activity
20042008
most citedAngular Momentum Transport in Accretion Disks: Scaling Laws in MRI-driven Turbulence

162 citations · 403 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph200867 cited

Viscous, Resistive Magnetorotational Modes

Martin E. Pessah, Chi-kwan Chan

We carry out a comprehensive analysis of the behavior of the magnetorotational instability (MRI) in viscous, resistive plasmas. We find exact, non-linear solutions of the non-ideal…

astro-ph2007162 cited

Angular Momentum Transport in Accretion Disks: Scaling Laws in MRI-driven Turbulence

Martin E. Pessah, Chi-kwan Chan, Dimitrios Psaltis

We present a scaling law that predicts the values of the stresses obtained in numerical simulations of saturated MRI-driven turbulence in non-stratified shearing boxes. It relates…

astro-ph200647 cited

The fundamental difference between shear alpha viscosity and turbulent magnetorotational stresses

Martin E. Pessah, Chi-kwan Chan, Dimitrios Psaltis

Numerical simulations of turbulent, magnetized, differentially rotating flows driven by the magnetorotational instability are often used to calculate the effective values of alpha…

astro-ph200656 cited

A Local Model for Angular Momentum Transport in Accretion Disks Driven by the Magnetorotational Instability

Martin E. Pessah, Chi-kwan Chan, Dimitrios Psaltis

We develop a local model for the exponential growth and saturation of the Reynolds and Maxwell stresses in turbulent flows driven by the magnetorotational instability. We first der…

astro-ph200671 cited

The signature of the magnetorotational instability in the Reynolds and Maxwell stress tensors in accretion discs

Martin E. Pessah, Chi-kwan Chan, Dimitrios Psaltis

The magnetorotational instability is thought to be responsible for the generation of magnetohydrodynamic turbulence that leads to enhanced outward angular momentum transport in acc…

astro-ph2004

The Stability of Magnetized Rotating Plasmas with Superthermal Fields

Martin E. Pessah, Dimitrios Psaltis

During the last decade it has become evident that the magnetorotational instability is at the heart of the enhanced angular momentum transport in weakly magnetized accretion disks…