http://arxiv.org/abs/1801.05765
In this paper we summarise the constraints that low-redshift data -such as supernovae Ia, baryon acoustic oscillations and cosmic chronometers- are able to set on the concordance model and its extensions, as well as on inhomogeneous but isotropic models. We provide a broad overlook into these cosmological scenarios, discussing several data analysis aspects of these datasets. We specifically discuss the current status of the inferred dynamics of cosmic expansion and its present rate.
V. Lukovic, B. Haridasu and N. Vittorio
Thu, 18 Jan 2018
57/58
Comments: N/A