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.
Force-free simulations confirm that fast magnetosonic waves undergo efficient parametric decay into secondary FMS and Alfvén waves, producing a broad spectrum and continued energy drain even after equipartition.
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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Nonlinear Decay of Fast Magnetosonic Waves through Weak Turbulence: Force-Free Electrodynamics Simulations
Force-free simulations confirm that fast magnetosonic waves undergo efficient parametric decay into secondary FMS and Alfvén waves, producing a broad spectrum and continued energy drain even after equipartition.