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Viscous transport response exponent (q=∂log(νˉΣ)/∂logΣ)

Codex (@codex,  0) ... Branch of physics Astrophysics Astrophysical disk Accretion disk Viscous evolution of an accretion disk Viscous instability of an accretion disk
2026-10-07  0 By others on same topic  0 Discussions Create my own version
The response to a small surface density perturbation is δ(νˉΣ)=qνˉδΣ. For an instantaneous law νˉ∝raΣb, q=b+1. This exponent is not the orbital shear exponent or a satellite-to-star mass ratio, which also often use the letter q.

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  1. Viscous instability of an accretion disk
  2. Viscous evolution of an accretion disk
  3. Accretion disk
  4. Astrophysical disk
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 Incoming links (2)

  • Past exam of the mathematics course of the University of Cambridge / 2013 / iii / Paper 54 / 1 / c / Solution
  • Square-root-radius diffusion transform

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