Ontology type: schema:ScholarlyArticle
2006-01
AUTHORSR. Venkateswarlu, K. Pavan Kumar
ABSTRACTThe field equations of Barber's (1982) second self-creation theory of gravitation are solved for 5D Friedmann-Robertson-Walker space time using perfect fluid energy momentum tensor. By assuming an equation of state p= ε ρ, (0 ≤ ε ≤ 1), the solutions of the field equations, in different scenarios, in Barber's second self-creation theory are presented and discussed. Some properties of these models are also discussed. More... »
PAGES73-77
http://scigraph.springernature.com/pub.10.1007/s10509-006-7304-3
DOIhttp://dx.doi.org/10.1007/s10509-006-7304-3
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