Case A: Magnetized Irrotational
Detail
In this case, the neutron stars have dipolar B-field lines extending to the exterior in the NSNS binary, as in a pulsar. The neutron stars each have initial spin $\chi_{\rm NS} = a/m = 0$
In this case, the neutron stars have dipolar B-field lines extending to the exterior in the NSNS binary, as in a pulsar. The neutron stars each have initial spin $\chi_{\rm NS} = a/m = 0$
12 Feb 2019, Kyle Nelli