NSNS Interior and Exterior B-field
Detail
In this case, the neutron stars have dipolar B-field lines extending to the exterior in the NSNS binary, as in a pulsar.
In this case, the neutron stars have dipolar B-field lines extending to the exterior in the NSNS binary, as in a pulsar.
| Initial Configuration |
| Density and Magnetic Field Evolution |
| Lagrangian Matter Tracers: The Jet Emerges |
| Gravitational Waveforms |
