OBSERVING OF BACKGROUND ELECTROMAGNETIC RADIATION OF THE REAL SKY THROUGH THE THROAT OF A WORMHOLE

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Resumo

The numerical investigation conducted in this paper addresses the problem of CMB radiation imaging as seen through the throat of the Ellis-Bronnikov-Morris-Thorne wormhole. It is assumed that both throats of the wormhole are relatively close to our stellar neighborhood, so close that the view of the ambient background radiation by an observer at the other throat of the wormhole is virtually identical to that seen from the Solar System neighborhood. A map of the temperature distribution of the cosmic microwave background radiation observed through the mouth of the wormhole has been constructed as well as a view of the Milky Way through the mouth of the wormhole. The resultant image contains characteristic details that enable it to be distinguished from an image produced by a black hole.

Sobre autores

M. Bugaev

Moscow Institute of Physics and Technology

Dolgoprudnyi, Moscow region, Russia

I. Novikov

Astrospace Center of P. N. Lebedev Physical Institute of the Russian Academy of Sciences; The Niels Bohr International Academy, The Niels Bohr Institute, Copenhagen, DenmarkThe Niels Bohr International Academy, The Niels Bohr Institute; National Research Center Kurchatov Institute, Moscow, Russia 𝑑National Research Center Kurchatov Institute

Moscow, Russia; Copenhagen, Denmark; Moscow, Russia

S. Repin

Astrospace Center of P. N. Lebedev Physical Institute of the Russian Academy of Sciences

Email: sergerepin1@gmail.com
Moscow, Russia

P. Samorodskaya

Moscow Institute of Physics and Technology

Dolgoprudnyi, Moscow region, Russia

I. Novikov, jr.

Lomonosov Moscow State University, Sternberg Astronomical Institute

Moscow, Russia

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