Electromagnetic Emission Post Spinning Black Hole Magnetized Neutron Star Mergers

  title={Electromagnetic Emission Post Spinning Black Hole Magnetized Neutron Star Mergers},
  author={Shu-Qing Zhong and Z. G. Dai and Can-Min Deng},
  journal={The Astrophysical Journal},
For a binary composed of a spinning black hole (BH) (with mass $\gtrsim 7M_\odot$) and a strongly magnetized neutron star (NS) (with surface magnetic field strength $B_{\rm S,NS}\gtrsim10^{12}$\,G and mass $\sim 1.4M_\odot$), the NS as a whole will possibly eventually plunge into the BH. During the inspiral phase, the spinning BH could be charged to the Wald charge quantity $Q_{\rm W}$ until merger in an electro-vacuum approximation. During the merger, if the spinning charged BH creates its own… 

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