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Long-wave and short-wave branches at marginal Toomre stability (∣k∣=[κ±n∣ΩP​−Ω∣]/a0​)

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
At fluid Toomre parameter Q=1, the local spiral-wave dispersion relation becomes n2(ΩP​−Ω)2=(a0​∣k∣−κ)2. The minus-sign, longer-wavelength root is nonnegative only between the two Lindblad resonance conditions. The plus-sign, shorter-wavelength root remains positive outside that interval. Thus this dispersion relation alone does not prove that every density wave is confined between Lindblad resonances; an additional physical restriction is needed.

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  1. Toomre parameter
  2. Toomre's stability criterion
  3. Gravitational instability of an astrophysical disk
  4. Astrophysical disk
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  • Past exam of the formation of Structure in the Universe course of the University of Cambridge / 2014 / Paper 1 / 2 / Solution

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