Using two-dimensional hybrid-kinetic simulations, we explore the nonlinear "interruption" of standing and traveling shear-Alfvén waves in collisionless plasmas. Interruption involves a self-generated pressure anisotropy removing the restoring force of a linearly polarized Alfvénic perturbation, and occurs for wave amplitudes δB_⊥/B_0≳β^(−1/2) (where β is the ratio of thermal to magnetic pressure). We use highly elongated domains to obtain maximal scale separation between the wave and the ion gyroscale. For standing waves above the amplitude limit, we find that the large-scale magnetic field of the wave decays rapidly. The dynamics are strongly affected by the excitation of oblique firehose modes, which transition into long-lived parallel fl...
Hybrid-kinetic numerical simulations of firehose and mirror instabilities in a collisionless plasma ...
The relationship between a decaying strong turbulence and kinetic instabilities in a slowly expandin...
Weakly collisional magnetized cosmic plasmas have a dynamical tendency to develop pressure anisotrop...
Using two-dimensional hybrid-kinetic simulations, we explore the nonlinear "interruption" of standin...
Using two-dimensional hybrid-kinetic simulations, we explore the nonlinear "interruption" of standin...
This work, which extends Squire et al (Astrophys. J. Lett. 2016 830 L25), explores the effect of sel...
It is shown that low-collisionality plasmas cannot support linearly polarized shear-Alfvén fluctuati...
Large amplitude Alfv\'en waves tend to be unstable to parametric instabilities which result in a dec...
A dispersive Landau-fluid model is used to study the decay and modulational instabilities of circula...
It is shown that low-collisionality plasmas cannot support linearly polarized shear-Alfvén fluctuati...
We present results from three-dimensional hybrid-kinetic simulations of Alfv\'enic turbulence in a h...
Using analytical theory and hybrid-kinetic numerical simulations, we demonstrate that, in a collisio...
Magnetic energy around astrophysical compact objects can strongly dominate over plasma rest mass. Em...
The stationary inertial Alfvén (StIA) wave (Knudsen, 1996) was predicted for cold, collisionless pla...
Pressure anisotropy can strongly influence the dynamics of weakly collisional, high-beta plasmas, bu...
Hybrid-kinetic numerical simulations of firehose and mirror instabilities in a collisionless plasma ...
The relationship between a decaying strong turbulence and kinetic instabilities in a slowly expandin...
Weakly collisional magnetized cosmic plasmas have a dynamical tendency to develop pressure anisotrop...
Using two-dimensional hybrid-kinetic simulations, we explore the nonlinear "interruption" of standin...
Using two-dimensional hybrid-kinetic simulations, we explore the nonlinear "interruption" of standin...
This work, which extends Squire et al (Astrophys. J. Lett. 2016 830 L25), explores the effect of sel...
It is shown that low-collisionality plasmas cannot support linearly polarized shear-Alfvén fluctuati...
Large amplitude Alfv\'en waves tend to be unstable to parametric instabilities which result in a dec...
A dispersive Landau-fluid model is used to study the decay and modulational instabilities of circula...
It is shown that low-collisionality plasmas cannot support linearly polarized shear-Alfvén fluctuati...
We present results from three-dimensional hybrid-kinetic simulations of Alfv\'enic turbulence in a h...
Using analytical theory and hybrid-kinetic numerical simulations, we demonstrate that, in a collisio...
Magnetic energy around astrophysical compact objects can strongly dominate over plasma rest mass. Em...
The stationary inertial Alfvén (StIA) wave (Knudsen, 1996) was predicted for cold, collisionless pla...
Pressure anisotropy can strongly influence the dynamics of weakly collisional, high-beta plasmas, bu...
Hybrid-kinetic numerical simulations of firehose and mirror instabilities in a collisionless plasma ...
The relationship between a decaying strong turbulence and kinetic instabilities in a slowly expandin...
Weakly collisional magnetized cosmic plasmas have a dynamical tendency to develop pressure anisotrop...