Testing a Dilaton Gravity Model Using Nucleosynthesis

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...

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Main Authors: S. Boran, E. O. Kahya
Format: Article
Language:English
Published: Wiley 2014-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2014/282675
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author S. Boran
E. O. Kahya
author_facet S. Boran
E. O. Kahya
author_sort S. Boran
collection DOAJ
description 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.
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spelling doaj-art-d3d43c059f1a495bb85665a6048c1ced2025-02-03T01:07:04ZengWileyAdvances in High Energy Physics1687-73571687-73652014-01-01201410.1155/2014/282675282675Testing a Dilaton Gravity Model Using NucleosynthesisS. Boran0E. O. Kahya1Department of Physics, İstanbul Technical University, Maslak, 34469 Istanbul, TurkeyDepartment of Physics, İstanbul Technical University, Maslak, 34469 Istanbul, TurkeyBig 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.http://dx.doi.org/10.1155/2014/282675
spellingShingle S. Boran
E. O. Kahya
Testing a Dilaton Gravity Model Using Nucleosynthesis
Advances in High Energy Physics
title Testing a Dilaton Gravity Model Using Nucleosynthesis
title_full Testing a Dilaton Gravity Model Using Nucleosynthesis
title_fullStr Testing a Dilaton Gravity Model Using Nucleosynthesis
title_full_unstemmed Testing a Dilaton Gravity Model Using Nucleosynthesis
title_short Testing a Dilaton Gravity Model Using Nucleosynthesis
title_sort testing a dilaton gravity model using nucleosynthesis
url http://dx.doi.org/10.1155/2014/282675
work_keys_str_mv AT sboran testingadilatongravitymodelusingnucleosynthesis
AT eokahya testingadilatongravitymodelusingnucleosynthesis