Abstract
In this work, we study the influence of the gravitational field induced by the presence of a cosmological constant [Formula: see text] on the Casimir energy density. We consider two metrics with the presence of the [Formula: see text]-term, namely de Sitter and Schwarzschild-de Sitter (SdS). In the former case, we consider a conformal de Sitter spacetime and in the last one, a weak gravitational SdS spacetime.
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