From the 1 of 8 linked papers with an AI index.
1 citations · 1 across the 3 of their papers we have counts for
8 papers
Modeling the Evolution of Protoplanetary Disks: Two Pathways from Gravitational Instability to MHD Wind-Driven Accretion
Yang Ni, Wenrui Xu, Xue-Ning Bai
The paper introduces a semi‑two‑dimensional model of protoplanetary disk evolution that includes gravitational instability, MHD winds, MRI, and radiative effects, and shows that th…
Angular Momentum Transport in Protoplanetary Disks
Xue-Ning Bai
We review our current understanding on the physical processes that govern angular momentum transport and evolution of protoplanetary disks. Extremely rich in physics, these process…
Complex gas flows in magnetized protoplanetary disks promote the formation of dust traps at low fragmentation velocities
Vignesh Vaikundaraman, Joanna Drazkowska, Nerea Gurrutxaga +1
Non-ideal magnetohydrodynamic simulations of protoplanetary disks show a plethora of complex gas structures, including winds, rings, and gaps. These affect dust transport and help…
Radiative Nonideal MHD Simulations of Inner Protoplanetary Disks: Temperature Structures, Asymmetric Winds, and Episodic Surface Accretion
Shoji Mori, Xue-Ning Bai, Kengo Tomida
We perform two-dimensional global magnetohydrodynamic (MHD) simulations including the full nonideal MHD effects (Ohmic diffusion, Hall effect, and ambipolar diffusion) and approxim…
Leaky Dust Traps in Planet-Embedded Protoplanetary Disks
Pinghui Huang, Fangyuan Yu, Eve J. Lee +2
From the survival of dust disks for a few Myr to the establishment of chemical dichotomy, dust traps are expected to play a pivotal role in sculpting protoplanetary disks and the e…
The Interplay between Dust Dynamics and Turbulence Induced by the Vertical Shear Instability
Pinghui Huang, Xue-Ning Bai
The interaction between gas and dust in protoplanetary disks (PPDs) plays a crucial role in setting the stage of planet formation. In particular, the streaming instability (SI) is…