2020
DOI: 10.3390/universe6100181
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Quantum Vacuum Effects in Braneworlds on AdS Bulk

Abstract: We review the results of investigations for brane-induced effects on the local properties of quantum vacuum in background of AdS spacetime. Two geometries are considered: a brane parallel to the AdS boundary and a brane intersecting the AdS boundary. For both cases, the contribution in the vacuum expectation value (VEV) of the energy–momentum tensor is separated explicitly and its behavior in various asymptotic regions of the parameters is studied. It is shown that the influence of the gravitational field on t… Show more

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Cited by 9 publications
(8 citation statements)
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References 106 publications
(202 reference statements)
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“…The vacuum fluctuations of quantum fields along those dimensions are quantized and, as a consequence, contributions in the vacuum expectation values (VEVs) of physical observables appear that depend on the geometrical characteristics of the compactification. The effects of compactification on the properties of the quantum vacuum in locally AdS spacetime have been considered previously (for a recent review see [19]). The vacuum energy, the Casimir forces and the radion stabilization in braneworld models with compact dimensions were discussed in [20]- [24].…”
Section: Introductionmentioning
confidence: 99%
“…The vacuum fluctuations of quantum fields along those dimensions are quantized and, as a consequence, contributions in the vacuum expectation values (VEVs) of physical observables appear that depend on the geometrical characteristics of the compactification. The effects of compactification on the properties of the quantum vacuum in locally AdS spacetime have been considered previously (for a recent review see [19]). The vacuum energy, the Casimir forces and the radion stabilization in braneworld models with compact dimensions were discussed in [20]- [24].…”
Section: Introductionmentioning
confidence: 99%
“…For the field corresponding to M = −iγ (3) we get the boundary condition (5.3). The FC and the VEV of the energy-momentum tensor in the RSII model with a topological defect (for quantum effects in higher-dimensional generalizations of RSII model see [30] and references therein) are expressed by the formulas given above for respective boundary conditions taking w 0 = a and with an additional coefficient 1/2. The latter is related to the fact that in Z 2symmetric braneworld model the integral over y in the normalization condition for the fermionic modes goes over the region −∞ < y < +∞ instead of the region y ∈ [y 0 = 0, ∞) in our consideration above for the R-region.…”
Section: Vevs For the Second Representation And Applications In Rsii ...mentioning
confidence: 99%
“…The results given above can be directly applied for the investigation of the cosmic string induced effects in background of the Randall-Sundrum model with a single brane (RSII model) [69,70] (for quantum effects in higher-dimensional generalizations of RSII model see [71] and references therein). In the presence of cosmic string perpendicular to the brane, the corresponding background geometry contains two copies of the R-region that are identified by the Z 2 -symmetry with respect to the brane located at y = 0 (or at w = w 0 = a in terms of the coordinate w).…”
Section: Applications To Randall-sundrum Modelmentioning
confidence: 99%