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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 This is true for energies below -10’ GeV, but at extremely high energies (=lo4 GeV) cosmic rays will probably not be superseded by accelerators in any forseeable future. 0.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).