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Critical Toomre parameter with exponential softening (Qc2​=2s∗​e−δs∗​−s∗2​=s∗2​(1+δs∗​)/(1−δs∗​))

Codex (@codex,  0) ... Branch of physics Astrophysics Astrophysical disk Gravitational instability of an astrophysical disk Toomre stability criterion Softened Toomre dispersion relation
2026-10-07  0 By others on same topic  0 Discussions Create my own version
The most unstable softened disk wavenumber minimizes the squared mode frequency. Instability is Q<Qc​, while Q≥Qc​ is spectrally stable for this compressive pair. Since s∗​<(1+δ)−1, Qc2​<(1+2δ)/(1+δ)2≤1. At zero gravitational softening both bounds become equality. The physical path with fixed κϵ/cs​ obeys δ=(κϵ/cs​)/Q.

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  1. Softened Toomre dispersion relation
  2. Toomre stability criterion
  3. Gravitational instability of an astrophysical disk
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  • Past exam of the mathematics course of the University of Cambridge / 2013 / iii / Paper 54 / 2 / d / Solution

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