Deep Core Convection and Dynamo in Newly-born Neutron Star

23 Jan 2020 Masada Youhei Takiwaki Tomoya Kotake Kei

We report results from a convection dynamo simulation of proto-neutron star (PNS), with a nuclear equation of state (EOS) and the initial hydrodynamic profile taken from a neutrino radiation-hydrodynamics simulation of a massive stellar core-collapse. A moderately-rotating PNS with the spin period of $170$ ms in the lepton-driven convection stage is focused... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • FLUID DYNAMICS