2000
DOI: 10.1063/1.1286671
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Billiard representation for multidimensional cosmology with intersecting p-branes near the singularity

Abstract: Multidimensional model describing the cosmological evolution of n Einstein spaces in the theory with l scalar fields and forms is considered. When electromagnetic composite p-brane ansatz is adopted, and certain restrictions on the parameters of the model are imposed, the dynamics of the model near the singularity is reduced to a billiard on the (N − 1)-dimensional Lobachevsky space H N −1 , N = n + l. The geometrical criterion for the finiteness of the billiard volume and its compactness is used. This criteri… Show more

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Cited by 55 publications
(108 citation statements)
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“…Moreover, the authors of [18] give a sketch of a proof of this conjecture. Although the ansatz for the cosmological metric in [18] contained d-beins leading to additional gravitational walls in the billiards and the Kasner parameters also depended on spatial coordinates, the analysis of [18], in essence, deals with the Bianchi-I type model with a maximal number of composite electric branes that form the billiard walls according to the prescription of [5]. The gravitational walls are irrelevant for the proof in [18].…”
Section: I2 Ementioning
confidence: 99%
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“…Moreover, the authors of [18] give a sketch of a proof of this conjecture. Although the ansatz for the cosmological metric in [18] contained d-beins leading to additional gravitational walls in the billiards and the Kasner parameters also depended on spatial coordinates, the analysis of [18], in essence, deals with the Bianchi-I type model with a maximal number of composite electric branes that form the billiard walls according to the prescription of [5]. The gravitational walls are irrelevant for the proof in [18].…”
Section: I2 Ementioning
confidence: 99%
“…It should be stressed that the billiard approach of [5] was derived in a class of block-diagonal metrics defined on the product of Einstein spaces (1) with certain restrictions imposed on the signatures of the Einstein metrics, g i . These restrictions are similar to the conditions > 0 for u 2 > 0 in the multicomponent fluid case.…”
Section: I2 Ementioning
confidence: 99%
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