Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission

arXiv:2512.07214 · astro-ph.HE · Submitted 2025-12-08 · Read on arXiv

astro-ph.HE

Submitted: 2025-12-08

Updated: 2026-08-29

Terminology

• Core — 9× in this paper · explained in 2 episodes
• Accuracy — 3× in this paper · explained in 1 episode
• Fidelity — 2× in this paper · explained in 2 episodes
• High-Order WENO — 2× in this paper
• Adaptive Mesh Refinement — 1× in this paper
• Clustering — 1× in this paper · explained in 2 episodes
• Cold front — 1× in this paper · explained in 2 episodes
• Lagrangian Smoothed Particle Hydrodynamics — 1× in this paper
• National Research Foundation — 1× in this paper
• Trace — 1× in this paper · explained in 2 episodes
• Weak Lensing — 1× in this paper · explained in 2 episodes
• Weighted Essentially Non-Oscillatory — 1× in this paper

Sources

• Cluster Radio Relics as a Tracer of Shock Waves of the Large-Scale Structure Formation
• Exploring the statistical properties of double radio relics in the TNG-Cluster and TNG300 simulations
• Science with an ngVLA: The ngVLA Science Case and Associated Science Requirements

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