Solution of a problem of cosmological constant and superconductive cosmology
Keywords:
cosmological constant, energy of vacuum, cosmologyAbstract
The description of formation of primary vacuum on Planck scales, with the use of the microscopic theory of superconductivity, allows to solve a problem of a cosmological constant and to obtain the value of the vacuum density, coinciding with the observed one. It is offered the new model of exponential expansion and the hot stage of the Universe, in which the synchronization of physical processes and the maintenance of uniformity occurs during each moment of time, instead of single-pass, as in inflationary cosmology.
References
Weinberg S. Mod.Phys. 61.1. (1989).
Burdyuzha V. arXiv:1030.1025.
Alexander S., Biswas T. arXiv:hep-th/0807.4468.
Alexander S. Phys.Lett. B629, 53 (2005) [arXiv:hep-th/0503146].
Fomin P. I. Zero cosmological constant and Planck scales phenomenology // Proc. of the Fourth Seminar on Quantum Gravity, May 25–29, Moskow / Ed. by M.A.Markov. — Singapore: World Scientific, 1988. — P. 813
Fomin P. I. On the crystal-like structure of physical vacuum on Planck distances // Probl. phys. kinetics and physics of solid body. — Kiev: Naukova dumka, 1990. — P. 387–398.
Bukalov A. V. Proc.Gamov conference 2010.
Bardeen J., Cooper L., Schrieffer J. R. Phys.Rev., 108, 1175 (1957).
Kirzhnits P. A. Sov.Phys.Usp. 21, 470-486 (1978).
Penrose R. The Road to Reality. — London: Jonathan CAP, 2004.
Feynman R. P. Statistical mechanics. A set of lectures. — Massachusetts: W. A. Benjamin, Inc., 1972
