arXiv · hep-th/9904077
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 electro-magnetic 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, N = n+l. The geometrical criterion for the finiteness of the billiard volume and its compactness is used. This criterion reduces the problem to the problem of illumination of (N-2)-dimensional sphere by point-like sources. Some examples with billiards of finite volume and hence oscillating behaviour near the singularity are considered. Among them examples with square and triangle 2-dimensional billiards (e.g. that of the Bianchi-IX model) and a 4-dimensional billiard in ``truncated'' D = 11 supergravity model (without the Chern-Simons term) are considered. It is shown that the inclusion of the Chern-Simons term destroys the confining of a billiard.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
V. D. Ivashchuk, V. N. Melnikov. 1999-04-09. Billiard Representation for Multidimensional Cosmology with Intersecting p-branes near the Singularity. https://doi.org/10.1063/1.1286671
Cite the original work for its findings. Save a collection to share your selection of sources.