Double-Averaging Can Fail to Characterize the Long-Term Evolution of Lidov-Kozai Cycles & Derivation of an Analytical Correction
Liantong Luo (KIAA-PKU), Boaz Katz (Weizmann), Subo Dong (KIAA-PKU)

TL;DR
This paper demonstrates that the standard double-averaging approximation can fail to accurately predict long-term Lidov-Kozai cycle evolution due to neglected short-term oscillations, and introduces a corrected analytical method to improve predictions.
Contribution
The authors derive analytical equations for short-term oscillations and develop a corrected double-averaging method that improves long-term evolution predictions in hierarchical three-body systems.
Findings
CDA significantly reduces errors in long-term evolution predictions.
Short-term oscillations can accumulate and cause major deviations from DA.
CDA is validated against N-body simulations across various initial conditions.
Abstract
The double-averaging (DA) approximation is widely employed as the standard technique in studying the secular evolution of the hierarchical three-body system. We show that effects stemmed from the short-timescale oscillations ignored by DA can accumulate over long timescales and lead to significant errors in the long-term evolution of the Lidov-Kozai cycles. In particular, the conditions for having an orbital flip, where the inner orbit switches between prograde and retrograde with respect to the outer orbit and the associated extremely high eccentricities during the switch, can be modified significantly. The failure of DA can arise for a relatively strong perturber where the mass of the tertiary is considerable compared to the total mass of the inner binary. This issue can be relevant for astrophysical systems such as stellar triples, planets in stellar binaries, stellar-mass binaries…
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