Cosmological Billiards
By T. Damour, M. Henneaux, H. Nicolai. 2002
293 citations recorded by the source corpus.
It is shown in detail that the dynamics of the Einstein-dilaton-pform system in the vicinity of a spacelike singularity can be asymptotically described, at a generic spatial point, as a billiard motion in a region of Lobachevskii space (realized as an hyperboloid in the space of logarithmic scale factors). This is done within the Hamiltonian formalism, and for an arbitrary number of spacetime dimensions D ≥ 4. A key rôle in the derivation is played by the Iwasawa decomposition of the spatial metric, and by the fact that the off-diagonal degrees of freedom, as well as the p-form degrees of freedom, get “asymptotically frozen” in this description. For those models admitting a Kac-Moody theoretic interpretation of the billiard dynamics we outline how to set up an asymptotically equivalent description in terms of a one-dimensional non-linear σ-model formally invariant under the corresponding Kac-Moody group.
Subfields: Astronomy and Astrophysics, Geometry and Topology, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/28f5ff1587e21d61153e5901c60e52e8c422d953
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In Astronomy and Astrophysics
In Geometry and Topology
- David S. Berman
- D. Waldram
- D. Thompson
- C. Strickland-Constable
- M. Perry
- H. Godazgar
- Axel Kleinschmidt
- K. Narayan
In Nuclear and High Energy Physics
- David S. Berman
- D. Thompson
- D. Waldram
- C. Strickland-Constable
- D. Marqués
- K. Narayan
- J. Gauntlett
- S. Hartnoll
Citations in the corpus
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