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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3947
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dc.contributor.authorSivaram, C-
dc.contributor.authorCampanelli, M-
dc.date.accessioned2008-10-16T09:45:13Z-
dc.date.available2008-10-16T09:45:13Z-
dc.date.issued1992-08-
dc.identifier.citationAstrophysics and Space Science, Vol. 194, No. 2, pp. 239 - 244en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/3947-
dc.description.abstractTheories with Lagrangians nonlinear in the curvature scalar can be reduced by appropriate transformations to a form similar to the Brans-Dicke model. This may enable us to have extended inflation in the early universe without the difficulties of introducing scalar fields.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/q864036t35477v34/en
dc.subjectBig Bang Cosmologyen
dc.subjectGravitational Fieldsen
dc.subjectLagrangian Equilibrium Pointsen
dc.subjectUniverseen
dc.subjectGravitational Constanten
dc.subjectRelativityen
dc.titleNonlinear curvature Lagrangians and extended inflation in the early universeen
dc.typeArticleen
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