Local and Global Casimir Energies: Divergences, Renormalization, and the Coupling to Gravity
Kimball A. Milton

TL;DR
This paper reviews the divergences in local and total Casimir energies, discusses their renormalization, and explores their coupling to gravity, emphasizing the physical significance of these infinities.
Contribution
It clarifies the distinction between divergences in local energy densities and total energies, and examines their implications for gravitational coupling and renormalization.
Findings
Divergences in local energy densities are consistent with Einstein's equations.
Total Casimir energy divergences can be absorbed into physical parameter renormalization.
Local energy-momentum tensor divergences couple to gravity, affecting mass renormalization.
Abstract
From the beginning of the subject, calculations of quantum vacuum energies or Casimir energies have been plagued with two types of divergences: The total energy, which may be thought of as some sort of regularization of the zero-point energy, , seems manifestly divergent. And local energy densities, obtained from the vacuum expectation value of the energy-momentum tensor, , typically diverge near boundaries. The energy of interaction between distinct rigid bodies of whatever type is finite, corresponding to observable forces and torques between the bodies, which can be unambiguously calculated. The self-energy of a body is less well-defined, and suffers divergences which may or may not be removable. Some examples where a unique total self-stress may be evaluated include the perfectly conducting spherical shell first considered by Boyer, a…
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