Sound-wave instabilities in dilute plasmas with cosmic rays: Implications for cosmic ray confinement and the Perseus X-ray ripples

Physics

• Intracluster Medium 100%
• Sound Wave 100%
• Thermal Plasma 100%
• Collisional Plasmas 100%
• Galaxy Halos 100%
• Magnetohydrodynamic Generator 50%
• Anisotropy 50%
• Gas Pressure 50%
• Galaxy Clusters 50%
• Galactic Cluster 50%
• Acoustic Wave 50%
• Acoustic Instability 50%
• Termination Shock 50%
• High-Energy Cosmic Radiation 50%
• Galactic Wind 50%
• Perseus Cluster 50%

Keyphrases

• Wave Instability 100%
• X-ray 100%
• Cosmic Rays 100%
• Perseus 100%
• Sound Wave 100%
• Shock 20%
• Collisional Plasma 20%
• Intracluster Medium 20%
• Thermal Plasma 20%
• Galaxy Halos 20%
• Anisotropic Viscosity 20%
• Virion 10%
• Gas Pressure 10%
• Fast-growing 10%
• Linear Stability Analysis 10%
• Magnetized Plasma 10%
• Dimensionless Parameters 10%
• Long Wavelength 10%
• Galaxy Clusters 10%
• Density Fluctuations 10%
• Phase Shift 10%
• Gas Density 10%
• Galaxy Groups 10%
• Magnetic Pressure 10%
• Acoustic Waves 10%
• Acoustic Instability 10%
• Pressure Anisotropy 10%
• Thermal Gas 10%
• Termination Shock 10%
• Additional Heating 10%
• Increased Pressure 10%
• Ultra-high Energy Cosmic Rays 10%
• Galactic Winds 10%
• Wave Growth 10%
• Anisotropic Conduction 10%
• Cluster Plasma 10%