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DeWitt-Schwinger renormalization and vacuum polarization in d dimensions

Journal Article · · Physical Review. D, Particles Fields
 [1];  [1]
  1. Centro Multidisciplinar de Astrofisica-CENTRA, Departamento de Fisica, Instituto Superior Tecnico-IST, Universidade Tecnica de Lisboa-UTL, Av. Rovisco Pais 1, 1049-001 Lisboa (Portugal)
Calculation of the vacuum polarization, <{phi}{sup 2}(x)>, and expectation value of the stress tensor, <T{sub {mu}}{sub {nu}}(x)>, 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 d dimensions includes d-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 <{phi}{sup 2}(x)> and <T{sub {mu}}{sub {nu}}(x)> calculations and a thorough introduction to the method of calculating <{phi}{sup 2}(x)>, 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 <{phi}{sup 2}(x)> and <T{sub {mu}}{sub {nu}}(x)> 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 <{phi}{sup 2}(x)> for certain spacetimes is discussed, with application to four and five dimensions.
OSTI ID:
21322730
Journal Information:
Physical Review. D, Particles Fields, Journal Name: Physical Review. D, Particles Fields Journal Issue: 6 Vol. 80; ISSN PRVDAQ; ISSN 0556-2821
Country of Publication:
United States
Language:
English

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