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Paper detail

Casimir densities for a boundary in Robertson-Walker spacetime

For scalar and electromagnetic fields we evaluate the vacuum expectation value of the energy-momentum tensor induced by a curved boundary in the Robertson--Walker spacetime with negative spatial curvature. In order to generate the vacuum densities we use the conformal relation between the Robertson-Walker and Rindler spacetimes and the corresponding results for a plate moving by uniform proper acceleration through the Fulling--Rindler vacuum. For the general case of the scale factor the vacuum energy-momentum tensor is presented as the sum of the boundary free and boundary induced parts.

preprint2009arXivOpen access
A. A. SaharianM. R. Setare
astro-ph.COgr-qchep-thquant-ph
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A. A. SaharianM. R. Setare

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