activity
20062024
most citedThe Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview

1.1k citations · 10.6k across the 78 of their papers we have counts for

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Showing astro-ph.HEShow all

16 papers · 1 filter

astro-ph.HE2023★ 17 cited

The Magnetohydrodynamic-Particle-In-Cell Module in Athena++: Implementation and Code Tests

Xiaochen Sun, Xue-Ning Bai

We present a new magnetohydrodynamic-particle-in-cell (MHD-PIC) code integrated into the Athena++ framework. It treats energetic particles as in conventional PIC codes while the re…

astro-ph.HE2022★ 21 cited

On the Role of Gas Cooling in the Dynamics of Circumbinary Disks

Hai-Yang Wang, Xue-Ning Bai, Dong Lai

Hydrodynamical interactions between binaries and circumbinary disks (CBDs) play an important role in a variety of astrophysical systems, from young stellar binaries to supermassive…

astro-ph.HE2022★ 2 cited

Hydrodynamical Simulations of Circumbinary Accretion: Balance between Heating and Cooling

Hai-Yang Wang, Xue-Ning Bai, Dong Lai +1

Hydrodynamical interaction in circumbinary discs (CBDs) plays a crucial role in various astrophysical systems, ranging from young stellar binaries to supermassive black hole binari…

astro-ph.HE2022★ 22 cited

Magnetic Flux Transport in Radiatively Inefficient Accretion Flows and the Pathway towards a Magnetically Arrested Disk

Prasun Dhang, Xue-Ning Bai, Christopher J. White

Large-scale magnetic fields play a vital role in determining the angular momentum transport and generating jets/outflows in the accreting systems, yet their origin remains poorly u…

astro-ph.HE2021★ 22 cited

Towards First-principle Characterization of Cosmic-ray Transport Coefficients from Multi-scale Kinetic Simulations

Xue-Ning Bai

A major uncertainty in understanding the transport and feedback of cosmic-rays (CRs) within and beyond our Galaxy lies in the unknown CR scattering rates, which are primarily deter…

astro-ph.HE2021★ 24 cited

Particle Diffusion and Acceleration in Magnetorotational Instability Turbulence

Xiaochen Sun, Xue-Ning Bai

Hot accretion flows contain collisionless plasmas that are believed to be capable of accelerating particles to very high energies, as a result of turbulence generated by the magnet…