On the Equation of State for Scalar Field

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

We consider Friedmann cosmologies with minimally coupled scalar field. Exact solutions are found, many of them elementary, for which the scalar field energy density, rho_f, and pressure, p_f, obey the equation of state (EOS) p_f=w_f\rho_f. For any constant |w_f|<1 there exists a two-parameter family of potentials allowing for such solutions; the range includes, in particular, the quintessence (-1

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