OBSERVATIONAL PHYSICS OF MIRROR WORLD

被引:0
|
作者
KHLOPOV, MY [1 ]
BESKIN, GM [1 ]
BOCHKAREV, NG [1 ]
PUSTILNIK, LA [1 ]
PUSTILNIK, SA [1 ]
机构
[1] PK SHTERNBERG ASTRON INST,MOSCOW,USSR
来源
ASTRONOMICHESKII ZHURNAL | 1991年 / 68卷 / 01期
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Mirror or shadow particles are predicted in physics to restore the symmetry between left-handed and righ-handed coordinate systems. These particles have only gravitational (or possibly superweak) interactions with ordinary matter and their own mirror (shadow) interactions. Study of such particles is possible in astronomical observations only. Qualitative analysis of effects, induced by the gravitational influence of mirror objects on the objects of ordinary matter is given. Broad program of searches for astronomical effects of mirror matter at the wide range of scales (from stellar to galaxy supercluster ones) is proposed.
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页码:42 / 57
页数:16
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