An Analytic Solution to the Kozai-Lidov Evolution Equations
arXiv:2107.09732 · doi:10.1093/mnras/stab2133
Abstract
A test particle in a noncoplanar orbit about a member of a binary system can undergo Kozai-Lidov oscillations in which tilt and eccentricity are exchanged. An initially circular highly inclined particle orbit can reach high eccentricity. We consider the nonlinear secular evolution equations previously obtained in the quadrupole approximation. For the important case that the initial eccentricity of the particle orbit is zero, we derive an analytic solution for the particle orbital elements as a function of time that is exact within the quadrupole approximation. The solution involves only simple trigonometric and hyperbolic functions. It simplifies in the case that the initial particle orbit is close to being perpendicular to the binary orbital plane. The solution also provides an accurate description of particle orbits with nonzero but sufficiently small initial eccentricity. It is accurate over a range of initial eccentricity that broadens at higher initial inclinations. In the case of an initial inclination of pi/3, an error of 1% at maximum eccentricity occurs for initial eccentricities of about 0.1.
arXiv commentTo be published in MNRAS, 8 pages, 7 figures
References in corpus (22)
- Shrinking binary and planetary orbits by Kozai cycles with tidal friction
- The Eccentric Kozai-Lidov Effect and Its Applications
- Planet Migration and Binary Companions: the case of HD 80606b
- Evolution in Binary and Triple Stars, with an application to SS Lac
- Secular Dynamics in Hierarchical Three-Body Systems
- The Kozai Mechanism and the Evolution of Binary Supermassive Black Holes
- On the triple origin of blue stragglers
- Four-Body Effects in Globular Cluster Black Hole Coalescence
- Black hole mergers and blue stragglers from hierarchical triples formed in globular clusters
- Satellite dynamics on the Laplace surface
- Formation and Stellar Spin-Orbit Misalignment of Hot Jupiters from Lidov-Kozai Oscillations in Stellar Binaries
- The Kozai-Lidov Mechanism in Hydrodynamical Disks
- Warm Jupiters from secular planet-planet interactions
- High Orbital Eccentricities of Extrasolar Planets Induced by the Kozai Mechanism
- A Class of Warm Jupiters with Mutually Inclined, Apsidally Misaligned, Close Friends
- Why do Earth satellites stay up?
- Formation and merging of Mass Gap Black Holes in Gravitational Wave Merger Events from Wide Hierarchical Quadruple Systems
- Lidov-Kozai Mechanism in Hydrodynamical Disks: Linear Stability Analysis
- Kozai-Lidov Disc Instability
- Massive binary star mergers in galactic nuclei: implications for blue stragglers, binary S-stars and gravitational waves
- Properties of von Zeipel-Lidov-Kozai oscillations in triple systems at the quadrupole order: relaxing the test particle approximation
- The Stability and Dynamics of Planets in Tight Binary Systems
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