Cosmic acceleration, scalar fields and observations

Abstract

Conditions for accelerated expansion of Friedmann-Robertson-Walker space-time are analyzed. Connection of this scenario with present-day observations are reviewed. It is explained how a scalar field could be responsible for cosmic acceleration observed in present times and predicted for the very early Universe. Ideas aimed at answering whether is that the actual case for our Universe are described.

Published in "The Early Universe and Observational Cosmology", Springer-Verlag, Eds.: N. Breton, J. L. Cota-Cervantes and M. Salgado

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