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by Pauli and Villars.4 It will be interesting to compare the present situation with the electromagnetic self-energy of the mesons as investigated by Heitler and McConnell.' I wish to express my thanks to Dr. S. T. Ma for many stimu- lating discussions. I am also indebted to Professor H. A. Bethe for some valuable comments. * State Scholar of the Government of India. 1 W. PauLli, and M. E. Rose, Phys. Rev. 49, 462 (1936). 2 S. N. Gupta, Proc. Phys. Soc. (to be published). 3R. P. Feynman, Phys. Rev. 74, 1430 (1948). 4 W. Pauli and F. Villars. Rev. Mod. Phys. 21, 434 (1949). 6 W. Heitler and J. McConnell, Nature 164, 218 (1949). Nuclear Gamma-Radiation of Cu"l F. BOEHM, J. P. BLASER, P. MARMIER, AND P. PREISWERK Department of Physics, Swiss Federal Institute of Technology, Zurich, Switzerland December 5, 1949 THE positron spectrum of Cu6' has been examined recently by Cook and Langer' with a large magnetic spectrometer. The experimental curves of these authors show a deviation from the Fermi distribution which is much larger than for Cu"4 and it seems possible that not all of this deviation arises from instru- mental factors. It is pointed
Physical Review – American Physical Society (APS)
Published: Jan 15, 1950
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