Reconstruction of f(G) gravity with polytropic and Chaplygin gas dark energy models
Department of Physics, Faculty of Basic Sciences, University of Mazandaran, P. O. Box 47416-95447, Babolsar, Iran
* e-mail: firstname.lastname@example.org
Accepted: 8 August 2017
Published online: 15 September 2017
We consider the modified Gauss-Bonnet gravity and reconstruct this theory from some dark energy scenarios such as the polytropic, generalized Chaplygin and modified Chaplygin gas models. We perform a numerical analysis with the best fit values from the observational data for the model parameters space and find that the reconstructed models lead to an effective quintessence acceleration phase. Furthermore, we investigate the stability of the calculated models through the squared speed of sound parameter.
© Società Italiana di Fisica and Springer-Verlag GmbH Germany, 2017