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Magnetospheric Scattering and Emission in Millisecond Pulsars

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arxiv astro-ph/0004407 v1 pith:7IGNLMZ2 submitted 2000-04-28 astro-ph

Timothy M. Braje , Roger W. Romani This is my paper · ORCID
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We model the formation of magnetospheric components of millisecond pulsar light curves, deriving an approximate model for the curved space, `swept-back' dipole field and following photon emission, propagation, and scattering. Magnetospheric pulse components are strongly affected by rapid rotation and Schwarzschild effects.

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Cited by 1 Pith paper

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  1. Radiative Back-Reaction on Charged Particle Motion in the Dipole Magnetosphere of Neutron Stars

    astro-ph.HE 2024-12 conditional novelty 6.0 of 10

    Radiative back-reaction makes charged particles under an attractive Lorentz force fall onto a magnetized neutron star, while under a repulsive force they either widen their orbits or fall, depending on the starting latitude.

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