We study the intermediate evolution model and show that, compared with the recent study of a power-law evolution, the intermediate evolution is a better description of the low-redshift regime supported by observations from type Ia supernovae and BAO. We found also that recent data suggest that the intermediate evolution is as good a fit to this redshift range as the ΛCDM model.
Cite
@article{arxiv.1509.04924,
title = {Intermediate evolution using SNIa, and BAO},
author = {V. H. Cardenas and O. Herrera},
journal= {arXiv preprint arXiv:1509.04924},
year = {2015}
}
Comments
7 pages, 5 figures. Accepted in Astrophysics and Space Science