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Observational Physics of Mirror World

Published online by Cambridge University Press:  25 May 2016

N.G. Bochkarev  and
M. Yu. Khlopov
N.G. Bochkarev
Affiliation:
Sternberg Astronomical Institute, Moscow, 119899, Russia
M. Yu. Khlopov
Affiliation:
Scientific-Educational Center “Cosmion”, Moscow, Russia

Extract

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Mirror (shadow) particles are required to restore symmetry between left- and right-handed coordinate systems. If mirror world exists, it has been born at the same time as the ordinary world and has the same evolution (in the case of the shadow world - broken mirror symmetry, the evolution and structure of the shadow world does not correspond with the observed world). Mirror world is a kind of dark matter. According to Bahcall (1984) local dark matter has a density approximately equal to the density of observed (ordinary) matter.

Type
V. Cosmological Models
Information
Symposium - International Astronomical Union , Volume 183: Cosmological Parameters and the Evolution of the Universe , 1999 , pp. 309
Copyright
Copyright © Kluwer 1999 

References

Bahcall, J., 1984 ApJ, 286, 169; 273, 200 Google Scholar
Blinnikov, S.N. and Khlopov, M. Yu. Zh., 60, 632, 1982.Google Scholar
Khlopov, M. Yu., Beskin, G.M., Bochkarev, N.G., Pustilnik, L.A., Pustilnik, S.A. 1991 Astron. Zh., 68, 42–57 (Sov. Astron. 35, 21-29) Google Scholar