A new view ofk-essence
- 2 June 2003
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 67 (12) , 123503
- https://doi.org/10.1103/physrevd.67.123503
Abstract
k-essence models, relying on scalar fields with noncanonical kinetic terms, have been proposed as an alternative to quintessence in explaining the observed acceleration of the Universe. We consider the use of field redefinitions to cast k-essence in a more familiar form. While k-essence models cannot in general be rewritten in the form of quintessence models, we show that in certain dynamical regimes an equivalence can be made, which in particular can shed light on the tracking behavior of k-essence. In several cases, k-essence cannot be observationally distinguished from quintessence using the homogeneous evolution, though there may be small effects on the perturbation spectrum. We make a detailed analysis of two k-essence models from the literature and comment on the nature of the fine-tuning arising in the models.Keywords
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This publication has 26 references indexed in Scilit:
- Cosmology and the fate of dilatation symmetryPublished by Elsevier ,2002
- Evidence for a non-zero and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and cosmic microwave background anisotropiesMonthly Notices of the Royal Astronomical Society, 2002
- Classification of scalar field potentials with cosmological scaling solutionsPhysical Review D, 1998
- Supernova Limits on the Cosmic Equation of StateThe Astrophysical Journal, 1998
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological ConstantThe Astronomical Journal, 1998
- Cosmology with a primordial scaling fieldPhysical Review D, 1998
- Exponential potentials and cosmological scaling solutionsPhysical Review D, 1998
- Cosmological Imprint of an Energy Component with General Equation of StatePhysical Review Letters, 1998
- Exponential Potentials, Scaling Solutions and InflationAnnals of the New York Academy of Sciences, 1993
- Cosmological consequences of a rolling homogeneous scalar fieldPhysical Review D, 1988