activity
20192025
most citedNon-resonant particle acceleration in strong turbulence: comparison to kinetic and MHD simulations

33 citations · 83 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2025

Particle acceleration up to the synchrotron burn-off limit in relativistic magnetized turbulence

M. Lemoine, V. Bresci, L. Gremillet

In high-energy astrophysics, interpreting observed spectra hinges on understanding the competition between energy gains and radiative losses. To progress along these lines, we repo…

astro-ph.GA2023★ 15 cited

Deciphering the physical basis of the intermediate-scale instability

Mohamad Shalaby, Timon Thomas, Christoph Pfrommer +2

We study the underlying physics of cosmic-ray (CR) driven instabilities that play a crucial role for CR transport across a wide range of scales, from interstellar to galaxy cluster…

astro-ph.HE2023★ 1 cited

Particle acceleration at magnetized, relativistic turbulent shock fronts

Virginia Bresci, Martin Lemoine, Laurent Gremillet

The efficiency of particle acceleration at shock waves in relativistic, magnetized astrophysical outflows is a debated topic with far-reaching implications. Here, for the first tim…

astro-ph.HE2022★ 33 cited

Non-resonant particle acceleration in strong turbulence: comparison to kinetic and MHD simulations

Virginia Bresci, Martin Lemoine, Laurent Gremillet +3

Collisionless, magnetized turbulence offers a promising framework for the generation of non-thermal high-energy particles in various astrophysical sites. Yet, the detailed mechanis…

physics.plasm-ph2021★ 10 cited

Saturation of the asymmetric current filamentation instability under conditions relevant to relativistic shock precursors

Virginia Bresci, Laurent Gremillet, Martin Lemoine

The current filamentation instability, which generically arises in the counterstreaming of supersonic plasma flows, is known for its ability to convert the free energy associated w…

astro-ph.HE2019★ 24 cited

Effects of reacceleration and source grammage on secondary cosmic rays spectra

Virginia Bresci, Elena Amato, Pasquale Blasi +1

The ratio between secondary and primary cosmic ray particles is the main source of information about cosmic ray propagation in the Galaxy. Primary cosmic rays are thought to be acc…