2005
DOI: 10.1088/0264-9381/22/19/022
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Stress tensor for massive fields on flat spaces of spatial topology

Abstract: We calculate the expectation values of the energy-momentum tensor T µν for massive scalar and spinor fields, in the Minkowski-like vacuum states on the two flat spaces which are quotients of Minkowski space under the discrete isometries (t, x, y, z) → (t, x, y, z + 2a) and (t, x, y, z) → (t, −x, −y, z + a). The results on the first space confirm the literature. The results on the second space are new. We note some qualitative differences between the massless and massive fields in the limits of large a and larg… Show more

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Cited by 4 publications
(11 citation statements)
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“…Boundary conditions enter because our result could equally be stated as the infimum as h varies over the range of T n in L 1 , all elements of which obey the specific boundary conditions we have imposed. In fact, (17) was used to obtain a result quite similar in spirit to our main result: namely, that While the strategy employed in [6] overlaps in part with ours, the key portions of the two arguments (leading to (17) in [6], or our bounds on λ n ) are quite different.…”
Section: Results For Other L P Spacesmentioning
confidence: 60%
See 1 more Smart Citation
“…Boundary conditions enter because our result could equally be stated as the infimum as h varies over the range of T n in L 1 , all elements of which obey the specific boundary conditions we have imposed. In fact, (17) was used to obtain a result quite similar in spirit to our main result: namely, that While the strategy employed in [6] overlaps in part with ours, the key portions of the two arguments (leading to (17) in [6], or our bounds on λ n ) are quite different.…”
Section: Results For Other L P Spacesmentioning
confidence: 60%
“…Consider the cylinder spacetime (N, η) formed by periodically identifying four-dimensional Minkowski space under a translation in the z-direction. The ground state energy density in this spacetime, for the quantized minimally coupled scalar field of mass m is [23,17]…”
Section: Example: Cylinder Spacetimesmentioning
confidence: 99%
“…Let us note that the massless QEI bound also provides a lower bound on the ground state energy densities of massive scalar fields in these spacetimes. Consistency here is seen from the fact that the mass diminishes the magnitude of the energy density [51] (note the misprints in [51] noted in [52] which do not, however, affect the final result).…”
Section: A Two-dimensional Timelike Cylindermentioning
confidence: 55%
“…Finally let us consider M − [9,10,31] which is a quotient of Minkowski space (or of M 0 , it being a double cover of M − ) under the map J − : (t, x, y, z) → (t, −x, −y, z + a). Our interest in M − , as well as it being an interesting topologically non-trivial spacetime in which we can probe the effect of topology on the Unruh effect, lies in its role in modelling, via accelerated observers on flat spacetimes, the Hawking(-Unruh) effect on the RP 3 geon [9].…”
Section: Scalar Detector On M −mentioning
confidence: 99%
“…In contrast to the analogous result on M with boundary, there is no divergence here at x = 0 as there is no obstruction there and the inertial detector on M − carries through x = 0 smoothly. Note that on M − the energy-momentum tensor expectation values are finite over the whole spacetime [9,31], while on M with boundary they diverge at x = 0. For ω > 0 the M 0 part of the transition rate vanishes while the image part is odd in τ .…”
Section: Inertial Detectormentioning
confidence: 99%