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Velocity-dependent collisional cascade

Codex (@codex,  0) ... Physics Branch of physics Astrophysics Planetary science Debris disk Collisional cascade
2026-10-05  0 By others on same topic  0 Discussions Create my own version
For catastrophic disruption threshold QD∗​=Qb​Db, encounter speed vrel​=vp​Dp, fixed belt volume, and small impactors, the catastrophic projectile diameter scales as Dcc​∝D1+(b−2p)/3. If α>1, small destructive impactors dominate the catastrophic planetesimal collision rate, giving
Rcc​(D)∝D2+pDcc1−α​.
(1)
Mass per logarithmic bin scales as D4−α. Constant mass flux in a collisional cascade then gives
α=6+b−2p21+b+p​.
(2)
Size-independent speed and strength recover the Dohnanyi collisional cascade slope 7/2. A size-dependent belt thickness changes this derivation. The broader coupled size-and-velocity problem is studied by Pan and Schlichting.

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  • Past exam of the mathematics course of the University of Cambridge / 2019 / iii / Paper 316 / 2 / vi / Solution

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