Constraints on millisecond magnetars as the engines of prompt emission in gamma-ray bursts

Keyphrases

• Baryons 11%
• Burst Energy 11%
• Burst Size 11%
• Central Engine 22%
• Dissipation Model 11%
• Emission Model 11%
• Energetic Spectrum 11%
• Energy Dissipation 11%
• Energy Distribution 11%
• Entrainment 11%
• Gamma Rays 11%
• Gamma-ray Bursts 100%
• Light Curves 11%
• Magnetar Model 22%
• Magnetars 100%
• Magnetic Dissipation 11%
• Magnetic Reconnection 11%
• Magnetization 22%
• Mass Loss 11%
• Neutrinos 11%
• Optically Thick 11%
• Optically Thin 11%
• Particle Acceleration 11%
• Peak Energy 11%
• Power Injection 11%
• Prompt Emission 100%
• Rotational Energy 11%
• Shock 11%
• Spectral Curve 11%
• Spectral Slope 11%
• Temporal Evolution 11%
• Thin Regions 11%
• Time Challenges 11%
• Ultra-long 11%
• Wind Model 11%

Physics

• Baryon 11%
• Black Holes 11%
• Energetics 22%
• Energy Distribution 11%
• Gamma Radiation 11%
• Gamma Ray Burst 100%
• Light Curve 11%
• Magnetars 100%
• Particle Acceleration 11%
• Wall Jet 11%