A new cosmological tracker solution for Quintessence

Astronomy and Astrophysics – Astrophysics

Scientific paper

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13 pages REVTeX, 5 eps color figures

Scientific paper

10.1103/PhysRevD.62.081302

In this paper we propose a quintessence model with the potential $V(\Phi )=V_{o}[ \sinh {(\alpha \sqrt{\kappa_{o}}\Delta \Phi})] ^{\beta}$, which asymptotic behavior corresponds to an inverse power-law potential at early times and to an exponential one at late times. We demonstrate that this is a tracker solution and that it could have driven the Universe into its current inflationary stage. The exact solutions and the description for a complete evolution of the Universe are also given. We compare such model with the current cosmological observations.

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