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In this interview, Edward Uhler Condon discusses topics such as: his family background; early education; influence of high school physics teacher, William Howell Williams, 1914-1918, and later teacher at University of California, Berkeley; interval as boy reporter. Undergraduate years at Berkeley, beginning in 1921 in chemistry department; Ph.D. in physics, 1926; association with Fred Weinberg. Discovery of Erwin Schrödinger's wave mechanics papers; International Education Board fellowship to study quantum mechanics at Göttingen, 1926. Work on Bell Systems technical journal for six months before accepting lectureship at Columbia University; teaching post at Princeton University; Condon and Philip Morse's Quantum Mechanics, result of Columbia and Princeton courses. Relations with University of California; role in persuading Ernest Lawrence to go to Berkeley from Yale University. Recollections of Michigan summer school. Work at Westinghouse on applications of nuclear physics to industry, including completion of Van de Graaff machine, 1937-1940; setting up Westinghouse research fellowships, 1938; Massachusetts Institute of Technology conference on applications of nuclear physics, October 1940; war work on microwave radar. J. Robert Oppenheimer asks Condon to come to Los Alamos Scientific Laboratory; tour of Los Alamos with Leslie Groves; reasons for leaving Los Alamos after a few weeks. Work as head of theoretical section of Lawrence's laboratory, August 1943-1945; British scientists. Evaluation of Westinghouse's four million-volt machine. Description of Nimitron, a physical computer, designed for 1939 World's Fair. Discussion of 1928 radioactivity. Reminiscences of Ronald Gurney's later career and his trouble with security. Discussion of postwar events, such as the Quebec Conference, McMahon Act, Moran's book about Winston Churchill. Peacetime development of atomic energy; establishment of the Senate's Special Committee on atomic energy. Directorship of the National Bureau of Standards (NBS), 1945-1951. Work on superconductivity; W. Emmanuel Maxwell and John Pelham. Accomplishments at NBS. Hearings in 1948 and 1952 before the Department of Commerce under Truman's loyalty program; Averell Harriman. Director of Research at Corning, 1951. House Un-American Activities Committee hearing, 1954; J. R. Oppenheimer and Bernard Peters; reopening of clearances, loss of Corning position; becomes Corning consultant. Head of Washington University physics department, 1956-1963; Oberlin College, 1962; interest in modernizing teaching; Joint Institute for Laboratory Astrophysics (JILA), from 1963; editor of Reviews of Modern Physics, 1957-1968; establishment of the National Accelerator Laboratory (Chicago); the UFO story. Comments on his most satisfying and his least satisfying work. Also prominently mentioned are: Raymond T. Birge and Henry Wallace.
Born 1910 Rhode Island. Engineering interest at an early age; Massachusetts Institute of Technology undergraduate, aeronautical engineering; graduate studies in physics (John Slater, Philip Morse); assistant to Stark Draper, 1932-1934; fellowship at University of Cambridge (Professor Ralph H. Fowler); internal conversion of x-rays (with Geoffrey I. Taylor, 1934); MIT Ph.D. (P. Morse) scattering of slower electrons; William Shockley; junior fellow at Harvard University, 1936-1938; work with Ivan Getting on an electrostatic generator; Harvard Society of Fellows; Bell Laboratories, 1939 (Shockley-Fisk fission work); war work mostly electronics; interaction with industrial research and with universities, 1946 reorganization of physics department forming a solid state physics group; team representing various disciplines to study fundamentals of solid state (Fisk associate director); Director of Research, U.S. Atomic Energy Commission, 1947; professor at Harvard, 1948; Director of Physics Research at Bell Labs, 1949; President of Bell Labs. Also prominently mentioned are: John Bardeen, Oliver E. Buckley, Karl Taylor Compton, Frank Jewett, J. B. Johnson, Ralph Johnson, Mervin J. Kelly, and Gerald Leondus Pearson.
Childhood and early education in New York, undergraduate education in philosophy at Columbia College, 1932-1936; years of graduate study in physics at Columbia University, 1936-1937; influence of Isidor I. Rabi, the joint NYU-Columbia seminar in physics; transfer to Cornell University for graduate work in nuclear physics, 1937-1939; influence of Hans Bethe; thesis work on white dwarfs; first teaching position at University of Rochester, joint work with Victor Weisskopf in nuclear physics and particles; remarks on war years, astrophysics, cyclotrons, and other matters; Shelter Island Conferences. Formation of the Federation of American Scientists (F.A.S.) in 1946; Marshak succeeds Robert Wilson as Chairman, 1947. World Federation of Scientific workers, chaired by Frédéric Joliot-Curie, wants to enroll F.A.S. (1947, in Paris meeting). Marshak's work on two-meson theory. F.A.S. issues in the 1950s; the Emergency Committee and F.A.S.; Einstein's interests and views on relation of science to society; comments on J. Robert Oppenheimer; chairmanship at University of Rochester; Lee DuBridge; long-range plan and extensive development of physics department funded through AEC contracts; training of students from abroad such as Okubo, Sudarshan, Messiah, Regge. Last half of interview covers the Rochester conferences. Scientific work during the 1950s, the V-A interaction (George Sudarshan) theory (a.k.a. Feynman-Gell-Mann theory of weak interactions); books and works with graduate students. Travels to Europe and India (Tata Institute), 1953. Accepts City College (CUNY) presidency; reasons for leaving University of Rochester. Also prominently mentioned are: Robert Fox Bacher, Subrahmanyan Chandrasekhar, George Braxton Pegram, Julian R. Schwinger, Edward Teller; Lawrence Radiation Laboratory, and Massachusetts Institute of Technology Radiation Laboratory.
<p>Then, the project finally got authorized in 1961 — but again after a rather amusing set of coincidences. At that time the Stanford project was sort of known as the Republican project because Eisenhower had proposed it to a Democratic Congress. At that time there was a project that the Democrats wanted in Congress which the Republican administration did not want. This was for the Hanford Reactor to generate power into the electrical net, because it was considered to be socialized electricity by the Republicans, to have power generated by a production reactor. There was also good economic and technical reasons against such a project. It’s a very inefficient reactor, for power generation because of the low temperature at which the Hanford reactor operates. Anyway, the Democrats wanted it and the Republicans didn't.</p>
<p>On the other hand, the Stanford linear accelerator was considered to be a Republican proposal, opposed by the Democrats. So after a while the Republicans and Democrats in the Joint Committee essentially said, "If you approve Hanford, then we approve Stanford." So it ended up with both of them getting approved, and it was this entirely political infighting in the Congress which resulted in that last hurdle being passed. However in 1960, we already had very good confidence that it would go, because the three million dollars was fundamentally a signal to us that Congress really meant it but that they wanted to slap Mr. Eisenhower’s wrist for non-consultation.</p>
Piore's involvement in science research policies; establishment of the Office of Naval Research and its relationship with institutions such as the National Science Foundation, National Science Board, Atomic Energy Commission, and the President's Science Advisory Committee; funding of large-scale research (SLAC and other accelerator centers). Education, from high school (Ethical Culture Society, New York City) and college years at University of Wisconsin (Ph.D. in physics, 1935). Career at Radio Corporation of America (RCA) and Columbia Broadcasting System (CBS), 1935-1942; work at Bureau of Ships during World War II, involving radar research, conventional weapons development, use of the atomic bomb, and early Russian space research. Also mentioned at length are: John Van Vleck, Raymond Herb, Ralph H. Fowler, Robert Serber, and Fritz Zworykin.