Journal Article

Thawing versus tracker behaviour: observational evidence

Shruti Thakur, Akhilesh Nautiyal, Anjan A. Sen and T. R. Seshadri

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 427, issue 2, pages 988-993
Published in print December 2012 | ISSN: 0035-8711
Published online December 2012 | e-ISSN: 1365-2966 | DOI:
Thawing versus tracker behaviour: observational evidence

Show Summary Details


Currently there exist a variety of scalar field models that attempt to explain the late-time acceleration of the Universe. This includes the standard canonical and non-canonical scalar field models together with the recently proposed Galileon scalar field models. One can divide all these scalar field models into two broad categories, namely thawing and tracker classes. In this work we investigate the evidence for these models from presently available observational data using the Bayesian approach. We use the generalized Chaplygin gas (GCG) parametrization for the dark energy equation of state (EoS), as it exhibits both thawer- and tracker-like behaviour for different values of the parameters. Subsequently we use Type Ia supernova (SnIa) measurements, recent measurements of the Hubble parameter at different redshifts (H(z)), measurements of the look-back time at different redshifts (Lookback), measurements of the linear growth factor in large-scale structure (GR) from various redshift surveys and finally measurement of the anisotropies in the cosmic microwave background radiation by WMAP−7 observations. The analysis of data from SN+H(z)+Lookback does not favour either tracker or thawer classes. Inclusion of data from GR+WMAP−7 favours the thawer class of models if one assumes the dark energy to be a smooth component. If we consider dark energy perturbations, however, both tracker and thawer types of models are equally favoured by the data.

Keywords: methods: data analysis; methods: statistical; cosmological parameters; cosmology: observations; dark energy; distance scale

Journal Article.  3817 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.