Investigation of space-times through W2-curvature tensor in f (R,G) gravity

The W-2-curvature tensor is an important geometric invariant with relativistic significance, introduced in the early 1970s by Pokhariyal and Mishra, which can be identified in class 4 in the classification of skew-symmetric operators. In this work, we investigate 4-dimensional space-times admitting W-2-curvature tensor in f (R, G) modified theory of gravity. It is proved that the W-2-curvature flat perfect fluid space-times obeying f (R, G) gravity represent inflation. Also, it is shown that the isotropic pressure and the energy density of such space-times are constant. It is to be noted that in such space-times the considered energy conditions are consistently satisfied if the scalar curvature is positive. Next, we study perfect fluid space-times admitting divergence free W-2-curvature tensor in f (R, G) gravity. Amongst other results, we prove that if the energy-momentum tensor of such space-times is bi-recurrent, then either the space-times represent inflation or their isotropic pressure and energy density are constants.(c) 2023 Elsevier B.V. All rights reserved.

Automated summary

This paper investigates space-times with W-2 curvature tensor in f (R, G) modified theory of gravity and space-times with divergence-free W-2 curvature tensor in f (R, G) gravity. It is found that space-times with W-2 curvature tensor represent inflation and have constant isotropic pressure and energy density. For space-times with divergence-free W-2 curvature tensor, it is proven that if the energy-momentum tensor is bi-recurrent, then either the space-times represent inflation or have constant isotropic pressure and energy density.