Solving for the dynamics of the universe

نویسنده

  • Valerio Faraoni
چکیده

A new method of solving the Einstein–Friedmann dynamical equations of a spatially homogeneous and isotropic universe is presented. The method is applicable when the equation of state of the material content assumes the form P = (γ − 1) ρ, γ = constant. The solution for the expansion factor is commonly given only for γ = 0, 1 and 4/3 when the curvature index is K = ±1. The proposed procedure is valid for general γ and K and it allows for ease of derivation of the solutions. This alternative method is useful pedagogically to introduce basic cosmology. To appear in Am. J. Phys.

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تاریخ انتشار 1999