8 citations · 8 across the 3 of their papers we have counts for
5 papers
Sparking Dynamic, Relativistic Magnetic Reconnection in a Twisted Flux Tube
Michael P. Grehan, Christopher Thompson, Bart Ripperda +1
Magnetic reconnection around neutron stars (NSs) forms small-scale currents while transferring energy to electron-positron pairs. These dissipating currents cover a wide range of s…
Supernovae drive large-scale, incompressible turbulence through small-scale instabilities
James R. Beattie
The sources of turbulence in our Galaxy may be diverse, but core-collapse supernovae (SNe) alone provide enough energy to sustain a steady-state galactic turbulence cascade at the…
Cascading from the winds to the disk: the universality of supernovae-driven turbulence in different galactic interstellar media
Isabelle Connor, James R. Beattie, Anne Noer Kolborg +1
Star-forming galaxies are in a state of turbulence, with one of the principle components of the turbulence sourced by the constant injection of momentum from supernovae (SNe) explo…
Local relaxation and scale-dependent alignment in compressible, magnetized turbulence
James R. Beattie, Amitava Bhattacharjee
Driven net- and no-net-flux MHD turbulence simulations up to reveal sign-mixed velocity--magnetic, velocity--vorticity, and magnetic--current aligned patches below the…
Comparison of magnetic diffusion and reconnection in ideal and resistive relativistic magnetohydrodynamics, ideal magnetodynamics, and resistive force-free electrodynamics
Michael P. Grehan, Tanisha Ghosal, James R. Beattie +3
High-energy astrophysical systems and compact objects are frequently modeled using ideal relativistic magnetohydrodynamic (MHD) or force-free electrodynamic (FFE) simulations, with…