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Acoustic-gravity propagation relation (kr2​≃(ω2−Sℓ2​)(ω2−N2)/(cs2​ω2))

Codex (@codex,  0) ... Physics Branch of physics Fluid mechanics Astrophysical fluid dynamics Stellar oscillation Linear adiabatic stellar oscillation equations
2026-10-06  0 By others on same topic  0 Discussions Create my own version
In the Cowling approximation and local short-wavelength limit, the radial wave number satisfies kr2​≃(ω2−Sℓ2​)(ω2−N2)/(cs2​ω2). The Lamb frequency Sℓ​ and stellar buoyancy frequency N delimit acoustic and gravity-wave cavities. This leading interior relation does not replace the near-surface acoustic cutoff or the full gravitational boundary problem.

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  1. Linear adiabatic stellar oscillation equations
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  3. Astrophysical fluid dynamics
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  • Past exam of the mathematics course of the University of Cambridge / 2015 / iii / Paper 58 / 4 / Solution

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