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This research applies open quantum system frameworks to analyze Unruh-DeWitt detector responses in impulsive plane wave spacetimes, offering non-perturbative insights into how gravitational and electromagnetic waves suppress excitation transitions. By calculating expectation values for position and momentum operators alongside transition probabilities, the study bridges theoretical quantum field theory with practical considerations for detectors operating in strong coupling regimes.
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Open quantum system approach to the Unruh-DeWitt detector in impulsive plane wave spacetimes

arXiv2 min read

arXiv:2608.19692v1 Announce Type: cross Abstract: In this paper we employ the open quantum system framework with the influence functional formalism to non-perturbatively analyze the response of an Unruh-DeWitt detector modeled as a harmonic oscillator which interacts with a massless scalar field in impulsive plane wave spacetimes. Subtracting the Minkowski results, we obtain the expectation values for $\langle Q^2 \rangle$, $\langle P^2 \rangle$, and $\langle \{Q,P\} \rangle$, along with transition probabilities $P_{0\rightarrow 1}$ from ground state to the first excited state of the detector due to the influence of the wave. Explicit calculations are performed for both a pure gravitational wave (vanishing Ricci tensor) and a null electromagnetic wave (vanishing Weyl tensor). In both scenarios, the wave suppresses excitation transitions. Since our approach is non-perturbative, we are able to consider cases with both weak and strong coupling constants.

Abstract:In this paper we employ the open quantum system framework with the influence functional formalism to non-perturbatively analyze the response of an Unruh-DeWitt detector modeled as a harmonic oscillator which interacts with a massless scalar field in impulsive plane wave spacetimes. Subtracting the Minkowski results, we obtain the expectation values for $\langle Q^2 \rangle$, $\langle P^2 \rangle$, and $\langle \{Q,P\} \rangle$, along with transition probabilities $P_{0\rightarrow 1}$ from ground state to the first excited state of the detector due to the influence of the wave. Explicit calculations are performed for both a pure gravitational wave (vanishing Ricci tensor) and a null electromagnetic wave (vanishing Weyl tensor). In both scenarios, the wave suppresses excitation transitions. Since our approach is non-perturbative, we are able to consider cases with both weak and strong coupling constants.

arXiv:2608.19692 [gr-qc]

(or arXiv:2608.19692v1 [gr-qc] for this version)

https://doi.org/10.48550/arXiv.2608.19692 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

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