Radar Time and a State-Space Based Approach To Quantum Field Theory In Gravitational and Electromagnetic Backgrounds
Carl E. Dolby, Stephen F. Gull

TL;DR
This paper extends a radar time-based formalism for fermionic quantum field theory to include gravitational backgrounds, enabling observer-dependent particle interpretations in dynamic spacetimes without gauge or coordinate ambiguities.
Contribution
It generalizes the radar time approach to non-stationary gravitational backgrounds, providing a consistent, observer-dependent particle interpretation applicable to arbitrary motions and spacetimes.
Findings
Demonstrates consistency with known results in Rindler and de Sitter spaces.
Extends formalism to arbitrary 1+1D spacetimes and 3+1D FRW universes.
Discusses finite volume measurements and particle detection precision.
Abstract
In a recent paper (hep-th/0103228) a new initial value formulation of fermionic QFT was presented that is applicable to an arbitrary observer in any electromagnetic background. This approach suggests a consistent particle interpretation at all times, with the concept of `radar time' used to generalise this interpretation to an arbitrarily moving observer. In the present paper we extend this formalism to allow for gravitational backgrounds. The observer-dependent particle interpretation generalises Gibbons' definition to non-stationary spacetimes. This allows any observer to be considered, providing a particle interpretation that depends {\it only} on the observer's motion and the background, not on any choice of coordinates or gauge, or on details of their particle detector. Consistency with known results is demonstrated for the cases of Rindler space and deSitter space. Radar time is…
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Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Quantum Electrodynamics and Casimir Effect · Cosmology and Gravitation Theories
