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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6 Pith papers cite this work, alongside 44 external citations. Polarity classification is still indexing.
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UNVERDICTED 6representative citing papers
3D PIC simulations find that diocotron modes produce charge diffusion and electric field perturbations that can modulate pulsar emission properties.
Chandra observations of CTA 1 PWN show jet/torus morphology, constrain pulsar velocity to ≲200 km/s, and model low magnetic field with PeV electron cutoff in a young low-efficiency nebula.
Synchrotron cooling produces an energy-dependent loss cone and a cooled-loss-cone plasma distribution in neutron star outer magnetospheres, with losses localized at a few hundred to a thousand stellar radii.
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.
Entity PIC code updated with up to 11th-order current deposit and generalized field stencils, with tests showing improved conservation properties and suppression of numerical effects.
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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Diocotron Modes in Pulsar Magnetospheres: Charge Diffusion and Implications for Radio Emission Variability
3D PIC simulations find that diocotron modes produce charge diffusion and electric field perturbations that can modulate pulsar emission properties.
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Chandra X-ray Observations of the Pulsar Wind Nebula within CTA 1
Chandra observations of CTA 1 PWN show jet/torus morphology, constrain pulsar velocity to ≲200 km/s, and model low magnetic field with PeV electron cutoff in a young low-efficiency nebula.
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Synchrotron-cooled plasma distribution in the outer magnetosphere of a neutron star
Synchrotron cooling produces an energy-dependent loss cone and a cooled-loss-cone plasma distribution in neutron star outer magnetospheres, with losses localized at a few hundred to a thousand stellar radii.
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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.
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Entity -- Hardware-agnostic Particle-in-Cell Code for Plasma Astrophysics. III: Higher-order shape functions & generalized field stencils
Entity PIC code updated with up to 11th-order current deposit and generalized field stencils, with tests showing improved conservation properties and suppression of numerical effects.