Abstract
Multidimensional, anisotropic cosmological models with Ricci-flat subspaces are investigated within the framework of low-energy string theory. The main properties of these models, their behavior at early and late stages of evolution, in particular, are determined on the basis of a qualitative theory of dynamical systems. The conditions for dynamical compactification of extra dimensions are found. A concrete model with a Kalb — Ramond field as the source is considered as an illustration.
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Translated from Astrofizika, Vol. 39, No. 2, pp. 287–311, April–June, 1996.
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Saharian, A.A. String cosmology and dynamical compactification. Astrophysics 39, 153–168 (1996). https://doi.org/10.1007/BF02044800
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DOI: https://doi.org/10.1007/BF02044800