Interacting Quantum Field Theory in de Sitter Vacua
Martin B. Einhorn, Finn Larsen

TL;DR
This paper clarifies the nature of quantum field theory in de Sitter space, emphasizing the importance of correlation function analyticity for defining vacua and developing perturbation theory.
Contribution
It demonstrates that the Mottola-Allen vacuum ambiguity is an artifact of free theory and establishes analyticity as a fundamental principle for interacting quantum fields in curved spacetime.
Findings
Mottola-Allen vacua are artifacts of free theory
Analyticity determines the vacuum uniquely in de Sitter space
Facilitates systematic perturbation theory development
Abstract
We discuss interacting quantum field theory in de Sitter space and argue that the Mottola-Allen vacuum ambiguity is an artifact of free field theory. The nature of the nonthermality of the MA-vacua is also clarified. We propose analyticity of correlation functions as a fundamental requirement of quantum field theory in curved spacetimes. In de Sitter space, this principle determines the vacuum unambiguously and facilitates the systematic development of perturbation theory.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Quantum Chromodynamics and Particle Interactions · Cosmology and Gravitation Theories
