Abstract

In this work we study the dynamics of the Universe in $f(R)=\sqrt{{R}^{2}\ensuremath{-}{R}_{0}^{2}}$ modified gravity with the Palatini formalism. We use data from recent observations, such as the supernova type Ia Gold sample and Supernova Legacy Survey data, the size of the baryonic acoustic peak from the Sloan Digital Sky Survey , the position of the acoustic peak from the cosmic microwave background observations, and large-scale structure formation from the 2dFGRS survey, to put constraints on the parameters of the model. To check the consistency of this action, we compare the age of old cosmological objects with the age of the Universe. In the combined analysis with all the observations, we find the parameters of the model as ${R}_{0}={6.192}_{\ensuremath{-}0.177}^{+0.167}\ifmmode\times\else\texttimes\fi{}{H}_{0}^{2}$ and ${\ensuremath{\Omega}}_{m}={0.278}_{\ensuremath{-}0.278}^{+0.273}$.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.