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

被引：7
|
作者：
Kirillov, A. A. [1 ]
Savelova, E. P. [1 ]
Shamshutdinova, G. D. [1 ]
机构：
[1] IN Ulyanov State Univ, Dimitrovgrad Branch, Dimitrovgrad 433507, Russia
来源：
JETP LETTERS | 2010年 / 90卷 / 09期
基金：
俄罗斯基础研究基金会;
关键词：
DARK-MATTER; INFLATIONARY UNIVERSE; FLATNESS; HORIZON;
D O I：
10.1134/S0021364009210024
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
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.
引用
收藏
页码：599 / 603
页数：5
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