activity
20122023
most cited3D Turbulent Reconnection: Theory, Tests and Astrophysical Implications

201 citations · 2k across the 65 of their papers we have counts for

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28 papers · 1 filter

astro-ph.HE2023

Numerical testing of mirror diffusion of cosmic rays

Chao Zhang, Siyao Xu

The tension between recent observations and theories on cosmic ray (CR) diffusion necessitates exploration of new CR diffusion mechanisms. We perform the first numerical study on t…

astro-ph.HE2023

Mirror acceleration of cosmic rays in a high- medium

Alex Lazarian, Siyao Xu

In a weakly compressible high- medium, pitch-angle scattering and the associated scattering acceleration of cosmic rays (CRs) by anisotropic Alfvén and slow modes of magnetohydr…

astro-ph.HE2022★ 39 cited

Faraday Rotation Measure Variations of Repeating Fast Radio Burst Sources

Yuan-Pei Yang, Siyao Xu, Bing Zhang

Recently, some fast radio burst (FRB) repeaters were reported to exhibit complex, diverse variations of Faraday rotation measures (RMs), which implies that they are surrounded by a…

astro-ph.HE2022★ 24 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.HE2021★ 23 cited

Shock acceleration with oblique and turbulent magnetic fields

Siyao Xu, Alex Lazarian

We investigate shock acceleration in a realistic astrophysical environment with density inhomogeneities. The turbulence induced by the interaction of the shock precursor with upstr…

astro-ph.HE2021★ 1 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.HE2021★ 18 cited

Mirror diffusion of cosmic rays in highly compressible turbulence near supernova remnants

Siyao Xu

Recent gamma-ray observations reveal inhomogeneous diffusion of cosmic rays (CRs) in the interstellar medium (ISM). This is expected as the diffusion of CRs depends on the properti…

astro-ph.HE2021★ 68 cited

Diffusion of cosmic rays in MHD turbulence with magnetic mirrors

Alex Lazarian, Siyao Xu

As the fundamental physical process with many astrophysical implications, the diffusion of cosmic rays (CRs) is determined by their interaction with magnetohydrodynamic (MHD) turbu…

astro-ph.HE2021★ 19 cited

Polarization Predictions in the GRB Prompt Phase with the Internal Shock Model

Mi-Xiang Lan, Hao-Bing Wang, Siyao Xu +2

As the standard gamma-ray burst (GRB) prompt-emission model, the internal shock (IS) model can reproduce the fast-rise and slow-decay features of the pulses in the GRB light curve.…

astro-ph.HE2020★ 22 cited

Probing the intergalactic turbulence with fast radio bursts

Siyao Xu, Bing Zhang

The turbulence in the diffuse intergalactic medium (IGM) plays an important role in various astrophysical processes across cosmic time, but it is very challenging to constrain its…

astro-ph.HE2020★ 13 cited

Nanoflare Theory Revisited

Amir Jafari, Ethan Vishniac, Siyao Xu

Local magnetic reversals are an inseparable part of magnetohydrodynamic (MHD) turbulence whose collective outcome on an arbitrary scale in the inertial range may lead to a global s…

astro-ph.HE2020★ 36 cited

Trapping of cosmic rays in MHD turbulence

Siyao Xu, Alex Lazarian

Astrophysical plasmas are turbulent and magnetized. The interaction between cosmic rays (CRs) and magnetohydrodynamic (MHD) turbulence is a fundamental astrophysical process. Based…

astro-ph.HE2020★ 201 cited

3D Turbulent Reconnection: Theory, Tests and Astrophysical Implications

Alex Lazarian, Gregory L. Eyink, Amir Jafari +4

Magnetic reconnection, topological change in magnetic fields, is a fundamental process in magnetized plasmas. It is associated with energy release in regions of magnetic field anni…

astro-ph.HE2019★ 1 cited

Synchrotron spectra of GRB prompt emission and pulsar wind nebulae

Siyao Xu

Particle acceleration is a fundamental process in many high-energy astrophysical environments and determines the spectral features of their synchrotron emission. We have studied th…

astro-ph.HE2019★ 87 cited

Cosmic ray transport in starburst galaxies

Mark R. Krumholz, Roland M. Crocker, Siyao Xu +3

Starburst galaxies are efficient -ray producers, because their high supernova rates generate copious cosmic ray (CR) protons, and their high gas densities act as thick targets o…

astro-ph.HE2018★ 24 cited

On the broad-band synchrotron spectra of pulsar wind nebulae

Siyao Xu, Noel Klingler, Oleg Kargaltsev +1

As shown by broad-band observations, pulsar wind nebulae (PWNe) are characterized by a broken power-law spectrum of synchrotron emission. Based on the modern magnetohydrodynamic (M…

astro-ph.HE2018★ 42 cited

Resonance-broadened transit time damping of particles in MHD turbulence

Siyao Xu, Alex Lazarian

As a fundamental astrophysical process, the scattering of particles by turbulent magnetic fields has its physical foundation laid by the magnetohydrodynamic (MHD) turbulence theory…

astro-ph.HE2018★ 33 cited

Gamma-ray Bursts Induced by Turbulent Reconnection

Alex Lazarian, Bing Zhang, Siyao Xu

We consider a simple model for gamma-ray bursts induced by magnetic reconnection in turbulent media. The magnetic field in a jet is subject to kink instabilities, which distort the…

astro-ph.HE2017★ 21 cited

On the synchrotron spectrum of GRB prompt emission

Siyao Xu, Yuan-Pei Yang, Bing Zhang

The prompt emission spectrum of Gamma-ray bursts (GRB) is characterized by a smoothly joint broken power-law spectrum known as the Band function. The typical low-energy photon inde…

astro-ph.HE2017★ 36 cited

Magnetic field amplification in supernova remnants

Siyao Xu, Alex Lazarian

Based on the new findings on the turbulent dynamo in \citet{XL16}, we examine the magnetic field amplification in the context of supernova remnants. Due to the strong ion-neutral c…

astro-ph.HE2017★ 39 cited

Adiabatic non-resonant acceleration in magnetic turbulence and hard spectra of gamma-ray bursts

Siyao Xu, Bing Zhang

We introduce a non-resonant acceleration mechanism arising from the second adiabatic invariant in magnetic turbulence and apply it to study the prompt emission spectra of gamma-ray…

astro-ph.HE2016★ 18 cited

TeV Cosmic-Ray Anisotropy from the Magnetic Field at the Heliospheric Boundary

Vanessa López-Barquero, S. Xu, P. Desiati +3

We performed numerical calculations to test the suggestion by Desiati & Lazarian (2013) that the anisotropies of TeV cosmic rays may arise from their interactions with the heliosph…

astro-ph.HE2016★ 48 cited

On the origin of the scatter broadening of fast radio burst pulses and astrophysical implications

Siyao Xu, Bing Zhang

Fast radio bursts (FRBs) have been identified as extragalactic sources which can make a probe of turbulence in the intergalactic medium (IGM) and their host galaxies. To account fo…

astro-ph.HE2015★ 29 cited

Cosmic Ray Small Scale Anisotropies and Local Turbulent Magnetic Fields

Vanessa López-Barquero, R. Farber, S. Xu +2

Cosmic ray anisotropy has been observed in a wide energy range and at different angular scales by a variety of experiments over the past decade. However, no comprehensive or satisf…