First predicted cosmic ray spectra, primary-to-secondary ratios, and ionization rates from MHD galaxy formation simulations

Keyphrases

• Galaxies 100%
• Cosmic Rays 100%
• Cosmic Ray Spectrum 100%
• Ionization Rate 100%
• Galaxy Formation 100%
• Scattering Coefficient 100%
• Local Interstellar Medium 100%
• Milky Way 50%
• Molecular Clouds 50%
• Galactic 50%
• Shock 50%
• Convection Term 50%
• Magnetohydrodynamics 50%
• Star Formation 50%
• Power Law 50%
• Solar Neighborhood 50%
• Local Structure 50%
• Single Power 50%
• Systematic Variation 50%
• Antiproton 50%
• Cosmic Acceleration 50%
• Spectral Slope 50%
• Source Distribution 50%
• Electron-positron 50%
• Cosmic Ray Ionization 50%
• Heavy nuclei 50%
• New numerical Scheme 50%
• Coefficient Scaling 50%
• Scattering Halos 50%
• 2-increasing 50%
• TeV Energies 50%
• Reacceleration 50%
• Historical Model 50%
• Distribution Effect 50%
• Loss Effect 50%
• Circumgalactic Medium 50%
• Proton-nucleus 50%
• Turbulent Fountain 50%
• 10Be 50%
• Secondary Spectrum 50%
• Transport Physics 50%
• Galaxy Simulation 50%
• Media Cloud 50%
• Resolved Spectra 50%
• Cosmic Ray Secondaries 50%
• Injection Coefficient 50%

Physics

• Magnetohydrodynamic Generator 100%
• Interstellar Matter 100%
• Galactic Evolution 100%
• Scattering Coefficient 100%
• Molecular Clouds 50%
• Milky Way 50%
• Magnetohydrodynamics 50%
• Physics 50%
• Star Formation 50%
• Positron 50%
• Solar Neighborhood 50%
• Mathematical Method 50%
• Heavy Nuclei 50%
• Secondary Cosmic Rays 50%
• Transportation 50%