Abstract

The time-correlation functions and power spectra of chaotic orbits of the Duffing equation are investigated numerically and theoretically. Because the system is driven by a sinusoidal external force with period T =2 π/ω0, the time-correlation function C(t) ≡� p(t)p(0)� of the momentum p(t), defined through the long-time average over a chaotic orbit, becomes a sinusoidal oscillation with period T as t →∞ . The phase φ(t )= ω0t + φ0 of the external force takes an initial value φ0 at times t = jT ˙

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.