Stress-Energy Tensors for Higher Dimensional Gravity
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چکیده
We calculate, in the context of higher dimensional gravity, the stress-energy tensor and Weyl anomaly associated with anti-de Sitter and anti-de Sitter black hole solutions. The boundary counter-term method is used to regularize the action and the resulting stress-energy tensor yields both the correct black hole energies as well as a vacuum energy contribution which is interpreted as a Casimir energy. This calculation is done up to d = 8 (d being the boundary dimension). We confirm some results for d < 8 as well as comment on some new results. All results for d = 8 are new. PACS number(s): 04.20.H, 04.70.-s, 04.62.+v
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تاریخ انتشار 1999