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Uniform sky glow (CMB) observed through the throat of a wormhole

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arxiv 2305.18041 v1 pith:W6BR7XAU submitted 2023-05-29 gr-qc

Mikhail A. Bugaev , Igor D. Novikov , Serge V. Repin , Polina S. Samorodskaya This is my paper · ORCID
classification gr-qc
keywords imagewormholeconstructeduniformbackgroundconsideredglowimages
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The problem of the possibility of observing a uniform sky glow through the throat of a Morris--Thorne wormhole by an observer located in another asymptotically flat space-time is considered. It is shown that an individual star has multiple images, and the image of a luminous sky has a complex structure and contains ring structures. The reasons for the emergence of such structures are considered. The distribution of radiation intensity in the image along the radial coordinate is constructed.In addition, an image of the Morris-Thorne wormhole was constructed against the background of uniform sky radiation in the observer's space. A comparison to observations can be made by producing a synthetic Morris-Thorne type wormhole image against a CMB background. This image has been constructed by a combination of the images for inner and outer areas.

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  1. Observing of background electromagnetic radiation of the real sky through the throat of a wormhole

    gr-qc 2024-12 conditional novelty 5.0 of 10

    A simulation shows that a nearby wormhole mouth would project a lensed image of the real CMB sky and Milky Way inside its silhouette, offering a possible observational signature distinct from a black hole.

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