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

  1. D. Waldram
  2. J. Hartong
  3. David S. Berman
  4. F. Piazza
  5. D. Thompson
  6. J. Khoury
  7. G. Horowitz
  8. G. W. Gibbons

In Geometry and Topology

  1. David S. Berman
  2. D. Waldram
  3. D. Thompson
  4. C. Strickland-Constable
  5. M. Perry
  6. H. Godazgar
  7. Axel Kleinschmidt
  8. K. Narayan

In Nuclear and High Energy Physics

  1. David S. Berman
  2. D. Thompson
  3. D. Waldram
  4. C. Strickland-Constable
  5. D. Marqués
  6. K. Narayan
  7. J. Gauntlett
  8. S. Hartnoll

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