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arXiv · 1509.04924

Intermediate evolution using SNIa, and BAO

V. H. Cardenas·O. Herrera
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Abstract

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 $\Lambda$CDM model.

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V. H. Cardenas, O. Herrera. 2015-09-16. Intermediate evolution using SNIa, and BAO. https://doi.org/10.1007/s10509-015-2507-0

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