activity
20152022
most cited3D Turbulent Reconnection: Theory, Tests and Astrophysical Implications

201 citations · 827 across the 25 of their papers we have counts for

collaborators

34 papers

astro-ph.GA202226 cited

The Velocity Statistics of Turbulent Clouds in the Presence of Gravity, Magnetic fields, Radiation, and Outflow Feedback

Yue Hu, Christoph Federrath, Siyao Xu +1

The interaction of turbulence, magnetic fields, self-gravity, and stellar feedback within molecular clouds is crucial for understanding star formation. We study the effects of self…

astro-ph.HE202224 cited

Cosmic ray streaming in the turbulent interstellar medium

Siyao Xu, Alex Lazarian

We study the streaming instability of GeVGeV cosmic rays (CRs) and its damping in the turbulent interstellar medium (ISM). We find that the damping of streaming instability…

astro-ph.GA2022

Damping of Alfvén waves in MHD turbulence and implications for cosmic ray streaming instability and galactic winds

Alex Lazarian, Siyao Xu

Alfvénic component of MHD turbulence damps Alfvénic waves. The consequences of this effect are important for many processes, from cosmic ray (CR) propagation to launching outflows…

astro-ph.HE20211 cited

Diffusion of cosmic rays in MHD turbulence

Siyao Xu

We review some recent findings on diffusion of cosmic rays (CRs) in magnetohydrodynamic (MHD) turbulence obtained by adopting the numerically-tested model of MHD turbulence, includ…

astro-ph.GA2021

Small-scale turbulent dynamo in astrophysical environments: nonlinear dynamo and dynamo in a partially ionized plasma

Siyao Xu, Alex Lazarian

Small-scale turbulent dynamo is responsible for the amplification of magnetic fields on scales smaller than the driving scale of turbulence in diverse astrophysical media. Most ear…

astro-ph.GA2021

Anisotropic Turbulence in Position-Position-Velocity Space: Probing Three-Dimensional Magnetic Fields

Yue Hu, A. Lazarian, Siyao Xu

Direct measurements of three-dimensional magnetic fields in the interstellar medium (ISM) are not achievable. However, the anisotropic nature of magnetohydrodynamic (MHD) turbulenc…