3 citations · 4 across the 4 of their papers we have counts for
6 papers · 1 filter
Ring Spacing from a Fourth-Order Radial Feedback Green Function in a Keplerian Accretion Disk
Yiwei Bao, Can Cui
ALMA observations of protoplanetary disks reveal ubiquitous concentric ring structures whose origin remains debated. We present an exactly solvable local model for ring spacing in…
Dust Growth in ALMA Rings: II. Dusty Rossby Wave Instability
Can Cui, Konstantin Gerbig, Ya-Ping Li +5
Annular substructures serve as ideal venues for planetesimal formation. In this series, we investigate the linear stage of dust growth within rings. The first paper examines the gl…
Vertical Shear Instability with Partially Reflecting Boundary Conditions
Yuzi Wu, Cong Yu, Can Cui
The vertical shear instability (VSI) is widely believed to be effective in driving turbulence in protoplanetary disks. Prior studies on VSI exclusively exploit the reflecting bound…
Rossby wave instability in weakly ionized protoplanetary disks. II. radial B-fields
Can Cui, Zijin Wang
Building on our first paper in this series, we investigate the impact of radial magnetic fields and non-ideal magnetohydrodynamic (MHD) effects - specifically, Ohmic resistivity, H…
Rossby wave instability in weakly ionized protoplanetary disks. I. azimuthal or vertical B-fields
Can Cui, Ashutosh Tripathi, Cong Yu +2
Rossby wave instability (RWI) is considered the underlying mechanism to crescent-shaped azimuthal asymmetries, discovered in (sub-)millimeter dust continuum of many protoplanetary…
Dust Dynamics in Hall-effected Protoplanetary Disks. I. Background Drift Hall Instability
Yinhao Wu, Min-Kai Lin, Can Cui +3
Recent studies have shown that the large-scale gas dynamics of protoplanetary disks (PPDs) are controlled by non-ideal magneto-hydrodynamics (MHD), but how this influences dust dyn…