activity
20082013
most citedAssessing Quantitative Results in Accretion Simulations: From Local to Global

226 citations · 733 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2013★ 28 cited

Relativistic MHD Simulations of Poynting Flux-Driven Jets

Xiaoyue Guan, Hui Li, Shengtai Li

Relativistic, magnetized jets are observed to propagate to very large distances in many Active Galactic Nuclei (AGN). We use 3D relativistic MHD (RMHD) simulations to study the pro…

astro-ph.IM2013★ 133 cited

Testing Convergence for Global Accretion Disks

John F. Hawley, Sherwood A. Richers, Xiaoyue Guan +1

Global disk simulations provide a powerful tool for investigating accretion and the underlying magnetohydrodynamic turbulence driven by the magneto-rotational instability (MRI). Us…

astro-ph.HE2011★ 226 cited

Assessing Quantitative Results in Accretion Simulations: From Local to Global

John F. Hawley, Xiaoyue Guan, Julian H. Krolik

Discretized numerical simulations are a powerful tool for investigation of nonlinear MHD turbulence in accretion disks. However, confidence in their quantitative predictions requir…

astro-ph.HE2010★ 69 cited

Radially Extended, Stratified, Local Models of Isothermal Disks

Xiaoyue Guan, Charles F. Gammie

We consider local, stratified, numerical models of isothermal accretion disks. The novel feature of our treatment is that radial extent L_x and azimuthal extent L_y satisfy H << L_…

astro-ph.HE2009★ 120 cited

The Turbulent Magnetic Prandtl Number of MHD Turbulence in Disks

Xiaoyue Guan, Charles F. Gammie

The magnetic Prandtl number Pr_M is the ratio of viscosity to resistivity. In astrophysical disks the diffusion of angular momentum (viscosity) and magnetic fields (resistivity) ar…

astro-ph.GA2009★ 108 cited

Locality of MHD Turbulence in Isothermal Disks

Xiaoyue Guan, Charles F. Gammie, Jacob B. Simon +1

We numerically evolve turbulence driven by the magnetorotational instability (MRI) in a 3D, unstratified shearing box and study its structure using two-point correlation functions.…