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Cosmological applications in Kaluza–Klein theory |
| M. I. Wanasa)c)d), Gamal G. L. Nashedb)c)d)†, and A. A. Nowayae) |
a. Astronomy Department, Faculty of Science, Cairo University, Giza, Egypt;
b. Mathematics Department, Faculty of Science, King Faisal University, P.O. Box 380 Al-Ahsaa 31982, the Kingdom of Saudi Arabia;
c. Mathematics Department, Faculty of Science, Ain Shams University, Cairo, 11566, Egypt;
d. Center for Theoretical Physics, British University of Egypt Sherouk City 11837, P.O. Box 43, Egypt;
e. Egyptian Relativity Group (ERG), Physics Department, Faculty of Science, Monofia University, Monofia, Egypt |
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Abstract The field equations of Kaluza-Klein (KK) theory have been applied in the domain of cosmology. These equations are solved for a flat universe by taking the gravitational and the cosmological constants as a function of time t. We use Taylor's expansion of cosmological function, $\varLambda$(t), up to the first order of the time t. The cosmological parameters are calculated and some cosmological problems are discussed.
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Received: 28 September 2011
Revised: 26 October 2011
Accepted manuscript online:
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PACS:
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98.80.-k
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(Cosmology)
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98.80.Jk
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(Mathematical and relativistic aspects of cosmology)
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04.50.Cd
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(Kaluza-Klein theories)
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Corresponding Authors:
Gamal G. L. Nashed,nashed@bue.edu.eg
E-mail: nashed@bue.edu.eg
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Cite this article:
M. I. Wanas, Gamal G. L. Nashed, and A. A. Nowaya Cosmological applications in Kaluza–Klein theory 2012 Chin. Phys. B 21 049801
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