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Childhood; early interest in science (astronomy). Member of Astronomical Society of the Pacific, 1928. Special student at University of California at Berkeley, 1931, with Donald H. Menzel’s help. Regular student from 1932; comments on teachers and fellow students at Berkeley Student Observatory. Summer assistantship at Lick Observatory (Nicholas Mayall, Arthur B. Wyse), life at Lick Observatory. To Harvard University in 1937 for graduate studies; comparison between Harvard and Berkeley/Lick; teaching assistant at Radcliffe; 3-year membership in Harvard Society of Fellows, from 1939, of enormous importance for his development; works with Menzel and James G. Baker on the Theory of Physical Processes in Gaseous Nebulae, 1937; Analysis of the Atmospheres of the A-type Dwarfs Gamma Geminorum and Sirius based on data from Louis Berman; Jesse Greenstein. Comments on Harvard Summer Schools, Harlow Shapley’ s Square.” Volunteer teacher of elementary physics courses from 1942 at Harvard. Lawrence Radiation Laboratory, 1943-1945; work involved evaluation of the chemists and the Counting Group’s output from the electromagnetic separation process. Job offer from University of Indiana (Frank Edmunson) accepted due to cutback at Radiation Laboratory. Indiana years, 1945-1948, very productive (drafts for two astrophysics books); problems getting telescope time at Yerkes Observatory and unsatisfactory living conditions leads to acceptance of a promising tenured position at Michigan, a center with very active research due to Leo Goldberg; Robert McMath’s influence in the department; Keith Pierce and Aller’s work on infrared solar spectrum. Work performed at Mt. Wilson Observatory and Dominion Astrophysical Observatory. Goldberg resigns in 1959; comments on Aller’s decision to leave Michigan; discussions of funding; “over-head” (Aller’s talk at an AAS Meeting); comparison of Lick Observatory and Kitt Peak Observatory policies. Work at Mt. Stromio Observatory, Australia on sabbatical visits, 1960, 1968-1969, 1977-1978. Overview of opinions of the present state of astronomy. Comments on personal life, wife and children.
This interview is concerned primarily with two periods in the life of Libby (1927-1940 and 1945-1954). After briefly discussing his early life and education, considerable attention is focused upon Libby's undergraduate, graduate, and post-graduate years (1927-1940) at the University of California, Berkeley. Major topics included are: growth of Berkeley science; Gilbert Lewis, Wendell Latimer and Ernest Lawrence; Libby's development of low-level counters; radiochemistry and discovery of isotopes; cross-disciplinary collaboration; Libby's interest in carbon-14; association with Samuel Ruben and Martin Kamen; hot atom chemistry and nuclear isomerism; Libby's experiences at Princeton during 1940-1941 (hot atom chemistry, development of heterogeneous catalysis and research on tritium) and his work on the chemistry of the diffusion process during WWII at Columbia University (Manhattan Project) are mentioned; the other major portion of the interview concentrates on Libby's development of the radiocarbon dating technique at the University of Chicago (1945-1954); special attention is devoted to: measurement of half-life of carbon-14; importance to Libby of Harold Urey; secrecy policy; collaboration with Aristid von Grosse, James Arnold and Ernest Anderson; improved counting technologies; first contacts with archaeologists; Viking Fund and cross-disciplinary collaboration; communicating ideas; Sunshine Project and fallout; AEC appointment; concluding remarks.
This interview is concerned primarily with two periods in the life of Libby (1927-1940 and 1945-1954). After briefly discussing his early life and education, considerable attention is focused upon Libby's undergraduate, graduate, and post-graduate years (1927-1940) at the University of California, Berkeley. Major topics included are: growth of Berkeley science; Gilbert Lewis, Wendell Latimer and Ernest Lawrence; Libby's development of low-level counters; radiochemistry and discovery of isotopes; cross-disciplinary collaboration; Libby's interest in carbon-14; association with Samuel Ruben and Martin Kamen; hot atom chemistry and nuclear isomerism; Libby's experiences at Princeton during 1940-1941 (hot atom chemistry, development of heterogeneous catalysis and research on tritium) and his work on the chemistry of the diffusion process during WWII at Columbia University (Manhattan Project) are mentioned; the other major portion of the interview concentrates on Libby's development of the radiocarbon dating technique at the University of Chicago (1945-1954); special attention is devoted to: measurement of half-life of carbon-14; importance to Libby of Harold Urey; secrecy policy; collaboration with Aristid von Grosse, James Arnold and Ernest Anderson; improved counting technologies; first contacts with archaeologists; Viking Fund and cross-disciplinary collaboration; communicating ideas; Sunshine Project and fallout; AEC appointment; concluding remarks.
In this interview, Melba Phillips discusses: Bryn Mawr College; group theory; Oppenheimer-Phillips process; Maria Goeppert-Mayer; teaching physics; Brooklyn College; her experience as a woman in physics; Freda Friedman Salzman; George Salzman; University of Minnesota; Frank Oppenheimer; Leo Nedelsky; Dave Bohm; Harvard University; Radcliffe College; University of California, Berkeley; status of professional women in the 1950s; Columbia University Radiation Laboratory; radar countermeasures; Federation of American Scientists; Association of Scientific Workers; Francis Bonner; May-Johnson bill; Los Alamos National Laboratory; Ed Condon; McCarthyism and universities; House Un-American Activities Committee (HUAC); Ellen Schrecker; Jim G. Crowther.
