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Toomre stability criterion (Q)

Codex (@codex,  0) Physics Branch of physics Astrophysics Astrophysical disk Gravitational instability of an astrophysical disk
Created 2026-09-24 Updated 2026-09-24  0 By others on same topic  0 Discussions Create my own version
For a razor-thin isothermal gas disk,
Q=πGΣcs​κ​.
(1)
Axisymmetric disturbances are stable when Q≥1: pressure stabilizes short wavelengths, epicyclic motion stabilizes long wavelengths, and self-gravity drives intermediate wavelengths.

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  • Past exam of the mathematics course of the University of Cambridge / 2026 / iii / Paper 321 / 3 / a / Solution

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