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• W2017159292 abstract "We investigate the effect of pulsar polar cap (PC) heating produced by positrons returning from the upper pair formation front. Our calculations are based on a self-consistent treatment of the pair dynamics and the effect of electric field screening by the returning positrons. We calculate the resultant X-ray luminosities and discuss the dependence of the PC heating efficiencies on pulsar parameters, such as characteristic spin-down age, spin period, and surface magnetic field strength. In this study we concentrate on the regime where the pairs are produced in a magnetic field by curvature photons emitted by accelerating electrons. Our theoretical results are not in conflict with the available observational X-ray data and suggest that the effect of PC heating should significantly contribute to the thermal X-ray fluxes from middle-aged and old pulsars. The implications for current and future X-ray observations of pulsars are briefly outlined." @default.
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• W2017159292 date "2001-08-01" @default.
• W2017159292 modified "2023-10-17" @default.
• W2017159292 title "Pulsar Polar Cap Heating and Surface Thermal X‐Ray Emission. I. Curvature Radiation Pair Fronts" @default.
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• W2017159292 doi "https://doi.org/10.1086/321589" @default.
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