activity
20102023
most citedFuture Physics Programme of BESIII

566 citations · 4.6k across the 89 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

31 papers · 1 filter

astro-ph.HE2023★ 18 cited

A Model for Nonthermal Particle Acceleration in Relativistic Magnetic Reconnection

Xiaocan Li, Fan Guo, Yi-Hsin Liu +1

The past decade has seen an outstanding development of nonthermal particle acceleration in magnetic reconnection in magnetically-dominated systems, with clear signatures of power-l…

astro-ph.HE2023★ 24 cited

First-Principle-Integrated Study of Blazar Synchrotron Radiation and Polarization Signatures from Magnetic Turbulence

Haocheng Zhang, Alan Marscher, Fan Guo +3

Blazar emission is dominated by nonthermal radiation processes that are highly variable across the entire electromagnetic spectrum. Turbulence, which can be a major source of nonth…

astro-ph.HE2022★ 51 cited

Particle Injection and Nonthermal Particle Acceleration in Relativistic Magnetic Reconnection

Omar French, Fan Guo, Qile Zhang +1

Magnetic reconnection in the relativistic regime has been proposed as an important process for the efficient production of nonthermal particles and high-energy emissions. Using ful…

astro-ph.HE2022★ 13 cited

Comment on "Nonideal Fields Solve the Injection Problem in Relativistic Reconnection"

Fan Guo, Xiaocan Li, Omar French +7

Recently, Sironi (PRL, 128, 145102; S22) reported the correlation between particles accelerated into high energy and their crossings of regions with electric field larger than magn…

astro-ph.HE2022★ 1 cited

Modeling the inner part of M87 jet: confronting jet morphology with theory

Hai Yang, Feng Yuan, Hui Li +5

The formation of jets in black hole accretion systems is a long-standing problem. It has been proposed that a jet can be formed by extracting the rotation energy of the black hole…

astro-ph.HE2021

Radiation and Polarization Signatures from Magnetic Reconnection in Relativistic Jets--II. Connection with -rays

Haocheng Zhang, Xiaocan Li, Dimitrios Giannios +5

It is commonly believed that blazar jets are relativistic magnetized plasma outflows from supermassive black holes. One key question is how the jets dissipate magnetic energy to ac…

astro-ph.HE2021★ 16 cited

First-Principle Prediction of X-ray Polarization from Magnetic Reconnection in High-Frequency BL Lacs

Haocheng Zhang, Xiaocan Li, Dimitrios Giannios +1

Relativistic magnetic reconnection is a potential particle acceleration mechanism for high-frequency BL Lacs (HBLs). The {\it Imaging X-ray Polarimetry Explorer} ({\it IXPE}) sched…

astro-ph.HE2020★ 23 cited

Fermi-type particle acceleration from magnetic reconnection at the termination shock of a relativistic striped wind

Yingchao Lu, Fan Guo, Patrick Kilian +3

An oblique-rotating pulsar generates a relativistic striped wind in a pulsar wind nebula (PWN). The termination shock of the PWN compresses the Poynting-flux-dominated flow and dri…

astro-ph.HE2020★ 42 cited

Radiation and Polarization Signatures from Magnetic Reconnection in Relativistic Jets--I. A Systematic Study

Haocheng Zhang, Xiaocan Li, Dimitrios Giannios +3

Blazars are relativistic magnetized plasma outflows from supermassive black holes that point very close to our line of sight. Their emission is nonthermal dominated and highly vari…

astro-ph.HE2020★ 66 cited

Magnetic Energy Release, Plasma Dynamics, and Particle Acceleration during Relativistic Turbulent Magnetic Reconnection

Fan Guo, Xiaocan Li, William Daughton +5

In strongly magnetized astrophysical plasma systems, magnetic reconnection is believed to be a primary process during which explosive energy release and particle acceleration occur…

astro-ph.HE2020★ 76 cited

Recent Progress on Particle Acceleration and Reconnection Physics during Magnetic Reconnectionin the Magnetically-dominated Relativistic Regime

Fan Guo, Yi-Hsin Liu, Xiaocan Li +3

Magnetic reconnection in strongly magnetized astrophysical plasma environments is believed to be the primary process for fast energy release and particle energization. Currently th…

astro-ph.HE2020★ 39 cited

Exploring the acceleration mechanisms for particle injection and power-law formation during trans-relativistic magnetic reconnection

