Electron Preacceleration at Weak Quasi-perpendicular Intracluster Shocks: Effects of Preexisting Nonthermal Electrons
Ji-Hoon Ha (1), Dongsu Ryu (1), Hyesung Kang (2), Sunjung Kim (1) ((1), UNIST, Korea, (2) Pusan National University, Korea)

TL;DR
This study investigates whether preexisting nonthermal electrons can facilitate electron preacceleration at weak quasi-perpendicular shocks in galaxy clusters, finding that they do not significantly aid in the injection process for diffusive shock acceleration.
Contribution
The paper demonstrates through PIC simulations that preexisting nonthermal electrons do not enhance ion reflection or ion-scale wave generation, thus not resolving electron preacceleration at subcritical shocks.
Findings
Suprathermal electrons enhance electron-scale wave excitation.
Ion reflection and ion-scale wave generation remain unaffected.
Preexisting nonthermal electrons do not improve electron injection at weak shocks.
Abstract
Radio relics in the outskirts of galaxy clusters imply the diffusive shock acceleration (DSA) of electrons at merger-driven shocks with Mach number in the intracluster medium (ICM). Recent studies have suggested that electron preacceleration and injection, prerequisite steps for DSA, could occur at supercritical shocks with in the ICM, thanks to the generation of multiscale waves by microinstabilities such as the Alfv\'en ion cyclotron (AIC) instability, the electron firehose instability (EFI), and the whistler instability (WI). On the other hand, some relics are observed to have subcritical shocks with , leaving DSA at such weak shocks as an outstanding problem. Reacceleration of preexisting nonthermal electrons has been contemplated as one of possible solutions for that puzzle. To explore this idea, we perform Particle-in-Cell…
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Taxonomy
TopicsDust and Plasma Wave Phenomena · Laser-Plasma Interactions and Diagnostics · Magnetic confinement fusion research
