Energy conditions in f(R) gravity and Brans-Dicke theories

Abstract

The equivalence between f(R) gravity and scalar-tensor theories is invoked to study the null, strong, weak and dominant energy conditions in Brans-Dicke theory. We consider the validity of the energy conditions in Brans-Dicke theory by invoking the energy conditions derived from a generic f(R) theory. The parameters involved are shown to be consistent with an accelerated expanding universe.

9 pages, 1 figure, to appear in IJMPD

References in corpus (2)

• Energy conditions in f(R)-gravity
• Energy Conditions and Cosmic Acceleration

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