title: Convection Scaling Laws
section: Introduction
head: Overview
o Part of The Quest, to show
- Astrophysics indepedent of diffusion coefficients
- Magnetic dissipation independent of eta
- Dynamo properties independent of eta and nu
- Convection independent of nu and kappa
o Classical Polytropes
- Radiative polytropic indices
o Problems and Constraints
- Large radiative fluxes
- Large range of temperatures
o Convection Dominated Polytropes
- Energy diffusion ~ entropy gradient
- Much better test benches
- Allow clean tests of, e.g.,
- Prandtl number dependence
- Time dependent MLT
o Conclusions
- Evidence for Prandtl number independence
- Overall scaling ~ Mixing Length Theory
- Because of overturning / mass conservation
head: The Quest
text: From the ironic point of view, this is just a self-cleansing
process among theoreticians. Most astrophysicist just take the
final outcome for granted, and go about doing more
productive things!
end:
box: The Quest: To show that / demonstrate why / large
scale, turbulent phenomena in Astrophysics are, in general, independent
of details of the microphysics, such as coefficients of
viscosity, thermal and electrical conductivity.
end:
text: There are of course interesting exceptions, where things
clearly depend on collision cross sections and the like:
end:
o Non-LTE radiative transfer
o Almost collisionless plasmas
- Particle acceleration
- Non-thermal emission
head: Boiling Stars
o A long tradition of Reynolds and Rayleigh number worshipping
- Astrophysics turbulence has so high Reynolds numbers
- Stellar convection has so low Prandtl numbers
o Often used in applications for super-computer time
- And not in the sense "let's show it does not matter"
box: If it really was the case that it mattered, then by the shear size of the dimensionless numbers we could all pack and go home, and those supercomputer applications should be turned down from the start. end:
o Simple polytropic models have been used traditionally - Suitable for parameter studies(?)