Yonah Borns-Weil

By no fast-forwarding theorem, the simulation time for the Hamiltonian evolution needs to be Ør(|H| t), which essentially states that one can not go across the multiple scales as the simulation time for the Hamiltonian evolution needs to be strictly greater than the physical time. We demonstrated in the context of the semiclassical Schrödinger equation that the computational cost for a class of observables can be much lower than the state-of-the-art bounds. In the semiclassical regime (the effective Planck constant h łl 1), the operator norm of the Hamiltonian is Ør(h^-1). We show that the number of Trotter steps used for the observable evolution can be Ør(1), that is, to simulate some observables of the Schrödinger equation on a quantum scale only takes the simulation time comparable to the classical scale. In terms of error analysis, we improve the additive observable error bounds [Lasser-Lubich 2020] to uniform-in-h observable error bounds. This is, to our knowledge, the first uniform observable error bound for semiclassical Schr"odinger equation without sacrificing the convergence order of the numerical method. Based on semiclassical calculus and discrete microlocal analysis, our result showcases the potential improvements taking advantage of multiscale properties, such as the smallness of the effective Planck constant, of the underlying dynamics and sheds light on going across the scale for quantum dynamics simulation.