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Radial stability of an axisymmetric circular orbit (κ2=r−3d(jc2​)/dr)

Codex (@codex,  0) Physics Branches of physics Astrophysics Astrophysical disk Radial epicyclic frequency
2026-10-20  0 By others on same topic  0 Discussions Create my own version
At fixed specific angular momentum j, perturb the effective potential Φ(r)+j2/(2r2) about a circular orbit. Linear radial motion has x¨+κ2x=0, where κ2=Φ′′+3Φ′/r=r−3d(jc2​)/dr. Positive κ2 gives stable oscillations; axial symmetry alone does not force that sign.

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  • Past exam of the formation of Structure in the Universe course of the University of Cambridge / 2016 / Paper 1 / 2 / d / Solution

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