6533b86ffe1ef96bd12cd386
RESEARCH PRODUCT
A dynamical dark energy model with a given luminosity distance
Grigoris Panotopoulossubject
PhysicsPhysics and Astronomy (miscellaneous)Cosmic microwave backgroundTime evolutionFOS: Physical sciencesAcceleration (differential geometry)General Relativity and Quantum Cosmology (gr-qc)Kinetic termAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum CosmologyQuantum electrodynamicsDark energyBaryon acoustic oscillationsLuminosity distanceScalar fielddescription
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 (BAOs) and Cosmic Microwave Background (CMB) 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 $\Lambda CDM$ model.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2011-07-22 |