Different parametrizations of field equations in the $f(R)$ theories of gravity
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TL;DR
This paper explores two different parametrizations of field equations in $f(R)$ gravity theories, analyzing their impact on curvature pressure and density, and providing formulas to convert between these parametrizations.
Contribution
It introduces and compares two parametrizations of field equations in $f(R)$ gravity, detailing their effects on curvature quantities and conditions for significant differences.
Findings
Different parametrizations yield distinct curvature pressure and density results.
Formulas are provided to convert between parametrizations.
Conditions are identified under which results significantly differ.
Abstract
In this paper we describe two different parametrizations of field equations in the theories of gravity and two resulting parametrizations of the Friedmann Equations. In particular we show how these two parametrizations lead to two different results for the curvature pressure and the curvature density obtained respectively as the component and the component of the curvature stress-energy tensor. We introduce formulas in order to pass from one parametrization to another one for the curvature pressure and the curvature density. Furthermore, we analyse under which conditions the two parametrizations of the curvature stress-energy tensor lead to significantly different results.
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Black Holes and Theoretical Physics
