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Search for Small Scale Anisotropy of the 3K Emission of the Universe

Published online by Cambridge University Press:  04 August 2017

A. B. Berlin
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz Stavropolskij Kraj, 357140, USSR
E. V. Bulaenko
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz Stavropolskij Kraj, 357140, USSR
V. V. Vitkovsky
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz Stavropolskij Kraj, 357140, USSR
V. K. Kononov
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz Stavropolskij Kraj, 357140, USSR
Yu. N. Parijskij
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz Stavropolskij Kraj, 357140, USSR
Z. E. Petrov
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz Stavropolskij Kraj, 357140, USSR

Extract

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One of the greatest mysteries of nature is the absence of any trace of the present structure of the nearby universe in its relict 3K emission.

If we live in an evolving world (which evolves from extremely smooth to extremely structural), our radio telescopes should see observable temperature variations of 3K in practically any world model.

Type
Research Article
Copyright
Copyright © Reidel 1983 

References

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Partridge, R.B.: 1979, in “The Large Scale Structure of the Universe,” proceedings of a summer school at Jodlowy Dwor, Poland, Demianski, M., ed., Springer Verlag.Google Scholar
Parijskij, Yu. N.: 1973, Ap. J. Letters, 180, L47.Google Scholar
Parijskij, Yu. N., Petrov, Z.E., Cherkov, L.: 1977, Pisma v Ast. Zh., 3, 483.Google Scholar