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The Forming of the Cosmological Constant

1999/12/29 by Vladimir Burdyuzha, V. V. Burdyuzha, O. Lalakulich +9
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics (astro-ph) #Earth Systems and Cosmic Evolution #FOS: Physical sciences #Quantum Mechanics and Applications #Relativity and Gravitational Theory #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9912542

LaTex 2.09, 11 pages

arxiv created 1999/12/29 · openalex publication_date 1999/12/29 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The problem of the physical nature and the cosmological constant genesis is discussed. This problem can't be solved in terms of the current quantum field theory which operates with Higgs and nonperturbative vacuum condensates and takes into account the changes of these condensates during relativistic phase transitions. The problem can't be completely solved also in terms of the conventional global quantum theory: Wheeler-DeWitt quantum geometrodynamics does not describe the evolution of the Universe in time (RPT in particular). We have investigated this problem in the context of energies density of different vacuum subsystems characteristic scales of which pervaid all energetic scale of the Universe. At first the phemenological solution of the cosmological constant problem and then the hypothesis about the possible structure of a new global quantum theory are proposed. The main feature of this theory is the irreversible evolution of geometry and vacuum condensates in time in the regime of their selforganization. The transformation of the cosmological constant in dynamical variable is inevitably.

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