Abstract
In this article, we review our recent works on fourth order Weyl gravity, and try to obtain same results for cosmological coefficients, using a different approach. Indeed we shall impose a de Sitter like condition on the original components of field equations. Afterwards using the reduced equations on a definite geometric background, we derive the same results as in [1], for same cosmological constraints.
Export citation and abstract BibTeX RIS
Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.