Torsion, Scalar Field and f(\mathcal{R}) Gravity
Prasanta Mahato

TL;DR
This paper explores how torsion and a scalar field in Riemann-Cartan geometry relate to f(R) gravity, showing the scalar field's connection to Ricci scalar and Newton's constant, thus linking torsion, scalar fields, and modified gravity.
Contribution
It demonstrates that a specific Lagrangian with torsion and scalar field reduces to an f(R) gravity theory, revealing new insights into their interrelation.
Findings
Divergence of axial torsion yields Newton's constant.
Scalar field becomes a function of Ricci scalar R.
Lagrangian reduces to f(R) gravity form.
Abstract
The role of torsion and a scalar field in gravitation in the background of a particular class of the Riemann-Cartan geometry is considered here. Some times ago, a Lagrangian density with Lagrange multipliers has been proposed by the author which has been obtained by picking some particular terms from the SO(4,1) Pontryagin density, where the scalar field causes the de Sitter connection to have the proper dimension of a gauge field. Here it has been shown that the divergence of the axial torsion gives the Newton's constant and the scalar field becomes a function of the Ricci scalar . The starting Lagrangian then reduces to a Lagrangian representing the metric gravity theory.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Advanced Differential Geometry Research
