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arXiv · 1704.07093

Wormhole Shadows in Rotating Dust

Takayuki Ohgami·Nobuyuki Sakai
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Abstract

As an extension of our previous work, which investigated the shadows of the Ellis wormhole surrounded by nonrotating dust, in this paper we study wormhole shadows in rotating dust flow. First, we derive steady-state solutions of slowly rotating dust surrounding the wormhole by solving relativistic Euler equations. Solving null geodesic equations and radiation transfer equations, we investigate the images of the wormhole surrounded by dust for the above steady-state solutions. Because the Ellis wormhole spacetime possesses unstable circular orbits of photons, a bright ring appears in the image, just as in Schwarzschild spacetime. The bright ring looks distorted due to rotation. Aside from the bright ring, there appear weakly luminous complex patterns by the emission from the other side of the throat. These structure could be detected by high-resolution very-long-baseline-interferometry observations in the near future.

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Takayuki Ohgami, Nobuyuki Sakai. 2017-04-24. Wormhole Shadows in Rotating Dust. https://doi.org/10.1103/physrevd.94.064071

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