Is evidence for a dynamical dark energy equation of state ?
arXiv:0906.5366 · doi:10.1103/PhysRevD.80.067302
Abstract
Current constraints on the dark energy equation of state parameter, , are expected to be improved by more than one order of magnitude in the next decade. If $|w-1| \gsim 0.01$ around the present time, but the dark energy dynamics is sufficiently slow, it is possible that future constraints will rule out a cosmological constant while being consistent with a time-independent equation of state parameter. In this paper, we show that although models with such behavior can be constructed, they do require significant fine-tuning. Therefore, if the observed acceleration of the Universe is induced by a dark energy component, then finding would, on its own, constitute very strong evidence for a dynamical dark energy equation of state.
5 pages, 2 figures
References in corpus (8)
- Dynamics of dark energy
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Dark Energy and the Accelerating Universe
- Adiabatic instability in coupled dark energy-dark matter models
- Dynamics of domain wall networks with junctions
- Frustrated Expectations: Defect Networks and Dark Energy
- Linear and non-Linear Instabilities in Unified Dark Energy Models
- Clustering Properties of Dynamical Dark Energy Models