Bianchi Type I Cosmology and the Euler-calogero-sutherland Model
نویسندگان
چکیده
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.
منابع مشابه
ar X iv : g r - qc / 0 20 80 37 v 2 2 3 Se p 20 02 Bianchi type I cosmology and Euler - Calogero - Sutherland model
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 3-body hyperbolic Euler-Calogero-Sutherland system.
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The Bianchi 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 3-body hyperbolic Euler-Calogero-Sutherland system.
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