Bianchi type I cosmology and the Euler-Calogero-Sutherland model

Details Bianchi type I cosmology and the Euler-Calogero-Sutherland model Bianchi type I cosmology and the Euler-Calogero-Sutherland model

2002-08-14

arxiv.org/abs/gr-qc/0208037v3

Phys.Rev. D66 (2002) 123504

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, LaTeX, no figures. V2: Title and abstract slightly changed, typos corrected. V3: Minor changes, version to appear in

Scientific paper

10.1103/PhysRevD.66.123504

The Bianchi type I cosmological model is brought into a form where the
evolution of observables is governed by the unconstrained Hamiltonian that
coincides with the Hamiltonian describing the relative motion of particles in
the integrable three-body hyperbolic Euler-Calogero-Sutherland system.

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