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6 , 322 (1963). 101. “La structure et I’Evolution de I’Univers,” Rapports et Discussions de I’onzienne Conseil de Physique, tenu A I’UniversitC de Bruxelles du 9 au 13 Juin 1958, R. Stoops, Bruxelles, 1958. 102. E. M. Burbidge, G. R. Burbidge, W. A. Fowler, and F. Hoyle, Rev. Mod. Phys.. 29, 547 (1957); Science, 124, 61 I (1956). 103. A. A. Penzias and R. H. Wilson, Asrr. J . , 142, 419 (1965). 104. J. R. Oppenheimer and H. Snyder, Phys. , 55, 455 (1939). 105. The Structure and Evolution of Galaxies, Proceedings of the Thirteenth Conference on Physics at the University of Brusselles, September 1964, Interscience.

Mag.. 1, 269 (1956). 90. Les hlictrons dans les Mgtaux, Rapports et Discussions du dixienne Conseil de Physique tenu a Bruxelles du 13 au 17 Septembre 1954, R. Stoops, Bruxelles, 1955. 91. J. Bardeen, L. N. Cooper, and J. R. Schrieffer, Phys. , 108, 1175 (1957). 92. Order and Fluctuations in Equilibrium and Non-Equilibrium Statistical Mechanics, G. Nicolis, G. Dewel, and J. W. , Wiley, New York, 1981. 93. K. G. Wilson and M. E. Fischer, Phys. Rev. , 28, 240 (1972); K. G. Wilson and J. Kogut, Phys.

M. Thomdike, and W. L. Whittermore, Phys. , 93, 861 (1954). 67. 68. 69. 70. 71. 72. 73. M. Gell-Mann and A. Pais, Proc. Glasgow Conf. , p. 342, Pergamon Press, London and New York, 1934; K. Nishijima, Prog. Theor. Phys. ( K y o t o ) , 12, 107 (1954). This is true for energies below -10’ GeV, but at extremely high energies (=lo4 GeV) cosmic rays will probably not be superseded by accelerators in any forseeable future. 0. Chamberlain, E. Segrt, C. Wiegand, and T. Ypsilantis, Phys. , 100,947 (1955).

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