Probing the Physics of Core-Collapse Supernovae and Ultra-Relativistic Outflows using Pulsar Wind Nebulae

Keyphrases

• Neutron Stars 100%
• Ultra-relativistic 100%
• Relativistic Outflows 100%
• Core-collapse Supernovae 100%
• Pulsar Wind Nebulae 100%
• Supernova Remnants 60%
• Nebulae 60%
• Pulsar Wind 60%
• Observatory 20%
• Kinetic Energy 20%
• Systematic Error 20%
• Dipole 20%
• Valuable Insight 20%
• Parameter Space 20%
• Dynamical Properties 20%
• Active Galactic nuclei 20%
• Gamma Rays 20%
• Supernovae 20%
• Massive Stars 20%
• Gamma-ray Bursts 20%
• Field Strength 20%
• X-ray 20%
• Ejecta 20%
• Monte Carlo Algorithm 20%
• Fermi-LAT 20%
• Star-forming Galaxies 20%
• High Velocity 20%
• Magnetosphere 20%
• Spin-down 20%
• Spectral Energy Distribution 20%
• Statistical Errors 20%
• Particle Acceleration 20%
• X-ray Photon 20%
• Consistent Measurement 20%
• Integrated Properties 20%
• Spectral Evolution 20%
• ATHENA 20%
• Decaying Dark Matter 20%
• Particle Spectrum 20%
• Cosmic-ray Positron 20%
• Cosmic-ray Electrons 20%
• Field Characteristics 20%
• Distribution Properties 20%
• NuSTAR 20%
• Cherenkov Telescope Array 20%
• Acceleration Mechanism 20%
• Star Power 20%

Physics

• Physics 100%
• Neutron Stars 100%
• Pulsar 100%
• Core-Collapse Supernovae 100%
• Nebula 100%
• Supernova Remnant 60%
• Field Strength 20%
• Kinetic Energy 20%
• Monte Carlo 20%
• Active Galactic Nuclei 20%
• Supernovae 20%
• Gamma Radiation 20%
• Massive Star 20%
• Gamma Ray Burst 20%
• Dark Matter 20%
• Ejecta 20%
• Magnetosphere 20%
• Spectral Energy Distribution 20%
• Positron 20%
• Particle Acceleration 20%