On the Observer Dependence of the Quantum Effective Potential
arXiv:2303.04039 · doi:10.1007/s10714-025-03449-3
Abstract
In this short paper, we investigate the consequences of observer dependence of the quantum effective potential for an interacting field theory. Specializing to dimensional Euclidean Rindler space, we develop the formalism to calculate the effective potential. While the free energy diverges due to the presence of the Rindler horizon, the effective potential, which is a local function of space, is finite after the necessary renormalization procedure. We apply the results of our formalism to understand the restoration of spontaneously broken symmetry in three and four dimensions.
arXiv comment7 pages, 2 Figures, Included additional citations, corrected some typos, added more explanation and citations
References in corpus (14)
- The Unruh effect and its applications
- On Geometric Entropy
- Black Hole Entropy in Canonical Quantum Gravity and Superstring Theory
- Basics of thermal field theory -- a tutorial on perturbative computations
- Black Hole Entropy and Entropy of Entanglement
- Remarks on geometric entropy
- Thermodynamics of Quantum Fields in Black Hole Backgrounds
- Heat kernels and thermodynamics in Rindler space
- Unruh Acceleration Radiation Revisited
- Symmetry Restoration By Acceleration
- Triggering the QCD phase transition through the Unruh effect: chiral symmetry restoration for uniformly accelerated observers
- Free energy and entropy in Rindler and de Sitter space-times
- Wedges, Cones, Cosmic Strings, and the Reality of Vacuum Energy
- Revisiting Vacuum Energy in Compact Spacetimes