Casimir Effect in $E^3$ closed spaces
Mariana P. Lima, Daniel Muller

TL;DR
This paper calculates the Casimir energy density for a massless scalar field in all compact orientable Euclidean 3-spaces, revealing independence from curvature coupling and providing numerical visualizations.
Contribution
It derives finite Epstein zeta function sums for Casimir energy in all compact orientable Euclidean 3-spaces, expanding understanding of topology's role in quantum field effects.
Findings
Casimir energy density is independent of curvature coupling.
Explicit finite sums for all compact orientable Euclidean 3-spaces.
Numerical plots illustrate energy distribution within Dirichlet regions.
Abstract
As it is well known the topology of space is not totally determined by Einstein's equations. It is considered a massless scalar quantum field in a static Euclidean space of dimension 3. The expectation value for the energy density in all compact orientable Euclidean 3-spaces are obtained in this work as a finite summation of Epstein type zeta functions. The Casimir energy density for these particular manifolds is independent of the type of coupling with curvature. A numerical plot of the result inside each Dirichlet region is obtained.
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