Nuclear forces (Physics)

Arrival in the U.S. in 1930; comparison of social, scientific, general intellectual climates in U.S and Europe; early interest in nuclear physics, relationship with graduate students; beta decay, compound nucleus model, Breit-Wigner formula, early shell model; review articles by Bethe; relation of early meson theory to nuclear physics; nuclear forces; charge independence; journal literature of physics ca. 1937; effectiveness of group-theoretic models in nuclear physics; effectiveness of quantum mechanics for nuclear physics; significant early experimental discoveries in nuclear physics: neutron, deutron, artificial radioactivity; fission, shell model of Mayer and Jensen; rotational levels in nuclei; the specialization of physics; effect of World War II on nuclear physics research; work at Chicago; conferences after the war; branching off of high-energy physics from nuclear physics; work personally regarded as interesting.

Early career through 1939. Midwestern background; education at University of Texas, graduate work at Harvard University in theoretical physics under Edwin C. Kemble and John Van Vleck, 1929-1933; traveling fellowship (chiefly in Germany, 1932); positions at Harvard, University of Wisconsin, Princeton University, and New York University. The nature of theoretical nuclear physics work in the 1930s including nuclear models and Feenberg's work with Eugene P. Wigner on nuclear forces. Also prominently mentioned are: John Bardeen, Niels Henrik David Bohr, C. P. Boner, Gregory Breit, Walter M. Elsasser, Wendell Furry, George Gamow, Julian Knipp, Ettore Majorana, R. L. Moore, Otto Oldenburg, Melba Newell Phillips, Roberts, Simon Share, C. G. Smith, Arnold Johannes Wilhelm Sommerfeld, Carl Friedrich Weizsäcker, (Freiherr von); Institute for Theoretical Physics (Copenhagen), Niels Bohr Institutet, and Raytheon Corporation.

Early career through 1939. Midwestern background; education at University of Texas, graduate work at Harvard University in theoretical physics under Edwin C. Kemble and John Van Vleck, 1929-1933; traveling fellowship (chiefly in Germany, 1932); positions at Harvard, University of Wisconsin, Princeton University, and New York University. The nature of theoretical nuclear physics work in the 1930s including nuclear models and Feenberg's work with Eugene P. Wigner on nuclear forces. Also prominently mentioned are: John Bardeen, Niels Henrik David Bohr, C. P. Boner, Gregory Breit, Walter M. Elsasser, Wendell Furry, George Gamow, Julian Knipp, Ettore Majorana, R. L. Moore, Otto Oldenburg, Melba Newell Phillips, Roberts, Simon Share, C. G. Smith, Arnold Johannes Wilhelm Sommerfeld, Carl Friedrich Weizsäcker, (Freiherr von); Institute for Theoretical Physics (Copenhagen), Niels Bohr Institutet, and Raytheon Corporation.

Natural radioactivity; ideas of nuclear constitution, size in 1920s; Gamow-Condon-Gurney theory of alpha decay 1928; discovery of neutron 1932; Cambridge as a center of research 1933; early theories of nuclear forces; analysis of short-range nuclear forces 1935-40; reasons for writing Rev. Mod. Phys. review articles 1935-37 and detailed review of articles' contents; beta decay and the neutrino hypothesis; application of group-theoretic methods to nuclear physics 1936-37; compound nucleus model 1936; nuclear models in general (compound nucleus, evaporation, liquid drop, direct interaction, statistical); contemporary knowledge of nuclear physics 1938-39; stellar energy production; energy limit on cyclotron; accelerators and theoreticians; nuclear physics at Los Alamos; post-war conferences; origins and development of the shell model of the nucleus; many-body theory in nuclear physics; current algebras in particle physics; origins and development of the optical model; of the collective model; autobiographical comments on political, social, scientific conditions in Germany and England in early 1930s ; nuclear studies at Cornell after the war; building the H-bomb; the Oppenheimer hearings; work as a consultant 1950-1970; involvement with PSAC 1956; views on disarmament; receipt of 1967 Nobel Prize.

Natural radioactivity; ideas of nuclear constitution, size in 1920s; Gamow-Condon-Gurney theory of alpha decay 1928; discovery of neutron 1932; Cambridge as a center of research 1933; early theories of nuclear forces; analysis of short-range nuclear forces 1935-40; reasons for writing Rev. Mod. Phys. review articles 1935-37 and detailed review of articles' contents; beta decay and the neutrino hypothesis; application of group-theoretic methods to nuclear physics 1936-37; compound nucleus model 1936; nuclear models in general (compound nucleus, evaporation, liquid drop, direct interaction, statistical); contemporary knowledge of nuclear physics 1938-39; stellar energy production; energy limit on cyclotron; accelerators and theoreticians; nuclear physics at Los Alamos; post-war conferences; origins and development of the shell model of the nucleus; many-body theory in nuclear physics; current algebras in particle physics; origins and development of the optical model; of the collective model; autobiographical comments on political, social, scientific conditions in Germany and England in early 1930s ; nuclear studies at Cornell after the war; building the H-bomb; the Oppenheimer hearings; work as a consultant 1950-1970; involvement with PSAC 1956; views on disarmament; receipt of 1967 Nobel Prize.

Natural radioactivity; ideas of nuclear constitution, size in 1920s; Gamow-Condon-Gurney theory of alpha decay 1928; discovery of neutron 1932; Cambridge as a center of research 1933; early theories of nuclear forces; analysis of short-range nuclear forces 1935-40; reasons for writing Rev. Mod. Phys. review articles 1935-37 and detailed review of articles' contents; beta decay and the neutrino hypothesis; application of group-theoretic methods to nuclear physics 1936-37; compound nucleus model 1936; nuclear models in general (compound nucleus, evaporation, liquid drop, direct interaction, statistical); contemporary knowledge of nuclear physics 1938-39; stellar energy production; energy limit on cyclotron; accelerators and theoreticians; nuclear physics at Los Alamos; post-war conferences; origins and development of the shell model of the nucleus; many-body theory in nuclear physics; current algebras in particle physics; origins and development of the optical model; of the collective model; autobiographical comments on political, social, scientific conditions in Germany and England in early 1930s ; nuclear studies at Cornell after the war; building the H-bomb; the Oppenheimer hearings; work as a consultant 1950-1970; involvement with PSAC 1956; views on disarmament; receipt of 1967 Nobel Prize.