AAWSAP DIRD, Quantum Tomography of Negative Energy States in the Vacuum, January 2011
DOW-UAP-D153 · page 18 of 51
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UNCLASSIFIED//FOR OFFICUtt H.!l! er~tv Casimir Vacuum plates fluctuations Figure 2. Schematic of the Casimir Effect. It turns out that there are many different types of Casimir effects found in quantum field theory [20-22, 26-28, 51]. For example, if one introduces a single infinite plane conductor into the Minkowski (flat spacetime) vacuum by bringing it adiabatically from infinity so that whatever quantum fields are present suffer no excitation but remain in their ground states, then the vacuum (electromagnetic) stresses induced by the presence of the infinite plane conductor produces a Casimir effect. This result holds equally well when two parallel plane conductors (with separation distance d) are present, which gives rise to the familiar Casimir effect inside a cavity. Note that in both cases, the spacetime manifold is made incomplete by the introduction of the plane conductor boundary condition(s). The vacuum region put under stress by the presence of the plane conductor(s) is called the Casimir vacuum. The generic expression for the energy density of the Casimir effect is PCE =- Ahcd-4 , where A= C,(D)/8rr-2 in spacetimes of arbitrary dimension O [20-22]. The appearance of the zeta-function (,(D) is characteristic of expressions for vacuum stress-energy tensors, T.J:i~ .t t t In our familiar 4-dimensional spacetime (0 = 4) we have that A = rc2/720. To calculate T_J:i~ for a given quantum field is to calculate its associated Casimir effect. We should also point out that the methods used to obtain the quantum vacuum electromagnetic T;~~ between parallel plane conductors can also be used when the conductors are not parallel but are joined together along a line of intersection. If the conductors have curved surfaces instead, then one obtains results that are similar to the case of intersecting conductors. These geometries have also been evaluated for the ttt The Greek tensor indices (µ, v = 0...3) denote spacetime coordinates, >l'...x3, such that xt...x 3 = space coordinates and x0 "' time coordinate. Note in general that T00 = p E (field energy density). UNCLASSIFIED/,'FOR OFFI&I.t..k W&li OPtk\S 14