Two-Fluid Cosmological Models in Kaluza-Klein Space Time
International Journal of Theoretical Physics, ISSN: 1572-9575, Vol: 52, Issue: 11, Page: 3999-4007
2013
- 9Citations
- 4Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Article Description
In this paper we presented a class of solutions of Einstein's field equations describing two-fluid models of the universe in a five dimensional spherical symmetric space time. In these models one fluid is the radiation distribution which represents the cosmic microwave background and the other fluid is the perfect fluid representing the matter content of the universe. The radiation and matter content of the universe are in interactive phase. Also we have discussed physical and kinematical behaviors of the model. © 2013 Springer Science+Business Media New York.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84884905270&origin=inward; http://dx.doi.org/10.1007/s10773-013-1713-1; http://link.springer.com/10.1007/s10773-013-1713-1; http://link.springer.com/content/pdf/10.1007/s10773-013-1713-1; http://link.springer.com/content/pdf/10.1007/s10773-013-1713-1.pdf; http://link.springer.com/article/10.1007/s10773-013-1713-1/fulltext.html; https://dx.doi.org/10.1007/s10773-013-1713-1; https://link.springer.com/article/10.1007/s10773-013-1713-1
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