Isotropic flat space cosmology in Jordan-Brans-Dicke theory

Statistics – Computation

Scientific paper

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Computational Astrophysics, Cosmology, Isotropism, Polytropic Processes, Two Fluid Models

Scientific paper

The process of re-escalation of the scalar field φ as φR3 ≡ ψ, the energy density ρ as ρR3 ≡ ɛ, and the pressure p as pR3 ≡ P, lends itself to obtain a reduced equation that represents, for a wide variety of equations of state, the cosmological evolution of an homogeneous and isotropic, flat Universe. A particular solution to this equation is presented.

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