Testing a Dilaton Gravity Model Using Nucleosynthesis

S. Boran*, E. O. Kahya

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

6 Citations (Scopus)

Abstract

Big bang nucleosynthesis (BBN) offers one of the most strict evidences for the Λ -CDM cosmology at present, as well as the cosmic microwave background (CMB) radiation. In this work, our main aim is to present the outcomes of our calculations related to primordial abundances of light elements, in the context of higher dimensional steady-state universe model in the dilaton gravity. Our results show that abundances of light elements (primordial D, 3He, 4He, T, and 7Li) are significantly different for some cases, and a comparison is given between a particular dilaton gravity model and Λ -CDM in the light of the astrophysical observations.

Original languageEnglish
Article number282675
JournalAdvances in High Energy Physics
Volume2014
DOIs
Publication statusPublished - 2014

Bibliographical note

Publisher Copyright:
© 2014 S. Boran and E. O. Kahya.

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