activity
19962024
most citedSpectrum of magnetohydrodynamic turbulence

591 citations · 4.7k across the 90 of their papers we have counts for

collaborators

92 papers

physics.plasm-ph2024

Relativistic Alfvén turbulence at kinetic scales

Cristian Vega, Stanislav Boldyrev, Vadim Roytershteyn

In a strongly magnetized, magnetically dominated relativistic plasma, Alfvénic turbulence can extend to scales much smaller than the particle inertial scales. It leads to an energy…

physics.plasm-ph2023★ 7 cited

Electron-Scale Current Sheets and Energy Dissipation in 3D Kinetic-Scale Plasma Turbulence with Low Electron Beta

Cristian Vega, Vadim Roytershteyn, Gian Luca Delzanno +1

3D kinetic-scale turbulence is studied numerically in the regime where electrons are strongly magnetized (the ratio of plasma species pressure to magnetic pressure is for…

physics.plasm-ph2023★ 10 cited

Spatial intermittency of particle distribution in relativistic plasma turbulence

Cristian Vega, Stanislav Boldyrev, Vadim Roytershteyn

Relativistic magnetically dominated turbulence is an efficient engine for particle acceleration in a collisionless plasma. Ultrarelativistic particles accelerated by interactions w…

physics.space-ph2022

The Heliospheric Ambipolar Potential Inferred from Sunward-Propagating Halo Electrons

Konstantinos Horaites, Stanislav Boldyrev

We provide evidence that the sunward-propagating half of the solar wind electron halo distribution evolves without scattering in the inner heliosphere. We assume the particles cons…

physics.plasm-ph2022★ 11 cited

Spectra of magnetic turbulence in a relativistic plasma

Cristian Vega, Stanislav Boldyrev, Vadim Roytershteyn

We present a phenomenological and numerical study of strong Alfvénic turbulence in a magnetically dominated collisionless relativistic plasma with a strong background magnetic fiel…

physics.plasm-ph2021★ 24 cited

Turbulence and particle acceleration in a relativistic plasma

Cristian Vega, Stanislav Boldyrev, Vadim Roytershteyn +1

In a collisionless plasma, the energy distribution function of plasma particles can be strongly affected by turbulence. In particular, it can develop a non-thermal power-law tail a…