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The Influence of Evolving Dark Energy on Cosmology

Published online by Cambridge University Press:  05 March 2013

Luke Barnes ,
Matthew J. Francis ,
Geraint F. Lewis  and
Eric V. Linder
Luke Barnes
Affiliation:
School of Physics, University of Sydney, Sydney NSW 2006, Australia
Matthew J. Francis
Affiliation:
School of Physics, University of Sydney, Sydney NSW 2006, Australia
Geraint F. Lewis*
Affiliation:
School of Physics, University of Sydney, Sydney NSW 2006, Australia
Eric V. Linder
Affiliation:
Physics Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA
*
BCorresponding author. Email: [email protected]
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Abstract

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Observational evidence indicating that the expansion of the universe is accelerating has surprised cosmologists in recent years. Cosmological models have sought to explain this acceleration by incorporating ‘dark energy’, of which the traditional cosmological constant is just one possible candidate. Several cosmological models involving an evolving equation of state of the dark energy have been proposed, as well as possible energy exchange to other components, such as dark matter. This paper summarizes the forms of the most prominent models and discusses their implications for cosmology and astrophysics. Finally, this paper examines the current and future observational constraints on the nature of dark energy.

Keywords

cosmology: theorycosmological parametersdark matter
Type
Review Article
Information
Publications of the Astronomical Society of Australia , Volume 22 , Issue 4 , 2005 , pp. 315 - 325
Copyright
Copyright © Astronomical Society of Australia 2005

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