Energy-momentum distribution of a general plane symmetric spacetime in metric f(R) gravity
Morteza Yavari

TL;DR
This paper derives energy-momentum distributions for a plane symmetric spacetime in metric f(R) gravity, assuming constant Ricci scalar, and examines specific models satisfying this condition.
Contribution
It provides exact vacuum solutions and energy distribution expressions in metric f(R) gravity under constant Ricci scalar assumption, which is a novel analysis.
Findings
Energy distribution expressions derived for specific f(R) models
Models satisfy the constant curvature condition
Exact vacuum solutions obtained in the studied spacetime
Abstract
In this paper, the exact vacuum solution of a general plane symmetric spacetime is investigated in metric f(R) gravity with the assumption of constant Ricci scalar. For this solution, we have studied the generalized Landau-Lifshitz energy-momentum complex in this theory to determine the energy distribution expressions for some specific f(R) models. Also, we show that these models satisfy the constant curvature condition.
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Black Holes and Theoretical Physics
