General-relativistic pulsar magnetospheric emission
J\'er\^ome P\'etri

TL;DR
This paper systematically compares various pulsar magnetospheric emission models using general-relativistic and Newtonian frameworks, analyzing how different emission sites and particle distributions influence observable light-curves and sky maps.
Contribution
It introduces a comprehensive 3D integration method for plasma emissivity in general-relativistic fields, evaluating the impact of electric charge and relativistic effects on pulsar emission models.
Findings
General-relativistic effects significantly alter sky maps and light-curves.
Electric charge on the star impacts emission profiles near the light-cylinder.
Emission site assumptions critically influence pulse profile shapes.
Abstract
Most current pulsar emission models assume photon production and emission within the magnetosphere. Low frequency radiation is preferentially produced in the vicinity of the polar caps whereas the high-energy tail is shifted to regions closer but still inside the light-cylinder. We conducted a systematic study of the merit of several popular radiation sites like the polar cap, the outer gap and the slot gap. We computed sky maps emanating from each emission site according to a prescribed distribution function for the emitting particles made of an electron/positron mixture. Calculations are performed using a three dimensional integration of the plasma emissivity in the vacuum electromagnetic field of a rotating centred general-relativistic dipole. We compare Newtonian electromagnetic fields to their general-relativistic counterpart. In the latter case, light bending is also taken into…
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