On topological bias of discrete sources in the gas of wormholes

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

2009-09-29

arxiv.org/abs/0909.5254v2

JETP Lett.90:599-603,2010

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

Scientific paper

10.1134/S0021364009210024

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.

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