Relativistic magnetohydrodynamics (RMHD) provides an extremely useful description of the
low-energy long-wavelength phenomena in a variety of physical systems from quark–gluon …

In recent years, our understanding of gamma‐ray bursts (GRB) prompt emission has been
revolutionized, due to a combination of new instruments, new analysis methods, and novel …

We introduce a new framework of highly anisotropic hydrodynamics that includes dissipation
effects. Dissipation is defined by the form of the entropy source that depends on the pressure …

We present results from particle-in-cell simulations of driven turbulence in magnetized,
collisionless, and relativistic pair plasmas. We find that the fluctuations are consistent with …

In models of inflation driven by an axion-like pseudoscalar field, the inflaton, a, may couple
to the standard model hypercharge via a Chern-Simons-type interaction, Script L⊃ a/(4Λ) F …

Binary black hole (BBH) mergers provide a prime source for current and future
interferometric gravitational wave observatories. Massive BBH mergers may often take place …

The observations of the pulsar wind nebula (PWN) around the Vela pulsar with the
Advanced CCD Imaging Spectrometer aboard the Chandra X-Ray Observatory, taken on …

Various attempts have been made in the literature at describing the origin and the physical
mechanisms behind flaring events in blazars with radiative emission models, but detailed …

We revisit the big bang nucleosynthesis limits on primordial magnetic fields and/or turbulent
motions accounting for the decaying nature of turbulent sources between the time of …

ABSTRACT A wide variety of astrophysical phenomena involve the flow of turbulent
magnetized gas with relativistic velocity or energy density. Examples include gamma-ray …