"Opik-type collision frequency for Kozai-driven projectiles: Target bodies on eccentric and inclined orbits

arXiv:2608.30972 · astro-ph.EP · Submitted 2026-08-31 · Read on arXiv

astro-ph.EP

Submitted: 2026-08-31

Updated: 2026-08-31

Comments: 24 pages, 3 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Secular Approximation — 1× in this paper · explained in 2 episodes
• Unified Framework — 1× in this paper · explained in 5 episodes

Sources

• \"Opik-type collision frequency for Kozai-driven projectiles: Target bodies on inclined circular orbits

Related papers

• PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
• Searching for substellar companion candidates with Gaia. V. M dwarfs within 15 pc studied with absolute astrometry, radial velocities, and direct imaging
• Gravitational Microlensing
• Two-stage disruption of resonant chains
• Detectability of resolved hydrogen lines from the accretion shock at gas giants and their circumplanetary discs
• Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function