Chaos and anomalous transport in a semiclassical Bose-Hubbard chain (2308.14720v3)
Abstract: We study chaotic dynamics and anomalous transport in a Bose-Hubbard chain in the semiclassical regime (the limit when the number of particles goes to infinity). We find that the system has mixed phase space with both regular and chaotic dynamics, even for long chains with up to hundred wells. The consequence of the mixed phase space is strongly anomalous diffusion in the space of occupation numbers, with a discrete set of transport exponents. After very long times the system crosses over to the hydrodynamic regime with normal diffusion. Anomalous transport is quite universal, almost completely independent of the parameters of the model (Coulomb interaction, chemical potential): it is mainly determined by the initial distribution of particles along the chain. We corroborate our findings by analytical arguments: scaling analysis for the anomalous regime and the Langevin equation for the normal diffusion regime.
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- Here we tacitly assume from the beginning that higher Lyapunov exponents mean stronger chaos. This is indeed generally true in systems with finite phase space volume; it is not in general true for systems like inverse harmonic oscillator where orbits can escape to infinity. But the latter does not happen in the Bose-Hubbard model so for us indeed the exponents λnsubscript𝜆𝑛\lambda_{n}italic_λ start_POSTSUBSCRIPT italic_n end_POSTSUBSCRIPT should be a meaningful indicator of chaos.
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- In Fig. 6 and all subsequent figures with log-log plots, we rescale the time by the scale t0subscript𝑡0t_{0}italic_t start_POSTSUBSCRIPT 0 end_POSTSUBSCRIPT for dimensional reasons. Here t0subscript𝑡0t_{0}italic_t start_POSTSUBSCRIPT 0 end_POSTSUBSCRIPT is determined by the hopping J𝐽Jitalic_J and the total number N𝑁Nitalic_N and is used as the time/energy unit for all quantities in the paper.
- Remember that for U/J𝑈𝐽U/Jitalic_U / italic_J very small or very large the system becomes integrable.
- Indeed, in many integrations the numerics becomes unstable before reaching t**subscript𝑡absentt_{**}italic_t start_POSTSUBSCRIPT * * end_POSTSUBSCRIPT; but we expect that normal diffusion will always exist once the ensemble of orbits has explored sufficiently large volume of the phase space.
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- We deliberately differentiate between the angle average and the average over the ensemble ⟨(…)⟩delimited-⟨⟩…\langle(\ldots)\rangle⟨ ( … ) ⟩. Although the two have to coincide if the diffusion approximation is exact, it never is in practice.
- We cannot provide a proof of this assumption (which in any case certainly only holds approximately); a look at the strongly erratic oscillations of some orbits in Figs. 1 and 2 provides some justification.
- The normalization by the factor ⟨⟨ϕ˙i2⟩⟩delimited-⟨⟩delimited-⟨⟩superscriptsubscript˙italic-ϕ𝑖2\langle\langle\dot{\phi}_{i}^{2}\rangle\rangle⟨ ⟨ over˙ start_ARG italic_ϕ end_ARG start_POSTSUBSCRIPT italic_i end_POSTSUBSCRIPT start_POSTSUPERSCRIPT 2 end_POSTSUPERSCRIPT ⟩ ⟩ is necessary because by construction of the Langevin equation (30) the Wiener process is assumed to be normalized, i.e. it is already multiplied by the right-hand side of the equations of motion.
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