English

Energy evolution in time-dependent harmonic oscillator

Chaotic Dynamics 2007-05-23 v1 Exactly Solvable and Integrable Systems

Abstract

The theory of adiabatic invariants has a long history, and very important implications and applications in many different branches of physics, classically and quantally, but is rarely founded on rigorous results. Here we treat the general time-dependent one-dimensional harmonic oscillator, whose Newton equation q¨+ω2(t)q=0\ddot{q} + \omega^2(t) q=0 cannot be solved in general. We follow the time-evolution of an initial ensemble of phase points with sharply defined energy E0E_0 at time t=0t=0 and calculate rigorously the distribution of energy E1E_1 after time t=Tt=T, which is fully (all moments, including the variance μ2\mu^2) determined by the first moment E1ˉ\bar{E_1}. For example, μ2=E02[(E1ˉ/E0)2(ω(T)/ω(0))2]/2\mu^2 = E_0^2 [(\bar{E_1}/E_0)^2 - (\omega (T)/\omega (0))^2]/2, and all higher even moments are powers of μ2\mu^2, whilst the odd ones vanish identically. This distribution function does not depend on any further details of the function ω(t)\omega (t) and is in this sense universal. In ideal adiabaticity E1ˉ=ω(T)E0/ω(0)\bar{E_1} = \omega(T) E_0/\omega(0), and the variance μ2\mu^2 is zero, whilst for finite TT we calculate E1ˉ\bar{E_1}, and μ2\mu^2 for the general case using exact WKB-theory to all orders. We prove that if ω(t)\omega (t) is of class Cm{\cal C}^{m} (all derivatives up to and including the order mm are continuous) μT(m+1)\mu \propto T^{-(m+1)}, whilst for class C{\cal C}^{\infty} it is known to be exponential μexp(αT)\mu \propto \exp (-\alpha T).

Keywords

Cite

@article{arxiv.nlin/0608004,
  title  = {Energy evolution in time-dependent harmonic oscillator},
  author = {Marko Robnik and Valery G. Romanovski},
  journal= {arXiv preprint arXiv:nlin/0608004},
  year   = {2007}
}

Comments

26 pages, 5 figures

R2 v1 2026-07-22T18:15:52.826Z