Model-independent constraints expose kinetic-luminosity and induced-Compton optical-depth bottlenecks that rule out or severely limit external-shock and light-cylinder reconnection FRB models while favoring magnetospheric scenarios with in-situ acceleration.
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3D force-free simulations demonstrate that FRBs excite Alfvén waves leading to nonlinear attenuation within 10-100 magnetar radii in quiescent fields and at larger radii in relativistic outflows.
Equatorial twist geometry in the magnetar magnetosphere allows resonant Compton upscattering to reproduce the hard X-ray spectrum of 4U 0142+61 with optical depth limits from resonant cooling.
citing papers explorer
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The kinetic-energy bottleneck in Fast Radio Burst models
Model-independent constraints expose kinetic-luminosity and induced-Compton optical-depth bottlenecks that rule out or severely limit external-shock and light-cylinder reconnection FRB models while favoring magnetospheric scenarios with in-situ acceleration.
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Damping of Fast Radio Bursts in the Inner Magnetospheres of Magnetars
3D force-free simulations demonstrate that FRBs excite Alfvén waves leading to nonlinear attenuation within 10-100 magnetar radii in quiescent fields and at larger radii in relativistic outflows.
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Resonant Inverse Compton Scattering and Hard X-ray Emission in Magnetar Magnetospheres
Equatorial twist geometry in the magnetar magnetosphere allows resonant Compton upscattering to reproduce the hard X-ray spectrum of 4U 0142+61 with optical depth limits from resonant cooling.