Particle motion in the gravitational field of a charged, radiating body.

Mathematics – Mathematical Physics

Scientific paper

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Gravitation Theory: Accretion Disks

Scientific paper

The motion of test bodies is examined in the framework of the Vaidya-Bonner model of a charged, radiating mass. The null and time-like geodesic equations are obtained exactly. Similar equations are obtained exactly for the case of charged test particles. It is demonstrated that the luminosity of the central body induces a relative motion between positive and negative test charges, leading to accretion disk temperatures for luminous bodies which are higher than those of non-radiating bodies.

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