3D kinetic simulations of pre-merger binary neutron star magnetospheres predict nonthermal gamma-ray signals at ~16 MeV and fast radio burst-like radio transients from reconnecting current sheets.
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A dynamical model of magnetar-driven jet and PWN emission predicts a sequence of thermal, X-ray plateau, and late synchrotron/inverse-Compton radiation that accounts for key features in merger GRBs.
3D kinetic simulations find that merging Lundquist flux tubes produce delayed reconnection onset in 3D, a normalized reconnection rate of 0.08-0.10, and nonthermal particle spectra with power-law index 1.6-2.0 and cutoff gamma_cut/sigma_in approximately 50.
citing papers explorer
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Electromagnetic Precursors to Binary Neutron Star Mergers: Kinetic Simulations of Magnetospheric Flaring
3D kinetic simulations of pre-merger binary neutron star magnetospheres predict nonthermal gamma-ray signals at ~16 MeV and fast radio burst-like radio transients from reconnecting current sheets.
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Multi-wavelength Emission for a Post-merger Magnetar: The Magnetar-Driven Poynting Jet and Its Associated Pulsar Wind Nebula
A dynamical model of magnetar-driven jet and PWN emission predicts a sequence of thermal, X-ray plateau, and late synchrotron/inverse-Compton radiation that accounts for key features in merger GRBs.
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3D Kinetic Simulations of Driven Reconnection in Merging Flux Tubes
3D kinetic simulations find that merging Lundquist flux tubes produce delayed reconnection onset in 3D, a normalized reconnection rate of 0.08-0.10, and nonthermal particle spectra with power-law index 1.6-2.0 and cutoff gamma_cut/sigma_in approximately 50.