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.
, year = 1990, month = feb, volume =
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.HE 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
Simulations demonstrate non-monotonic guide-field regulation of reconnection efficiency via balance between drift-kink suppression and tearing-mode hindrance in 3D relativistic current sheets.
2D radiative PIC simulations show multi-sheet reconnection in relativistic pair plasma evolving into Kolmogorov-like turbulence that provides secondary particle acceleration while keeping the high-energy spectrum steep.
citing papers explorer
-
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.
-
Guide-Field-mediated Multiscale Instabilities in Relativistic Reconnection
Simulations demonstrate non-monotonic guide-field regulation of reconnection efficiency via balance between drift-kink suppression and tearing-mode hindrance in 3D relativistic current sheets.
-
Radiative PIC simulations of relativistic pair plasma: multiple interacting current sheets and turbulent evolution
2D radiative PIC simulations show multi-sheet reconnection in relativistic pair plasma evolving into Kolmogorov-like turbulence that provides secondary particle acceleration while keeping the high-energy spectrum steep.