Astronomy and astrophysics Definition
Mixing length theory
Builds on Schwarzschild criterion for convectionHydrostatic equilibrium
Definition
Consider a convective layer of a star in hydrostatic equilibrium. Let , and be its pressure, density and temperature, the local gravity and the specific heat at constant pressure. Let be the pressure scale height and . Let be the gradient of the surroundings and the gradient followed by a moving blob, with . Mixing length theory with parameter models convection by blobs that travel a mean distance before they dissolve. The distance is the mixing length, and the theory sets, as averages over the blobs:
- the temperature excess of a blob, ;
- the blob speed, ;
- the convective flux, .
Remarks
Combining the three clauses gives The numerical factors and come from averaging over blobs that have travelled between and . Other versions of the theory use other factors, which change the fitted value of . Example: in the deep convective envelope of the Sun the density is high. So a tiny excess already carries the whole luminosity, and is very close to the adiabatic gradient. Non-example: in a layer with , stable by the Schwarzschild criterion, a displaced blob returns, and the model gives no convective flux. Solar models usually need between about and .
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Further reading
About this page
| Tag | MS1Q8E9YS4 |
|---|---|
| URI | m2://MS1Q8E9YS4 |
| Kind | definition |
| Writing | W0 stub |
| MSC | 85A15, 85A30 |
| Defines | Mixing length theory |
| Uses | Schwarzschild criterion for convection, Hydrostatic equilibrium |
| Changed | 3 November 2026 |
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