Unruh effect in a real scalar field with the Higgs type potential on the de Sitter space

TL;DR

This paper investigates the Unruh effect's implications on a scalar field with Higgs potential in de Sitter space, predicting thermal radiation in the inertial frame and analyzing symmetry restoration and spacetime deformation.

Contribution

It introduces a novel analysis of the Unruh effect on a Higgs-type scalar field in de Sitter space, including one-loop potential corrections and spacetime deformation effects.

Findings

Restoration of spontaneous symmetry breaking at high Unruh temperatures

Deformation of background spacetime due to thermal corrections

Variation in energy related to changes in acceleration

Abstract

It has been predicted that an accelerating electron performs a Brownian motion in the inertial frame. This Brownian motion in the inertial frame has its roots in the interaction with the thermal excitation given by the Unruh effect in the accelerating frame. If such a prediction is possible, we correspondingly propose a prediction in this study that the thermal radiation appears in the inertial frame from an electron heated by the Unruh effect in the accelerating frame. The point in our prediction is, although the Unruh effect is only in the accelerating frame, if the appearance of the Brownian motion rooted in the Unruh effect in the inertial frame can be predicted, the heat that the particle gets in its body by the Unruh effect in the accelerating frame could survive in the inertial frame. Based on such a prediction, in this paper we investigate phenomena in the neighborhood of an accelerating electron in the inertial frame. The model we consider is the four-dimensional Klein-Gordon real scalar field model with the Higgs type potential term at the finite temperature identified with the Unruh temperature on the de Sitter space-time. We calculate the one-loop effective potential in the inertial frame with the corrections by the thermal radiation rooted in the Unruh effect in the accelerating frame. In this calculation, we take into account that the background space-time is deformed due to the field theory's corrected one-loop effective potential. Based on such an analysis, we illustrate the restoration of the spontaneous symmetry breaking and the variation of the background space-time, and we examine the accelerating particle's world-line and the amount of the energy corresponding to the change of the acceleration.