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On the topological bias of discrete sources in the gas of wormholes

  • Gravity, Astrophysics
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Abstract

A model of space in the form of a static gas of wormholes has been considered. It has been shown that the scattering of light on such a gas gives rise to the formation of a specific halo around every discrete source. The properties of the halo are determined by the spatial distribution of wormholes and the halo should correlate with the distribution of dark matter; this makes it possible to explain the complete absence of dark mass in the intergalactic gas. The parameters of the gas of wormholes have also been estimated.

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Authors and Affiliations

  1. Dimitrovgrad Branch, Ulyanovsk State University, Dimitrovgrad, 433507, Russia

    A. A. Kirillov, E. P. Savelova & G. D. Shamshutdinova

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  1. A. A. Kirillov
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  2. E. P. Savelova
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  3. G. D. Shamshutdinova
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Additional information

Original Russian Text © A.A. Kirillov, E.P. Savelova, G.D. Shamshutdinova, 2009, published in Pis’ma v Zhurnal Éksperimental’noĭ i Teoreticheskoĭ Fiziki, 2009, Vol. 90, No. 9, pp. 663–667.

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Kirillov, A.A., Savelova, E.P. & Shamshutdinova, G.D. On the topological bias of discrete sources in the gas of wormholes. Jetp Lett. 90, 599–603 (2010). https://doi.org/10.1134/S0021364009210024

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  • DOI: https://doi.org/10.1134/S0021364009210024

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