Table of Contents
Fetching ...

Semiclassical Gravity Beyond General Relativity: Insights from Torsion

R. Morales-Cabrera, Y. Bonder

TL;DR

The paper addresses incorporating quantum matter effects into gravity with torsion by extending semiclassical gravity to Einstein–Cartan theory and applying Hadamard renormalization to a nonminimally coupled Klein–Gordon field. It develops a Wald-like axiomatic framework and a point-splitting renormalization scheme that yield finite, renormalized energy–momentum and spin densities, while making explicit the scale and renormalization ambiguities via a differential-form renormalization Lagrangian. It further shows that the conformal anomaly persists in the presence of torsion, with the state-dependent term $v_1$ driving the anomaly. Overall, the work demonstrates that semiclassical methods provide a robust and informative approach to exploring torsionful modifications of gravity and their potential phenomenology.

Abstract

We develop a semiclassical theory of modified gravity with nontrivial spacetime torsion. In particular, we show that the semiclassical treatment can be axiomatized in the case of Einstein--Cartan theory with a nonminimally coupled, free Klein--Gordon field, in four dimensions. Using Hadamard renormalization, we obtain well-defined expectation values for both, the energy--momentum and spin--density operators. These objects exhibit scale and renormalization ambiguities; we identify the latter by constructing a renormalization Lagrangian in terms of differential forms, which are particularly well suited for this purpose. Furthermore, we analyze the conformal anomaly, which persists in the presence of torsion.

Semiclassical Gravity Beyond General Relativity: Insights from Torsion

TL;DR

The paper addresses incorporating quantum matter effects into gravity with torsion by extending semiclassical gravity to Einstein–Cartan theory and applying Hadamard renormalization to a nonminimally coupled Klein–Gordon field. It develops a Wald-like axiomatic framework and a point-splitting renormalization scheme that yield finite, renormalized energy–momentum and spin densities, while making explicit the scale and renormalization ambiguities via a differential-form renormalization Lagrangian. It further shows that the conformal anomaly persists in the presence of torsion, with the state-dependent term driving the anomaly. Overall, the work demonstrates that semiclassical methods provide a robust and informative approach to exploring torsionful modifications of gravity and their potential phenomenology.

Abstract

We develop a semiclassical theory of modified gravity with nontrivial spacetime torsion. In particular, we show that the semiclassical treatment can be axiomatized in the case of Einstein--Cartan theory with a nonminimally coupled, free Klein--Gordon field, in four dimensions. Using Hadamard renormalization, we obtain well-defined expectation values for both, the energy--momentum and spin--density operators. These objects exhibit scale and renormalization ambiguities; we identify the latter by constructing a renormalization Lagrangian in terms of differential forms, which are particularly well suited for this purpose. Furthermore, we analyze the conformal anomaly, which persists in the presence of torsion.

Paper Structure

This paper contains 18 sections, 75 equations, 3 tables.