Abstract

A dynamical model of the decaying vacuum energy is presented, which is based on Jordan-Brans-Dicke theory with a scalar field ϕϕ. The solution of an evolutionary differential equation for the scalar field ϕϕ drives the vacuum energy towards a cosmological constant at the present epoch that can give for the age of the universe, t0∼13.5t_0\sim 13.5 Gyr for Ω0=1Ω_0=1, which is consistent with the age of globular clusters.

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