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Gravitational Lensing of Rays through the Levitating Atmospheres of Compact Objects

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arxiv 1701.05693 v1 pith:U37RSART submitted 2017-01-20 gr-qc astro-ph.HE

classification gr-qcastro-ph.HE
keywords rayscompactshellatmospheresgravitationallevitatinglow-frequencyobject
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Electromagnetic rays travel on curved paths under the influence of gravity. When a dispersive optical medium is included, these trajectories are frequency-dependent. In this work we consider the behaviour of rays when a spherically symmetric, luminous compact object described by the Schwarzschild metric is surrounded by an optically thin shell of plasma supported by radiation pressure. Such levitating atmospheres occupy a position of stable radial equilibrium, where radiative flux and gravitational effects are balanced. Using general relativity and an inhomogeneous plasma we find the existence of a stable circular orbit within the atmospheric shell for low-frequency rays. We explore families of bound orbits that exist between the shell and the compact object, and identify sets of novel periodic orbits. Finally, we examine conditions necessary for the trapping and escape of low-frequency radiation.

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  1. Gravitational shadow and emission spectrum of thin accretion disks in a plasma medium

    gr-qc 2025-05 conditional novelty 6.0 of 10

    A blackbody accretion disk viewed through transparent, rotating plasma produces frequency-dependent shadows and emission maps, with the frequency of the brightest total flux controlled mainly by viewing angle.

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