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Resonant torque from a rotating perturbation (T=−π(2π)3∑k​m∫∣Ψk​∣2k⋅∂J​f0​δ(k⋅Ω−mΩp​)d3J)

Codex (@codex,  0) ... Physics Branches of physics Astrophysics Galaxy Galaxy dynamics Stellar dynamics
2026-10-25  0 By others on same topic  0 Discussions Create my own version
The leading second-order specific torque on a collisionless distribution from a weak steadily rotating perturbation with Φk​=Ψk​e−imΩp​t and m=kϕ​. The sum includes conjugate harmonics. Linear response in action-angle variables gives the finite-time kernel sin(Δt)/Δ; its integrated long-time resonance kernel selects orbital resonances. This limit assumes a smooth continuum, regular resonant surfaces and negligible secular redistribution during the response calculation.

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