Fits of a magnetized plasma radiative-transfer model to bright magnetar bursts favor heavy nuclei (effective charge Z≈37) over light ions, suggesting neutron-star crust material enters the emitting fireball.
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2026 3representative citing papers
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.
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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Spectral Evidence of Heavy Nuclei from the Neutron Star Crust in Magnetar Bursts
Fits of a magnetized plasma radiative-transfer model to bright magnetar bursts favor heavy nuclei (effective charge Z≈37) over light ions, suggesting neutron-star crust material enters the emitting fireball.
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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.
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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.