dc.creatorFranchino Viñas, Sebastián Alberto
dc.creatorMazzitelli, Francisco Diego
dc.date2021-03
dc.date2022-10-11T17:54:43Z
dc.date.accessioned2023-07-15T05:13:22Z
dc.date.available2023-07-15T05:13:22Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/143583
dc.identifierissn:2470-0010
dc.identifierissn:2470-0029
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7472545
dc.descriptionWe study the vacuum fluctuations of a quantum scalar field in the presence of a thin and inhomogeneous flat mirror, modelled 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 inhomogeneites, the Wick-rotated effective action gives the probability of particle creation due to the dynamical Casimir effect.
dc.descriptionFacultad de Ciencias Exactas
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsCreative Commons Attribution 4.0 International (CC BY 4.0)
dc.subjectCiencias Exactas
dc.subjectFísica
dc.subjectvacuum fluctuations
dc.subjectinhomogeneities
dc.titleEffective action for delta potentials: Spacetime-dependent inhomogeneities and Casimir self-energy
dc.typeArticulo
dc.typeArticulo


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