Implications of the Holst term in a $f(R)$ theory with torsion
Flavio Bombacigno, Giovanni Montani

TL;DR
This paper explores a modified $f(R)$ gravity theory with torsion and a dynamical Immirzi field, revealing unique gravitational wave polarizations that differ from General Relativity and could be experimentally detectable.
Contribution
It introduces a novel $f(R)$ gravity model with a Holst term and Immirzi field, analyzing its effects on gravitational wave polarization and torsion elimination.
Findings
Scalar mode of $f(R)$ is frozen out in linearized theory
Emergence of a modified Newtonian potential
Detection of anomalous gravitational wave polarizations
Abstract
We analyze a modified theory of gravity in the Palatini formulation, when an Holst term endowed with a dynamical Immirzi field is included. We study the basic features of the model, especially in view of liminating the torsion field via the Immirzi field and the scalar-tensor degrees of freedom of the model. The main task of this study is the investigation of the morphology of the gravitational wave polarization when their coupling to a circle of test particles is considered. We first observe that the dynamics of the scalar mode of the Lagrangian is frozen out, since its first order term identically vanishes. This allows a detailed characterization of the linearized theory, which outlines the emergence of a modified Newtonian potential in the static limit, and when time independence is relaxed a standard gravitational wave plus the scalar wave associated to the…
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