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.
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The routine model with bulk viscosity best reproduces the Crab pulsar's magnetic inclination angle, spin period, and derivative, while electromagnetic torque and accretion suppress inclination growth and most other effects are negligible.
citing papers explorer
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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.
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Evolution of Crab Pulsar: Magnetic Inclination Angle and Spin
The routine model with bulk viscosity best reproduces the Crab pulsar's magnetic inclination angle, spin period, and derivative, while electromagnetic torque and accretion suppress inclination growth and most other effects are negligible.