One-loop $\lambda \phi^4$ theory in Robertson-Walker spacetimes: adiabatic regularization and analytic approximation

TL;DR

This paper develops an adiabatic regularization method for $mbda 4$ scalar field theory in Robertson-Walker spacetimes, providing numerical and analytic tools for calculating the energy-momentum tensor and backreaction effects.

Contribution

It introduces a variation of adiabatic regularization that yields analytic approximations for the energy-momentum tensor and effective mass, facilitating self-consistent backreaction calculations.

Findings

The full renormalized energy-momentum tensor is conserved.

Analytic approximations produce conserved energy-momentum tensors.

The method is suitable for numerical and analytic studies of quantum fields in cosmology.

Abstract

The renormalization of a scalar field theory with a quartic self-coupling (a $\lambda \phi^4$ theory) via adiabatic regularization in a general Robertson-Walker spacetime is discussed. The adiabatic counterterms are presented in a way that is most conducive to numerical computations. A variation of the adiabatic regularization method is presented which leads to analytic approximations for the energy-momentum tensor of the field and the quantum contribution to the effective mass of the mean field. Conservation of the energy-momentum tensor for the field is discussed and it is shown that the part of the energy-momentum tensor which depends only on the mean field is not conserved but the full renormalized energy-momentum tensor is conserved as expected and required by the semiclassical Einstein's equation. It is also shown that if the analytic approximations are used then the resulting approximate energy-momentum tensor is conserved. This allows a self-consistent backreaction calculation to be performed using the analytic approximations. The usefulness of the approximations is discussed.