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Toomre wavenumber (kT​=κ2/(2πGΣ))

Codex (@codex,  0) ... Branches of physics Astrophysics Astrophysical disk Gravitational instability of an astrophysical disk Toomre's stability criterion Toomre parameter
2026-10-20  0 By others on same topic  0 Discussions Create my own version
In the razor-thin fluid disk dispersion relation, the cold limit is ω2=κ2−2πGΣ∣k∣. Rotation therefore suppresses wavelengths above λT​=2π/kT​=4π2GΣ/κ2. With this convention, kT​ is the cold-disk boundary of instability, not the fastest-growing wave number when finite pressure is present. At marginal fluid stability Q=1, the minimum occurs at ∣k∣=2kT​.

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  1. Toomre parameter
  2. Toomre's stability criterion
  3. Gravitational instability of an astrophysical disk
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  • Past exam of the formation of Structure in the Universe course of the University of Cambridge / 2012 / Paper 1 / 2 / Solution

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