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Reference24 articles.
1. See, for example,D. J. Gross:Nucl. Phys. B,132, 439 (1978);P. Tataru-Mihai:On the two-dimensional O(3) σ-nonlinear model, preprint Starnberg University (1978);V. de Alfaro, S. Fubini andG. Furlan:Nonlinear sigma model and classical solutions, preprint ICTP-Trieste 78/69 (1978);H. Eichenherr:Nucl. Phys. B,146, 215 (1978);H. J. Borchers andW. D. Garber:Analyticity of solutions of the O(N) nonlinear σ-model, preprint University of Göttingen (July 1979);Local theory of solutions for the O(2k+1) σ-model, preprint University of Göttingen (October 1979);D. Maison:Some facts about classical nonlinear σ-models, preprint Max-Planck Institut für Physik und Astrophysik, München, MPI-PAE/PTh 52/79 (November 1979).
2. V. De Alfaro, S. Fubini andG. Furlan:Nuovo Cimento A,50, 523 (1979).
3. S. M. Christensen andM. J. Duff:Quantizing gravity with a cosmological constant, preprint University of California, Santa Barbara ITP-79-01 (October 1979).
4. J. A. Wheeler: inRelativity Groups and Topology, edited byB. S. De Witt andC. M. De Witt (New York, N. Y., 1964).
5. S. W. Hawking:Nucl. Phys. B,144, 349 (1978).
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