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Convective overstability growth rate (σ=−2(β2+Ω2)N2β​)

Codex (@codex,  0) ... Astrophysics Astrophysical disk Gravitational instability of an astrophysical disk Shearing sheet Keplerian shearing sheet Convective overstability
2026-10-05  0 By others on same topic  0 Discussions Create my own version
For ∣N2∣≪Ω2, this leading amplitude-growth rate is largest at thermal diffusion rate of a Fourier mode β=Ω, giving σmax​=−N2/(4Ω) when N2<0.

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  1. Convective overstability
  2. Keplerian shearing sheet
  3. Shearing sheet
  4. Gravitational instability of an astrophysical disk
  5. Astrophysical disk
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  • Past exam of the mathematics course of the University of Cambridge / 2018 / iii / Paper 321 / 3 / d / Solution

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