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

Abstract

The model of space in the form of a static gas of wormholes is considered. It is shown that the scattering on such a gas gives rise to the formation of a specific diffuse halo around every discrete source. Properties of the halo are determined by the distribution of wormholes in space and the halo has to be correlated with the distribution of dark matter. This allows to explain the absence of dark matter in intergalactic gas clouds. Numerical estimates for parameters of the gas of wormholes are also obtained.

Cosmological wormholes

“…We stress that such boundary conditions have the direct analogy to moving flat mirrors in the flat spacetime which were used in describing the general behavior of the metric near the cosmological singularity in classical and quantum gravity, e.g., see Refs. [10] and references therein.…”

Effects of Scattering of Radiation on Wormholes

“…We consider a ball of the radius r around a point-like source. For example, for an isotropic source, the number of particles emitted in the unit time in the solid angle dΩ = r 2 dφd cos θ remains constant, dN ∼ f 0 dΩ = const, which gives the standard distribution of Equation (15), that is, f 0 ∼ I/4πr 2 .…”

On scattering of CMB radiation on wormholes: Kinematic SZ-effect

“…The scattering of signals on spherical wormholes has been already studied e.g., [9,10] see also recent papers [11][12][13]. The basic two important features is the generation of a specific interference picture (upon scattering on a single wormhole) and the generation of a diffuse halo around any discrete source.…”