Abstract
The theory of quantized fields in curved spacetime has reached a high level of development, and a number of important physical consequences have been predicted. By treating the metric of the gravitational field classically, one avoids the nonrenormalizability problems of quantized gravity, but nevertheless retains a wide domain of applicability. I have already given a recent review of quantized fields in curved spacetime [L. Parker, 1977], in which the creation of elementary particles by strong gravitational fields (as in cosmology and near black holes) was emphasized. The present lectures will emphasize material which was not covered in the previous review.
Work supported by the National Science Foudation(PHY77-07111).
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Parker, L. (1979). Aspects of Quantum Field Theory in Curved Space-Time: Effective Action and Energy-Momentum Tensor. In: Lévy, M., Deser, S. (eds) Recent Developments in Gravitation. NATO Advanced Study Institutes Series, vol 44. Springer, Boston, MA. https://doi.org/10.1007/978-1-4613-2955-8_6
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