@Article{Panotopoulos2011,
author="Panotopoulos, G.",
title="A dynamical dark energy model with a given luminosity distance",
journal="General Relativity and Gravitation",
year="2011",
publisher="Springer/Plenum Publishers",
volume="43",
number="11",
pages="3191--3199",
optkeywords="Dark energy; Observational cosmology; Particle-theory",
abstract="It is assumed that the current cosmic acceleration is driven by a scalar field, the Lagrangian of which is a function of the kinetic term only, and that the luminosity distance is a given function of the red-shift. Upon comparison with baryon acoustic oscillations and cosmic microwave background data the parameters of the models are determined, and then the time evolution of the scalar field is determined by the dynamics using the cosmological equations. We find that the solution is very different than the corresponding solution when the non-relativistic matter is ignored, and that the universe enters the acceleration era at larger red-shift compared to the standard I > CDM model.",
optnote="WOS:000295982800015",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=782), last updated on Fri, 11 Nov 2011 15:29:25 +0000",
issn="0001-7701",
doi="10.1007/s10714-011-1230-6",
opturl="http://arxiv.org/abs/1107.4475",
opturl="https://doi.org/10.1007/s10714-011-1230-6",
archivePrefix="arXiv",
eprint="1107.4475",
language="English"
}