The stress-pressure relationship in simulations of MRI-induced turbulence
Johnathan Ross, Henrik N. Latter, Jerome Guilet

TL;DR
This study investigates how MRI-induced turbulent stresses depend on gas pressure in simulations, revealing a stronger relationship than previously thought and highlighting issues with numerical convergence and the influence of imposed magnetic flux.
Contribution
The paper demonstrates that the stress-pressure relationship in MRI turbulence is stronger than earlier reports suggested, emphasizing the importance of physical diffusivities and box size in simulations.
Findings
Stress proportional to P^{0.5} without physical diffusion
Stress approaches P^{0.9} with physical diffusivities
Numerical convergence issues affect stress-pressure relationship
Abstract
We determine how MRI-turbulent stresses depend on gas pressure via a suite of unstratified shearing box simulations. Earlier numerical work reported only a very weak dependence at best, results that call into question the canonical alpha-disk model and the thermal stability results that follow from it. Our simulations, in contrast, exhibit a stronger relationship, and show that previous work was box-size limited: turbulent `eddies' were artificially restricted by the numerical domain rather than by the scale height. Zero-net-flux runs without physical diffusion coefficients yield a stress proportional to , where P is pressure. The stresses are also proportional to the grid length and hence remain numerically unconverged. The same runs with physical diffusivities, however, give a result closer to an alpha-disk: the stress is proportional to . Net-flux simulations…
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