Asymmetry in the reconstructed deceleration parameter
arXiv:1606.07333 · doi:10.1016/j.physletb.2016.12.008
Abstract
We study the orientation dependence of the reconstructed deceleration parameter as a function of redshift. We use the Union 2 and Loss datasets, by using the well known preferred axis discussed in the literature, finding the best fit reconstructed deceleration parameter. We found that a low redshift transition of the reconstructed is clearly absent in one direction and amazingly sharp in the opposite one. We discuss the possibility that such a behavior can be associated with large scale structures affecting the data.
9 pages, 12 figures
References in corpus (11)
- Dark Energy and the Accelerating Universe
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
- Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
- Modified gravity models of dark energy
- Quintessence: a mini-review
- Power asymmetry in WMAP and Planck temperature sky maps as measured by a local variance estimator
- Mimicking Dark Energy with Lemaitre-Tolman-Bondi Models: Weak Central Singularities and Critical Points
- Alignment of quasar polarizations with large-scale structures
- Probing bulk flow with nearby SNe Ia data
- Comparison between hemisphere comparison method and dipole-fitting method in tracing the anisotropic expansion of the Universe use the Union2 dataset