DeWitt-Schwinger Renormalization and Vacuum Polarization in d Dimensions
arXiv:0811.3962 · doi:10.1103/PhysRevD.80.064017
Abstract
Calculation of the vacuum polarization, , and expectation value of the stress tensor, , has seen a recent resurgence, notably for black hole spacetimes. To date, most calculations of this type have been done only in four dimensions. Extending these calculations to dimensions includes -dimensional renormalization. Typically, the renormalizing terms are found from Christensen's covariant point splitting method for the DeWitt-Schwinger expansion. However, some manipulation is required to put the correct terms into a form that is compatible with problems of the vacuum polarization type. Here, after a review of the current state of affairs for and calculations and a thorough introduction to the method of calculating , a compact expression for the DeWitt-Schwinger renormalization terms suitable for use in even-dimensional spacetimes is derived. This formula should be useful for calculations of and in even dimensions, and the renormalization terms are shown explicitly for four and six dimensions. Furthermore, use of the finite terms of the DeWitt-Schwinger expansion as an approximation to for certain spacetimes is discussed, with application to four and five dimensions.
21 pages, 2 tables, 3 figures. References added, rewritten to clarify some points, corrections performed, our claim in the first version that there is an error in Anderson's calculations is incorrect
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- A Mode-Sum Prescription for Vacuum Polarization in Even Dimensions
- Self-energy of a scalar charge near higher-dimensional black holes
- Stress-energy tensor of the quantized massive fields in Schwarzschild-Tangherlini spacetimes. The back reaction
- Twist decomposition of proton structure from BFKL and BK amplitudes
- Vacuum polarization on the brane
- Vacuum polarization of the quantized massive scalar field in Reissner-Nordström spacetime
- Semiclassical lukewarm black holes
- Stress-energy tensor of quantized massive fields in static wormhole spacetimes
- Inside the Schwarzschild-Tangherlini black holes
- Vacuum polarization for varying quantum scalar field parameters in Schwarzschild-anti-de Sitter spacetime
- Black Hole Quantum Vacuum Polarization in Higher Dimensions
- Quantum vacuum polarization around a Reissner-Nordström black hole in five dimensions
- Classical and Quantum Thermodynamic Systems in Curved Spacetime