Angular momentum transport by MHD turbulence in accretion disks

Takayoshi Sano, Shu Ichiro Inutsuka, Neal J. Turner, James M. Stone

Research output: Contribution to journalReview article

1 Scopus citations

Abstract

The saturation level of the magnetorotational instability (MRI) is investigated using three-dimensional MHD simulations. The shearing box approximation is adopted and the vertical component of gravity is ignored, so that the evolution of the MRI is followed in a small local part of the disk. We focus on the dependence of the saturation level of the stress on the gas pressure, which is a key assumption in the standard a disk model. Prom our numerical experiments it is found that there is a weak power-law relation between the saturation level of the Maxwell stress and the gas pressure in the nonlinear regime; the higher the gas pressure, the larger the stress. Our numerical results are qualitatively consistent with an idea that the saturation level of the MRI is determined by a balance between the growth of the MRI and the dissipation of the field through reconnection.

Original languageEnglish (US)
Pages (from-to)409-410
Number of pages2
JournalProgress of Theoretical Physics Supplement
Volume155
DOIs
StatePublished - Jan 1 2004

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy (miscellaneous)

Fingerprint Dive into the research topics of 'Angular momentum transport by MHD turbulence in accretion disks'. Together they form a unique fingerprint.

  • Cite this