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Universe 2018, 4(2), 35; https://doi.org/10.3390/universe4020035

Effects of Scattering of Radiation on Wormholes

1
Department of Physics, Bauman Moscow State Technical University, Moscow 105005, Russia
2
Department of Mathematical Modeling, Bauman Moscow State Technical University, Moscow 105005, Russia
These authors contributed equally to this work.
*
Author to whom correspondence should be addressed.
Received: 28 December 2017 / Revised: 4 February 2018 / Accepted: 8 February 2018 / Published: 12 February 2018
(This article belongs to the Special Issue Wormholes in Space-Time: Theory and Facts)
Full-Text   |   PDF [316 KB, uploaded 12 February 2018]

Abstract

Significant progress in the development of observational techniques gives us the hope to directly observe cosmological wormholes. We have collected basic effects produced by the scattering of radiation on wormholes, which can be used in observations. These are the additional topological damping of cosmic rays, the generation of a diffuse background around any discrete source, the generation of an interference picture, and distortion of the cosmic microwave background (CMB) spectrum. It turns out that wormholes in the leading order mimic perfectly analogous effects of the scattering of radiation on the standard matter (dust, hot electron gas, etc.). However, in higher orders, a small difference appears, which allows for disentangling effects of wormholes and ordinary matter. View Full-Text
Keywords: cosmology; diffuse background radiations; microwave; cosmological wormholes cosmology; diffuse background radiations; microwave; cosmological wormholes
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited (CC BY 4.0).
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Kirillov, A.; Savelova, E. Effects of Scattering of Radiation on Wormholes. Universe 2018, 4, 35.

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