Effective action for delta potentials: spacetime-dependent inhomogeneities and Casimir self-energy

We study the vacuum fluctuations of a quantum scalar field in the presence of a thin and inhomogeneous flat mirror, modeled with a delta potential. Using heat-kernel techniques, we evaluate the Euclidean effective action perturbatively in the inhomogeneities (nonperturbatively in the constant backgr...

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Bibliographic Details
Main Authors: Franchino-Viñas, Sebastián (Author) , Mazzitelli, Francisco D. (Author)
Format: Article (Journal)
Language:English
Published: 16 March 2021
In: Physical review
Year: 2021, Volume: 103, Issue: 6, Pages: 1-17
ISSN:2470-0029
DOI:10.1103/PhysRevD.103.065006
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1103/PhysRevD.103.065006
Verlag, lizenzpflichtig, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.103.065006
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Author Notes:S.A. Franchino-Viñas and F.D. Mazzitelli
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Summary:We study the vacuum fluctuations of a quantum scalar field in the presence of a thin and inhomogeneous flat mirror, modeled with a delta potential. Using heat-kernel techniques, we evaluate the Euclidean effective action perturbatively in the inhomogeneities (nonperturbatively in the constant background). We show that the divergences can be absorbed into a local counterterm and that the remaining finite part is in general a nonlocal functional of the inhomogeneities, which we compute explicitly for massless fields in D=4 dimensions. For time-independent inhomogeneities, the effective action gives the Casimir self-energy for a partially transmitting mirror. For time-dependent inhomogeneities, the Wick-rotated effective action gives the probability of particle creation due to the dynamical Casimir effect.
Physical Description:Online Resource
ISSN:2470-0029
DOI:10.1103/PhysRevD.103.065006