On 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.

References in corpus (3)

• A direct empirical proof of the existence of dark matter
• Testing Einstein's special relativity with Fermi's short hard gamma-ray burst GRB090510
• Dark Matter from a gas of wormholes

Cited by in corpus (6)

• On distortion of the background radiation spectrum by wormholes: kinematic Sunyaev-Zel'dovich effect
• Density perturbations in the gas of wormholes
• Galaxy clusters as probes for cosmology and dark matter
• On Scattering of Electromagnetic Waves by a Wormhole
• On possible origin of an anisotropy in the speed of light in vacuum
• The universe formation by a space reduction cascade with random initial parameters