1995
DOI: 10.1063/1.531290
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Integrable pseudo-Euclidean Toda-like systems in multidimensional cosmology with multicomponent perfect fluid

Abstract: The multidimensional cosmological model describing the evolution of n Einstein spaces in the presence of multicomponent perfect fluid is considered. When the vectors corresponding to the equations of state of the components are orthogonal with respect to the minisuperspace metric, the Einstein equations are integrated and a Kasner-like form of the solutions is presented. For special sets of parameters the cosmological model is reduced to the Euclidean Toda-like system connected with some Lie algebra G. For G=A… Show more

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Cited by 48 publications
(72 citation statements)
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“…The latter can be achieved if the decay rate becomes larger. However, a fast decay in the regime of a broad parametric resonance [62] may not be realized for gravexcitons since it requires the condition Γ >> H at the beginning of the decay (H ∼ m ψ ) which is not satisfied (see estimate (34)). …”
Section: Heavy Gravexcitonsmentioning
confidence: 99%
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“…The latter can be achieved if the decay rate becomes larger. However, a fast decay in the regime of a broad parametric resonance [62] may not be realized for gravexcitons since it requires the condition Γ >> H at the beginning of the decay (H ∼ m ψ ) which is not satisfied (see estimate (34)). …”
Section: Heavy Gravexcitonsmentioning
confidence: 99%
“…gauge fields and scalar fields 6 . In some models these matter fields can be considered phenomenologically as a perfect fluid with energy density ρ and corresponding equation of state [20,21,34,35]. This provides, for example, an efficient way to take into account the Casimir effect [36], Freund-Rubin monopoles [24,37,38] or other hypothetical potentials [20,39].…”
Section: Gravitational Excitonsmentioning
confidence: 99%
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“…Other possible manifestations of extra dimensions are monopole modes in gravitational waves, various predictions for standard cosmological tests and generation of the cosmological constant [10], and numerous effects connected with local field sources, some of them being the subject of the present paper. These include, in particular, deviations from the Newton and Coulomb laws [11,4,5,12] and properties of black holes.…”
Section: Introductionmentioning
confidence: 99%