TY  - JOUR
AU  - Panotopoulos, G.
PY  - 2011
DA  - 2011//
TI  - A dynamical dark energy model with a given luminosity distance
T2  - Gen. Relativ. Gravit.
JO  - General Relativity and Gravitation
SP  - 3191
EP  - 3199
VL  - 43
IS  - 11
PB  - Springer/Plenum Publishers
KW  - Dark energy
KW  - Observational cosmology
KW  - Particle-theory
AB  - 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.
SN  - 0001-7701
UR  - http://arxiv.org/abs/1107.4475
UR  - https://doi.org/10.1007/s10714-011-1230-6
DO  - 10.1007/s10714-011-1230-6
LA  - English
N1  - WOS:000295982800015
ID  - Panotopoulos2011
ER  -