Abstract:We present an analytical study of light curves of slowly rotating pulsars with emphasis on the chromatic effects derived from the presence of a plasma environment; analyzing the effects of the compactness and charge of the star, the metric model, and the electronic plasma density profile. After doing a numerical integration of the trajectories and luminosity curves of pulsars for different spherically symmetric metrics representing the exterior region of the pulsar, we generalize the approximate Beloborodov fo… Show more
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