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Xue-Ning Bai

Professor

Tsinghua University

China

Research Interests

Articles (20)

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2026

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2023

Collaborators (8)

Ruobing Dong

Professor

Peking University

CHINA

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Cauê Sciascia Borlina

Purdue University

UNITED STATES

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Eve Ostriker

Professor

Princeton University

UNITED STATES

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Kengo Tomida

Associate Professor

Tohoku University

JAPAN

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Chris Ormel

Professor

Tsinghua University

CHINA

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Shoji Mori

Tohoku University

JAPAN

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Ilaria Pascucci

University of Arizona

UNITED STATES

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Joanna Drazkowska

Research Group Leader

Max Planck Institute for Solar System Research

GERMANY

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Xue-Ning Bai

Research Interests

Articles (20)

Complex gas flows in magnetized protoplanetary disks promote the formation of dust traps at low fragmentation velocities

Cosmic-ray Magnetohydrodynamics: A New Two-moment Framework with Numerical Implementation

Paleomagnetic evidence for a nebular magnetic field from calcium-aluminum-rich inclusions

A Radiation Transport Module based on M1 Closure for the Athena++ MHD Code

GRACE-DG: A Discontinuous Galerkin Method–based Code for General Nonlinear Coagulation–Fragmentation Equations

Guangqi: A 2D Radiation Hydrodynamic Code with Realistic Equations of State

Magnetohydrodynamic Guiding Center Particle-in-cell Method for Multiscale Plasma Kinetic Simulations

Solving for the 2D water snowline with hydrodynamic simulations

Radiative Nonideal Magnetohydrodynamic Simulations of Inner Protoplanetary Disks: Temperature Structures, Asymmetric Winds, and Episodic Surface Accretion

Leaky Dust Traps in Planet-embedded Protoplanetary Disks

Radiation Hydrodynamics of Self-gravitating Protoplanetary Disks. I. Direct Formation of Gas Giants via Disk Fragmentation

Kinetic Simulations of the Cosmic-Ray Pressure Anisotropy Instability: Cosmic-Ray Scattering Rate in the Saturated State

Linear analysis and simulations of the cosmic-ray streaming instability: The importance of oblique waves

Dust Clumping in Outer Protoplanetary Disks: The Interplay among Four Instabilities

The Interplay between Dust Dynamics and Turbulence Induced by the Vertical Shear Instability

Small and Large Dust Cavities in Disks around Mid-M Stars in Taurus

Evidence for Magnetically‐Driven Accretion in the Distal Solar System

Dynamical Consequence of Shadows Cast to the Outer Protoplanetary Disks. I. Two-dimensional Simulations

Hydrodynamical simulations of circumbinary accretion: balance between heating and cooling

Simulations of weakly magnetized turbulent mixing layers

Collaborators (8)

Ruobing Dong

Cauê Sciascia Borlina

Eve Ostriker

Kengo Tomida

Chris Ormel

Shoji Mori

Ilaria Pascucci

Joanna Drazkowska

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