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By L. Marton

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S. Masower, J . Tech. Phys. ) 9, 808 (1939); N. D. Morgulis anu B. I. Djatlowitskaja, ibid. 10,637 (1940); Izvest. Akad. , Ser. Fiz. 12, 126 (1948); N. Schaetti and W. Baumgartner, Helv. Phys. Acta. 24, 614 (1951); R. Suhrmann and C. Kangro, Naturwiss. 40, 137 (1953); L. I. Schafratowa-Ekertowa, J . Tech. Phys. J. Harper and W. J. Choyke, J . Appl. Phys. 27, 745 (1956). 11. N. S. Chlebnikow, J . Tech. Phys. ) 16, 745 (1946). 12. D. A. ” Wiley, New York, 1950. 13. KI and RbI: L. Apker and E. Taft, Phys.

With the magnetic field H upward, the counting rate was (12 f 3)% lower than with H downward, indicating that the positrons are preferably emitted along the direction ofithe nuclear spin (in contrast to the electrons from Co6O). Postma et al. ( I S ) have shown that their observed P-asymmetry is compatible with the value predicted - - 42 R. M. STERNHEIMER by the two-component neutrino theory (with V A interaction): /3 = +v,/c [see Eq. (17)]. Their results are thus also in agreement with the observations of Ambler et al.

Wonssowski et al. (39). 28 P. GORLICH puted the probability for the incidence of simultaneous absorption of two or more light quanta by one electron. Although the probability of a secondorder photoelectric effect in metallic surfaces is small, there may be certain instances where it must be taken into account. It goes without saying that the theoretical deliberations on the photoeffect of metals also affect the considerations on the photoeffect of semiconductors. Thus, the calculations (LO)of the probability of releasing electrons from a surface band or from surface levels had broad successes; of course, the limitations on the validity of the equations arrived a t were clear cut.

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