Kozai-Lidov effectResonanceExploring weakly perturbed Keplerian motion within the restricted three-body problem, Lidov (1962) and, independently, Kozai (1962) discovered coupled oscillations of eccentricity and inclination (the KL-cycles). Their classical studies were based on an integrable model of ...
The short, 6-month dynamical lifetime has often been explained through an increase in eccentricity due to the Lidov-Kozai effect. However, the classical Lidov-Kozai solution is only valid in the limit of small semi-major axis ratio, a condition that is satisfied only for solar (but not for...
The short, 6-month dynamical lifetime has often been explained through an increase in eccentricity due to the Lidov–Kozai effect. However, the classical Lidov–Kozai solution is only valid in the limit of small semi-major axis ratio, a condition that is satisfied only fo...
I. I. Shevchenko, The Lidov-Kozai Effect-- Applications in Exoplanet Research and Dynamical Astronomy, Astrophys. Space Sci. Library (Springer, 2017), p. 194 [in Russian].Shevchenko, I.I. (Ed.), 2017. The Lidov-Kozai Effect; Applications in Exoplanet Research and Dynamical Astronomy. ...
Frederic A. RasioFani DosopoulouIOP PublishingB.-M. Hoang, S. Naoz, B. Kocsis, F. A. Rasio, and F. Dosopoulou, "Black Hole Mergers in Galactic Nuclei Induced by the Eccentric Kozai-Lidov Effect," ApJ 856 (Apr., 2018) 140, 1706.09896....
In this paper, we use three-dimensional hydrodynamical simulations to analyze how various binary and disk parameters affect the Kozai-Lidov mechanism in hydrodynamical disks. The simulations include the effect of gas pressure and viscosity, but ignore the effects of disk self-gravity. We describe ...
In the Kuiper belt, however, the drag is linear with velocity and the effect of the wind cancels out as the angular momentum gained in half an orbit is exactly lost in the other half; the drag timescales for 10 km bodies remain greater than or similar to 10 Myr. In this situation we...
MODELRELATIVISTICBINARIESWe consider the hierarchical three-body problem, with a binary and a planet-mass object. We investigate the effect of general relativity (GR) corrections to the Newtonian interactions. We focus on the Lidov-Kozai resonance, and the secular dynamics are analyzed over wide ...
The Lidov–Kozai effect reveals itself in coupled periodic variations (which can be very large) of the inclination and eccentricity of an orbiting body in presence of an inclined perturber. The effect...doi:10.1007/978-3-030-52144-8_15Shevchenko, Ivan I....
Launched in October 1959 on a translunar trajectory with large semimajor axis and eccentricity, it...doi:10.1007/s10569-020-09972-6Davide AmatoRenu MalhotraVladislav SidorenkoAaron J. RosengrenCelestial Mechanics and Dynamical Astronomy