A gyro-phase-resolved pulsar emission code calibrated against a gyro-centric model reproduces its curvature radiation maps and spectra for a Vela-like pulsar and converges to the Aristotelian Electrodynamics limit.
@doi [ ] 10.1093/mnras/stv468, https://ui.adsabs.harvard.edu/abs/2015MNRAS.449.2759B 449
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Towards Modelling AR Sco: Calibration -- Reproducing High-Energy Pulsar Emission and Testing Convergence to Aristotelian Electrodynamics
A gyro-phase-resolved pulsar emission code calibrated against a gyro-centric model reproduces its curvature radiation maps and spectra for a Vela-like pulsar and converges to the Aristotelian Electrodynamics limit.