Trajectory of test particle around a slowly rotating relativistic star emitting isotropic radiation
Jae-Sok Oh, Hongsu Kim, and Hyung Mok Lee

TL;DR
This paper investigates the motion of test particles near a slowly rotating relativistic star emitting isotropic radiation, revealing the existence of a stable 'suspension orbit' influenced by radiation forces and star properties.
Contribution
It introduces a detailed analysis of test particle trajectories considering radiation effects, highlighting the phenomena of radiation drag and counter-drag in relativistic star environments.
Findings
Existence of a 'suspension orbit' at a radius determined by luminosity and star's angular momentum.
Radiation counter-drag can cause particles to hover with angular velocity exceeding frame-dragging effects.
Radial position of the suspension orbit is independent of initial particle conditions.
Abstract
We explored the motion of test particles near slowly rotating relativistic star having a uniform luminosity. In order to derive the test particle's equations of motion, we made use of the radiation stress-energy tensor first constructed by Miller and Lamb \cite{ML96}. From the particle's trajectory obtained through the numerical integration of the equations of motion, it is found that for sufficiently high luminosity, "suspension orbit" exists, where the test particle hovers around at uniform angular velocity in the same direction as the star's spin. Interestingly, it turned out that the radial position of the "suspension orbit" was determined by the luminosity and the angular momentum of the star alone and was independent of the initial positions and the specific angular momentum of the particle. Also found is that there exist not only the radiation drag but also "radiation…
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