arXiv · 1301.4044
Constraints from Cosmography in various parameterizations
Abstract
We use cosmography to present constraints on the kinematics of the Universe without postulating any underlying theoretical model a priori. To this end, we use a Markov Chain Monte Carlo analysis to perform comparisons to the supernova Ia union 2 compilation, combined with the Hubble Space Telescope measurements of the Hubble constant, and the Hubble parameter datasets. The cosmographic approach to our analysis is revisited and extended for new notions of redshift presented as alternatives to the redshift z. Furthermore, we introduce a new set of fitting parameters describing the kinematical evolution of the Universe in terms of the equation of state of the Universe and derivatives of the total pressure. Our results are consistent with the ΛCDM model, although alternative models, with nearly constant pressure and no cosmological constant, match the results accurately as well.
Explore related subjects
Keep this discovery
Alejandro Aviles, Christine Gruber, Orlando Luongo, Hernando Quevedo. 2013-01-17. Constraints from Cosmography in various parameterizations. https://arxiv.org/abs/1301.4044
Cite the original work for its findings. Save a collection to share your selection of sources.