Abstract
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.
- Received 1 September 2002
DOI:https://doi.org/10.1103/PhysRevD.66.123504
©2002 American Physical Society