Neutrino transport in strongly magnetized proto-neutron stars and the origin of pulsar kicks: The effect of asymmetric magnetic field topology

Physics & Astronomy

• pulsars 99%
• neutron stars 96%
• topology 86%
• neutrinos 82%
• opacity 54%
• magnetic fields 49%
• poles 43%
• field strength 29%
• cross sections 19%
• absorption cross sections 16%
• energy 14%
• energy levels 13%
• stars 11%
• neutrons 11%
• modulation 10%
• protons 10%

Earth & Environmental Sciences

• topology 100%
• magnetic field 87%
• cross section 40%
• energy 24%
• effect 23%
• energy flux 18%