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The Kozai-Lidov Mechanism in Hydrodynamical Disks

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arxiv 1409.1226 v1 pith:RLPYPRA4 submitted 2014-09-03 astro-ph.EP astro-ph.HE

Rebecca G. Martin , Chris Nixon , Stephen H. Lubow , Philip J. Armitage , Daniel J. Price , Suzan Dogan , Andrew King This is my paper · ORCID
classification astro-ph.EPastro-ph.HE
keywords accretionbinarydiskdiskshydrodynamicalkozai-lidovsystemsaccreting
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We use three dimensional hydrodynamical simulations to show that a highly misaligned accretion disk around one component of a binary system can exhibit global Kozai-Lidov cycles, where the inclination and eccentricity of the disk are interchanged periodically. This has important implications for accreting systems on all scales, for example, the formation of planets and satellites in circumstellar and circumplanetary disks, outbursts in X-ray binary systems and accretion on to supermassive black holes.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. 2D hydrodynamical simulations of Be star decretion disc formation through boundary layer effects

    astro-ph.SR 2026-07 conditional novelty 6.0 of 10

    Viscous boundary layer effects launch a decretion disc around a star spinning at 80% of breakup but not at 70%, in 2D hydro simulations.

  2. Circumstellar and circumbinary discs in multiple stellar systems

    astro-ph.EP 2025-01 conditional novelty 1.0 of 10

    This review consolidates current knowledge on how stellar multiplicity shapes protoplanetary disc structure, dust evolution, and planet formation outcomes.

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