Afterglow radiation in gamma-ray bursts (GRB), extending from the radio band to GeV
energies, is produced as a result of the interaction between the relativistic jet and the …

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

GRB 221009A is a bright gamma-ray burst (GRB) with isotropic energy larger than 10 54
erg. Its fairly low redshift makes it a promising candidate for high-energy neutrino detection …

We present an analytical solution of a highly magnetized jet/wind flow. The left side of the
general force-free jet/wind equation (the" pulsar" equation) is separated into a rotating and a …

Time-resolved linear polarization (Π) measurements of the prompt gamma-ray burst
emission can reveal its dominant radiation mechanism. A widely considered mechanism is …

Very high energy (VHE) emission is usually interpreted in the synchrotron self-Compton
scenario and expected from the low-redshift and high-luminosity gamma-ray bursts (GRBs) …

The composition of gamma-ray burst (GRB) jets remained a mystery until recently. In
practice, we usually characterize the magnetization of the GRB jets (σ 0) through the ratio …

The ubiquitous turbulence in astrophysical plasmas is important for both magnetic
reconnection and reconnection acceleration. We study the particle acceleration during fast …

The theoretical prediction that magnetic reconnection spontaneously drives turbulence has
been supported by magnetohydrodynamic (MHD) and kinetic simulations. While …

Recently, a kilonova-associated gamma-ray burst (GRB 211211A), whose light curve
consists of a precursor (∼ 0.2 s), a hard spiky emission (∼ 10 s), and a soft long extended …