Hierarchical three-body problem at high eccentricities = simple pendulum – III. Precessing quadrupole

ABSTRACT The very long-term evolution of the hierarchical restricted three-body problem with a slightly aligned precessing quadrupole potential is investigated analytically and solved for both rotating and librating Kozai–Lidov cycles (KLCs) with high eccentricities. We describe the finding of a striking similarity between librating and rotating KLCs for some range of precession rates. We show that the main effect occurs in both categories when the KLC frequency is equal to the precession rate of the perturbing potential. We solve the resonant dynamics analytically and show that it is equivalent to a simple pendulum model allowing us to map the strikingly rich structures that arise for precession rates similar to the Kozai–Lidov time-scale (ratio of a few) and explain the similarity and when it vanishes. Additionally, we show that the regular KLCs at high eccentricities can also be described using a simple pendulum.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society Letters
Published
2025-02-27
DOI
https://doi.org/10.1093/mnrasl/slaf017
Citations
2
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
2.31
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article

Hierarchical three-body problem at high eccentricities = simple pendulum – III. Precessing quadrupole

Boaz Katz, Ygal Klein
2 citations
Monthly Notices of the Royal Astronomical Society Letters
Pulsars and Gravitational Waves Research
2.31
article

Hierarchical three-body problem at high eccentricities = simple pendulum – III. Precessing quadrupole

Boaz Katz, Ygal Klein
article en
2 citations

Abstract

ABSTRACT The very long-term evolution of the hierarchical restricted three-body problem with a slightly aligned precessing quadrupole potential is investigated analytically and solved for both rotating and librating Kozai–Lidov cycles (KLCs) with high eccentricities. We describe the finding of a striking similarity between librating and rotating KLCs for some range of precession rates. We show that the main effect occurs in both categories when the KLC frequency is equal to the precession rate of the perturbing potential. We solve the resonant dynamics analytically and show that it is equivalent to a simple pendulum model allowing us to map the strikingly rich structures that arise for precession rates similar to the Kozai–Lidov time-scale (ratio of a few) and explain the similarity and when it vanishes. Additionally, we show that the regular KLCs at high eccentricities can also be described using a simple pendulum.

Monthly Notices of the Royal Astronomical Society LettersVol. 539(1)
Weizmann Institute of Science (IL)
Openalex Percentile: Top 13%
Pulsars and Gravitational Waves Research
2.31
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Hierarchical three-body problem at high eccentricities = simple pendulum – III. Precessing quadrupole — Boaz Katz, Ygal Klein · Monthly Notices of the Royal Astronomical Society Letters (2025) | TGRS Research Map | TGRS