The growth of massive black holes in galaxy merger simulations with feedback by radiation pressure

Keyphrases

• Radiation Pressure 100%
• Galaxy Mergers 100%
• Black Hole Accretion 100%
• Massive Black Holes 100%
• Merger Simulation 100%
• Hole Growth 75%
• Galaxies 50%
• Star Formation 50%
• Optical Depth 50%
• Host Galaxy 50%
• Accretion Rate 50%
• Black Hole Feedback 50%
• Galactic nuclei 50%
• Optically Thick 25%
• Low-mass 25%
• Quasars 25%
• Luminosity 25%
• Far-infrared 25%
• Interstellar Medium 25%
• Star Formation Rate 25%
• Black Hole Mass 25%
• Time Dependence 25%
• Parameter-free 25%
• Cold Gas 25%
• Accretion Model 25%
• Massive Galaxies 25%
• Stellar Masses 25%
• Ambient Gas 25%
• Galaxy Masses 25%
• Subgrid 25%
• Ultraluminous Infrared Galaxies 25%
• Star Clusters 25%
• Robust Prediction 25%
• Smoothed Particle Hydrodynamics 25%
• Limited Supply 25%

Physics

• Black Holes 100%
• Radiation Pressure 100%
• Galaxy Mergers 100%
• Star Formation 15%
• Galactic Nuclei 15%
• Physics 7%
• Quasar 7%
• Interstellar Matter 7%
• Star Formation Rate 7%
• Time Dependence 7%
• Active Galactic Nuclei 7%
• Stellar Mass 7%
• Galaxy Masses 7%
• Star Cluster 7%
• Cold Gas 7%
• Ultraluminous Infrared Galaxies 7%
• Galaxy Mass 7%
• Far Infrared Radiation 7%