\mathbb{R}^3$ such that the corresponding nonautonomous geodesic flow has orbits along which the energy, and thus the speed, goes to infinity.
Non-autonomous perturbation, Àrees temàtiques de la UPC::Matemàtiques i estadística, Dynamical Systems (math.DS), 530, Hamiltonian dynamics, 510, Fermi acceleration, Arnold diffusion, Geodesic flow, FOS: Mathematics, Sistemes hamiltonians, and nonholonomic systems, Hamiltonian systems, Mathematics - Dynamical Systems, Classificació AMS::37 Dynamical systems and ergodic theory::37J Finite-dimensional Hamiltonian, Lagrangian, contact, and nonholonomic systems, Classificació AMS::37 Dynamical systems and ergodic theory::37J Finite-dimensional Hamiltonian, Lagrangian, contact
Non-autonomous perturbation, Àrees temàtiques de la UPC::Matemàtiques i estadística, Dynamical Systems (math.DS), 530, Hamiltonian dynamics, 510, Fermi acceleration, Arnold diffusion, Geodesic flow, FOS: Mathematics, Sistemes hamiltonians, and nonholonomic systems, Hamiltonian systems, Mathematics - Dynamical Systems, Classificació AMS::37 Dynamical systems and ergodic theory::37J Finite-dimensional Hamiltonian, Lagrangian, contact, and nonholonomic systems, Classificació AMS::37 Dynamical systems and ergodic theory::37J Finite-dimensional Hamiltonian, Lagrangian, contact
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