The characteristics of dark energy in the developing Universe are studied.
Similar content being viewed by others
References
Yu. N. Eroshenko, Usp. Fiz. Nauk, 176, 440 (2006).
A. I. Smirnov, Russ. Phys. J., No. 2, 225 (2006).
A. D. Chernin, Usp. Fiz. Nauk, 171, 1153 (2001).
Ya. B. Zel’dovich and I. D. Novikov, The Structure and Evolution of the Universe [in Russian], Nauka, Moscow, 1975.
A. I. Smirnov, Russ. Phys. J., No. 10, 1061 (2007).
A. I. Smirnov, Ibid., No. 3, 255 (2005).
V. A. Rubakov, Usp. Fiz. Nauk, 177, 407 (2007).
Author information
Authors and Affiliations
Corresponding author
Additional information
Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 5, pp. 10–13, May, 2010.
Rights and permissions
About this article
Cite this article
Smirnov, A.I. The dominating stage of cosmological vacuum. Russ Phys J 53, 446–450 (2010). https://doi.org/10.1007/s11182-010-9441-y
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s11182-010-9441-y