Galaxy Cluster simulations with a spectral Cosmic Ray model -- "Wrong Way" Radio Relics
Ludwig M. B\"oss, Ulrich P. Steinwandel, Klaus Dolag

TL;DR
This paper introduces a novel spectral Cosmic Ray model integrated into galaxy cluster simulations, enabling detailed on-the-fly evolution of CR populations and providing insights into radio relic formation.
Contribution
It develops an efficient on-the-fly Fokker-Planck solver for CRs, allowing simultaneous evolution of protons and electrons in high-resolution galaxy cluster simulations.
Findings
Preliminary results suggest a new formation mechanism for 'Wrong Way' Radio Relics.
The spectral CR model captures shock acceleration, re-acceleration, and radiative processes.
Simulation results offer insights into non-thermal emissions and magnetic field structures in galaxy clusters.
Abstract
Non-thermal emission from relativistic electrons gives insight into the strength and morphology of intra-cluster magnetic fields, as well as providing powerful tracers of structure formation shocks. Emission caused by Cosmic Ray (CR) protons on the other hand still challenges current observations and is therefore testing models of proton acceleration at intra-cluster shocks. Large-scale simulations including the effects of CRs have been difficult to achieve and have been mainly reduced to simulating an overall energy budget, or tracing CR populations in post-processing of simulation output and has often been done for either protons or electrons. We use an efficient on-the-fly Fokker-Planck solver to evolve distributions of CR protons and electrons within every resolution element of our simulation. The solver accounts for CR acceleration at intra-cluster shocks, based on results of…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Solar and Space Plasma Dynamics · Radio Astronomy Observations and Technology
