Casimir Energy of a Relativistic Perfect Fluid Confined to a D-dimensional Hypercube
arXiv:math-ph/0211059 · doi:10.1063/1.1531822
Abstract
Compact formulas are obtained for the Casimir energy of a relativistic perfect fluid confined to a -dimensional hypercube with von Neumann or Dirichlet boundary conditions. The formulas are conveniently expressed as a finite sum of the well-known gamma and Riemann zeta functions. Emphasis is placed on the mathematical technique used to extract the Casimir energy from a -dimensional infinite sum regularized with an exponential cut-off. Numerical calculations show that initially the Dirichlet energy decreases rapidly in magnitude and oscillates in sign, being positive for even and negative for odd . This oscillating pattern stops abruptly at the critical dimension of D=36 after which the energy remains negative and the magnitude increases. We show that numerical calculations performed with 16-digit precision are inaccurate at higher values of .
20 pages, 4 figures
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Cited by in corpus (7)
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