GRB spectrum from gradual dissipation in a magnetized outflow

Keyphrases

• Power Law 100%
• Heating Scenarios 100%
• Thermal Component 100%
• Distributed Heating 100%
• Energy Dissipation 50%
• Energy-dependent 50%
• Ultra-relativistic 50%
• Spectral Components 50%
• Gamma-ray Bursts 50%
• Synchrotron Emission 50%
• Prompt Emission 50%
• Lorentz Factor 50%
• Steady State 50%
• Emission Model 50%
• Linear Polarization 50%
• Magnetic Field Structure 50%
• Energy Dissipation Rate 50%
• Magnetic Reconnection 50%
• Magnetic Energy 50%
• Low Energy 50%
• Band Functions 50%
• Emission Spectrum 50%
• X-ray Emission 50%
• Energy Injection 50%
• Energy Density 50%
• Two-mode 50%
• Numerical Code 50%
• Field Reversal 50%
• Monoenergetic Electrons 50%
• Magnetohydrodynamic Instabilities 50%
• Dynamic Power Dissipation 50%
• All-electron 50%
• Electron-positron-ion Plasma 50%
• Comptonization 50%
• Two-particle 50%
• Particle Heating 50%
• Kinetic Equation 50%
• Double Hump 50%
• Injected Energy 50%
• Thermal Peak 50%
• Particle Energy 50%

Physics

• Flux Density 100%
• Gamma Ray Burst 100%
• Interstellar Synchrotron Emission 100%
• Steady State 100%
• Magnetic Field 100%
• Linear Polarization 100%
• Magnetohydrodynamics 100%
• Emission Spectra 100%
• Electron-Positron Plasmas 100%
• Kinetic Equation 100%
• Volume 100%