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Origin of interest in nuclear physics, discussions of compound nucleus, Copenhagen, 1936; work on interaction of evaporation and nuclear temperature, 1936; Breit-Wigner formula; application of evaporation model to nuclear reactions; postwar work in electrodynamics and nuclear reactions; relative merits of compound nucleus and shell models, 1950-51; explanation of independent particle motion by Pauli principle, 1951; estimates of shell model radiative transition probabilities; optical model and relation to compound nucleus models, 1953-55; emigration to U.S., 1937; initial impressions of Ame

Origin of interest in nuclear physics, discussions of compound nucleus, Copenhagen, 1936; work on interaction of evaporation and nuclear temperature, 1936; Breit-Wigner formula; application of evaporation model to nuclear reactions; postwar work in electrodynamics and nuclear reactions; relative merits of compound nucleus and shell models, 1950-51; explanation of independent particle motion by Pauli principle, 1951; estimates of shell model radiative transition probabilities; optical model and relation to compound nucleus models, 1953-55; emigration to U.S., 1937; initial impressions of Ame