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Constraints on the mean density of the Universe which follow from the theories of adiabatic and whirl perturbations

Published online by Cambridge University Press:  07 February 2017

A. A. Kurskov  and
L. M. Ozernoy

Extract

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The aim of this communication is to investigate what constraints to the cosmological parameter Ω = 2qO can be obtained if one assumes that primaeval whirl motions or adiabatic density perturbations with an appropriate initial spectrum were responsible for the formation of large scale structure in the Universe. These constraints are readily obtained from the two conditions: (i) an upper limit to small scale temperature fluctuations of the microwave background radiation, and (ii) the requirement that the primaeval perturbations should be large enough in order to produce observed structures.

Type
IV. Observational Evidence for Cosmological Evolution
Information
Symposium - International Astronomical Union , Volume 79: The Large Scale Structure of the Universe , 1978 , pp. 404 - 405
Copyright
Copyright © Reidel 1978 

References

Anile, A.M., Danese, L., De Zotti, G. and Motta, S., 1976. Astrophys. J., 205, L59.CrossRefGoogle Scholar
Chibisov, G.V., 1972. Astron. Zh., 49, 74.Google Scholar
Chibisov, G.V. and Ozernoy, L.M., 1969. Astrophys. Lttters, 3, 189.Google Scholar
Kurskov, A.A. and Ozernoy, L.M., 1977a. Astrophys. Sp. Sci. (submitted).Google Scholar
Kurskov, A.A. and Ozernoy, L.M., 1977b. Astrophys. Sp. Sci. (submitted).Google Scholar
Zeldovich, Ya. B. and Sunyaev, R.A., 1972. Astrophys. Sp. Sci., 7, 3.Google Scholar