In the unscreened-field case, Schwinger pair creation supplies charges far exceeding the Goldreich-Julian rate and removes ~90% of rotational energy within 30 ms for B_p=10^14 G and P_0=1 ms, suppressing gravitational-wave losses and linking millisecond magnetars to the observed population.
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Anisotropic bipolar and equatorial ejecta distributions produce two-peak features in late-time radio light curves that align with main thermal emissions, with non-detections in AT 2017gfo consistent under typical parameters.
citing papers explorer
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Energy Loss of Newborn Magnetars by Schwinger Process
In the unscreened-field case, Schwinger pair creation supplies charges far exceeding the Goldreich-Julian rate and removes ~90% of rotational energy within 30 ms for B_p=10^14 G and P_0=1 ms, suppressing gravitational-wave losses and linking millisecond magnetars to the observed population.
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Anisotropic Ejecta from Binary Neutron Star Mergers: Self-Consistent Main Thermal and Late-Time Radio Emission of NS-Powered Kilonovae
Anisotropic bipolar and equatorial ejecta distributions produce two-peak features in late-time radio light curves that align with main thermal emissions, with non-detections in AT 2017gfo consistent under typical parameters.