Gravitational wave signature of proto-neutron star convection: I. MHD numerical simulations
Gravitational wave signature of proto-neutron star convection: I. MHD numerical simulations
Gravitational waves provide a unique and powerful opportunity to constrain the dynamics in the interior of proto-neutron stars during core collapse supernovae. Convective motions play an important role in generating neutron stars magnetic fields, which could explain magnetar formation in the presence of fast rotation. We compute the gravitational wave …