Dark Sector from Interacting Canonical and Non-Canonical Scalar Fields

Details Dark Sector from Interacting Canonical and Non-Canonical Scalar Fields Dark Sector from Interacting Canonical and Non-Canonical Scalar Fields

2010-06-16

arxiv.org/abs/1006.3146v1

Class.Quant.Grav.27:175006,2010

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

20 pages, 13 figures, accepted for publication in Classical and Quantum Gravity

Scientific paper

10.1088/0264-9381/27/17/175006

In this work it is investigated general models with interactions between two canonical scalar fields and between one non-canonical (tachyon-type) and one canonical scalar field. The potentials and couplings to the gravity are selected through the Noether symmetry approach. These general models are employed to describe interactions between dark energy and dark matter, with the fields being constrained by the astronomical data. The cosmological solutions of some cases are compared with the observed evolution of the late Universe.

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