Patrick Kilian, Xiaocan Li, Fan Guo +1

Magnetic reconnection in the relativistic and trans-relativistic regimes is able to accelerate particles to hard power law energy spectra (approaching ). Th…

astro-ph.HE2019★ 18 cited

The Critical Role of Collisionless Plasma Energization on the Structure of Relativistic Magnetic Reconnection

Yi-Hsin Liu, Shan-Chang Lin, Michael Hesse +4

During magnetically dominated relativistic reconnection, inflowing plasma depletes the initial relativistic pressure at the x-line and collisionless plasma heating inside the diffu…

astro-ph.HE2019

Neutrinos, Cosmic Rays and the MeV Band

R. Ojha, H. Zhang, M. Kadler +23

The possible association of the blazar TXS 0506+056 with a high-energy neutrino detected by IceCube holds the tantalizing potential to answer three astrophysical questions: 1. Wher…

astro-ph.HE2019★ 4 cited

High-Energy Polarimetry - a new window to probe extreme physics in AGN jets

B. Rani, H. Zhang, S. D. Hunter +31

The constantly improving sensitivity of ground-based and space-borne observatories has made possible the detection of high-energy emission (X-rays and gamma-rays) from several thou…

astro-ph.HE2019★ 71 cited

Determining the Dominant Acceleration Mechanism during Relativistic Magnetic Reconnection in Large-scale Systems

Fan Guo, Xiaocan Li, William Daughton +5

While a growing body of research indicates that relativistic magnetic reconnection is a prodigious source of particle acceleration in high-energy astrophysical systems, the dominan…

astro-ph.HE2018★ 67 cited

Large-Amplitude Blazar Polarization Angle Swing as a Signature of Magnetic Reconnection

Haocheng Zhang, Xiaocan Li, Fan Guo +1

Relativistic magnetic reconnection events can widely exist in magnetized plasmas in astrophysical systems. During this process, oppositely directed magnetic field lines reconnect a…

astro-ph.HE2017★ 528 cited

Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth

A. U. Abeysekara, A. Albert, R. Alfaro +113

The unexpectedly high flux of cosmic ray positrons detected at Earth may originate from nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary prod…

astro-ph.HE2016★ 40 cited

Polarization Signatures of Kink Instabilities in the Blazar Emission Region from Relativistic Magnetohydrodynamic Simulations

Haocheng Zhang, Hui Li, Fan Guo +1

Kink instabilities are likely to occur in the current-carrying magnetized plasma jets. Recent observations of the blazar radiation and polarization signatures suggest that the blaz…

astro-ph.HE2016★ 2 cited

A model of global magnetic reconnection rate in relativistic collisionless plasmas

Yi-Hsin Liu, Michael Hesse, Fan Guo +2

A model of global magnetic reconnection rate in relativistic collisionless plasmas is developed and validated by the fully kinetic simulation. Through considering the force balance…

astro-ph.HE2016★ 33 cited

Particle Acceleration during Magnetic Reconnection in a Low-beta Pair Plasma

Fan Guo, Hui Li, William Daughton +2

Plasma energization through magnetic reconnection in the magnetically-dominated regime featured by low plasma beta () and/or high magnetization ($σ= B^2/(4 π…

astro-ph.HE2015★ 134 cited

Efficient Production of High-energy Nonthermal Particles during Magnetic Reconnection in a Magnetically-dominated Ion-Electron Plasma

Fan Guo, Xiaocan Li, Hui Li +6

Magnetic reconnection is a leading mechanism for dissipating magnetic energy and accelerating nonthermal particles in Poynting-flux dominated flows. In this letter, we investigate…

astro-ph.HE2015★ 8 cited

Particle Acceleration and Plasma Dynamics during Magnetic Reconnection in the Magnetically-dominated Regime

Fan Guo, Yi-Hsin Liu, William Daughton +1

Magnetic reconnection is thought to be the driver for many explosive phenomena in the universe. The energy release and particle acceleration during reconnection have been proposed…

astro-ph.HE2015★ 88 cited

Polarization Swings Reveal Magnetic Energy Dissipation in Blazars

Haocheng Zhang, Xuhui Chen, Markus Boettcher +2

The polarization signatures of the blazar emissions are known to be highly variable. In addition to small fluctuations of the polarization angle around a mean value, sometimes larg…