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Gravitational vacuum polarization II: Energy conditions in the Boulware vacuum

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arxiv gr-qc/9604008 v1 pith:WVKIIQSF submitted 1996-04-03 gr-qc hep-th

Gravitational vacuum polarization II: Energy conditions in the Boulware vacuum

classification gr-qc hep-th
keywords conditionsenergyvacuumeventhorizonquantumviolatedboulware
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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I show that in the Boulware vacuum (1) all standard (point-wise and averaged) energy conditions are violated throughout the exterior region---all the way from spatial infinity down to the event horizon, and (2) outside the event horizon the standard point-wise energy conditions are violated in a maximal manner: they are violated at all points and for all null/timelike vectors. (The region inside the event horizon is considerably messier, and of dubious physical relevance. Nevertheless the standard point-wise energy conditions also seem to be violated even inside the event horizon.) This is rather different from the case of the Hartle--Hawking vacuum, wherein violations of the energy conditions were confined to the region inside the unstable photon orbit. These calculations are for the quantum stress-energy tensor corresponding to a conformally-coupled massless scalar field in the Boulware vacuum. I work in the test-field limit, restrict attention to the Schwarzschild geometry, and invoke a mixture of analytical and numerical techniques. This *suggests* that general self-consistent solutions of semiclassical quantum gravity might *not* satisfy the energy conditions, and may in fact for certain quantum fields and certain quantum states violate *all* the energy conditions.

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