The proto-neutron star phase of the collapsar model and the route to long-soft gamma-ray bursts and hypernovae

Keyphrases

• Gamma-ray Bursts 100%
• Hypernova 100%
• Proto-neutron Star 100%
• Soft gamma Rays 100%
• Collapsar 100%
• Iron Core 60%
• Angular Momentum 40%
• Massive Stars 40%
• Low Metallicity 40%
• Magnetorotational Instability 40%
• High Angular Momentum 40%
• Angular Momentum Distribution 40%
• Magnetically Driven 40%
• Two Dimensional 20%
• Distinctive Features 20%
• MHD Simulation 20%
• Magnetic Field 20%
• Non-relativistic 20%
• Bi-flux Diffusion 20%
• Black Hole Formation 20%
• Surface Layer 20%
• Baryons 20%
• Type Ia Supernovae 20%
• Neutron Stars 20%
• Core-collapse 20%
• Magnetic Field Amplification 20%
• Multigroup 20%
• Angular Momentum Transfer 20%
• X-ray Bursts 20%
• Stellar Mass Loss 20%
• Rotational Surface 20%
• Chemically Homogeneous Evolution 20%
• Main Sequence Stars 20%
• Fast Rotation 20%
• Evolutionary Calculation 20%

Physics

• Angular Momentum 100%
• Neutron Stars 100%
• Hypernovae 100%
• Gamma-Ray Burst 100%
• Metallicity 28%
• Magnetic Field 28%
• Black Hole 28%
• Massive Star 28%
• Magnetohydrodynamic Generator 14%
• Baryon 14%
• Main Sequence Stars 14%
• Surface Layers 14%
• Type Ic Supernovae 14%
• Stellar Mass Loss 14%
• Transportation 14%