Early life in Illinois; B.S. from Purdue University under Karl Lark-Horovitz, 1929-1933. Visit to Technische Hochschule in Karlsruhe. Theoretical and experimental work and teaching at Harvard University, 1934-1941, under Emory L. Chaffee, Kenneth T. Bainbridge, John Van Vleck. World War II research on radar at MIT Radiation Laboratory, 1941-1946. Return to Harvard; teaching, nuclear magnetic resonance and 21-cm line research. Discusses government consulting work, 1950-1970, especially President's Science Advisory Committee, American Physical Society presidency; teaching at Harvard. Interests in astrophysics, developing physics curricula. Also prominently mentioned are: Kenneth Tompkins Bainbridge, Felix Bloch, Bobby Cutler, Robert Henry Dicke, Edwards, Dwight D. Eisenhower, Harold Ewen, Ferry, William Francis Giauque, William Webster Hansen, Malcolm Hebb, Ted Hunt, Lyndon B. Johnson, Fritz Leonhart, Dunlap McNair, Otto Oldenburg, Jan Hendrik Oort, Wolfgang Pauli, Robert V. Pound, Isidor Isaac Rabi, Norman Foster Ramsey, Franklin D. Roosevelt, Schnabel, Julian R. Schwinger, Francis Eugene Simon, Charles Steinmetz, Henry Torrey, Hendrik Christoffell van de Hulst, John Von Neumann, Isidor Walerstein, Walter Witzel, Hubert J. Yearian, Jerrold Reinach Zacharias; Bell System Technical Journal, Great Britain Royal Air Force Coastal Command, Radio Research Laboratory, Illinois Southeastern Telephone Co., Killian Committee, Lawrence Radiation Laboratory, National Academy of Sciences, Rijksuniversiteit te Leiden, Unitarian Church, United States Office of Naval Research, University of California at Berkeley, and Voice of America.
Early life in Illinois; B.S. from Purdue University under Karl Lark-Horovitz, 1929-1933. Visit to Technische Hochschule in Karlsruhe. Theoretical and experimental work and teaching at Harvard University, 1934-1941, under Emory L. Chaffee, Kenneth T. Bainbridge, John Van Vleck. World War II research on radar at MIT Radiation Laboratory, 1941-1946. Return to Harvard; teaching, nuclear magnetic resonance and 21-cm line research. Discusses government consulting work, 1950-1970, especially President's Science Advisory Committee, American Physical Society presidency; teaching at Harvard. Interests in astrophysics, developing physics curricula. Also prominently mentioned are: Kenneth Tompkins Bainbridge, Felix Bloch, Bobby Cutler, Robert Henry Dicke, Edwards, Dwight D. Eisenhower, Harold Ewen, Ferry, William Francis Giauque, William Webster Hansen, Malcolm Hebb, Ted Hunt, Lyndon B. Johnson, Fritz Leonhart, Dunlap McNair, Otto Oldenburg, Jan Hendrik Oort, Wolfgang Pauli, Robert V. Pound, Isidor Isaac Rabi, Norman Foster Ramsey, Franklin D. Roosevelt, Schnabel, Julian R. Schwinger, Francis Eugene Simon, Charles Steinmetz, Henry Torrey, Hendrik Christoffell van de Hulst, John Von Neumann, Isidor Walerstein, Walter Witzel, Hubert J. Yearian, Jerrold Reinach Zacharias; Bell System Technical Journal, Great Britain Royal Air Force Coastal Command, Radio Research Laboratory, Illinois Southeastern Telephone Co., Killian Committee, Lawrence Radiation Laboratory, National Academy of Sciences, Rijksuniversiteit te Leiden, Unitarian Church, United States Office of Naval Research, University of California at Berkeley, and Voice of America.
Slater leaves Harvard University for Massachusetts Institute of Technology in 1930 (Karl Compton) to build up Physics Department there; work on quantum electrodynamics. Growth of MIT Physics Department in the 1930s and 1940s, relations between experimentalists and theorists; discussion of works and publications during the 1930s. Changes in U.S. physics; overview of post-World War II physics to 1951, and reasons for establishing own research group; establishment of the Radiation Lab, 1940; magnetron work; Bell Labs visits, 1941-1942 and 1943-1945. Planning of postwar development in MIT Physics Department; transition from Radiation Lab to Research Lab of Electronics; formation of laboratories of nuclear science, acoustics, and spectroscopy; the Lincoln Laboratory, the Instrumental Lab; growth of nuclear branch of Physics Department; physics activity in general in postwar years, Solid State and Molecular Theory Group; the Compton Lab.; Materials Science Center established ca. 1958; interdepartmental and interdisciplinary work; visits to Brookhaven National Laboratory; Slater and Per Olov Lowdin’s Florida Group. Also prominently mentioned are: John Bardeen, W. Buechner, Arthur Holly Compton, Edward Uhler Condon, Jens Dahl, Robley Dunglison Evans, James Brown Fisk, George Harrison, Douglas Rayner Hartree, Raymond George Herb, Milton Stanley Livingston, Millard Manning, Jacob Millman, Wayne B. Nottingham, Isidor Isaac Rabi, Schafer, William Shockley, R. A. Smith, Julius Stratton, Robert Jamison Van de Graaff, John Hasbrouck Van Vleck, Eugene Paul Wigner; American Physical Society, California Institute of Technology, Florida State University, Lawrence Radiation Laboratory, Princeton University, University of Bristol, University of California at Berkeley, and University of Chicago.
Slater leaves Harvard University for Massachusetts Institute of Technology in 1930 (Karl Compton) to build up Physics Department there; work on quantum electrodynamics. Growth of MIT Physics Department in the 1930s and 1940s, relations between experimentalists and theorists; discussion of works and publications during the 1930s. Changes in U.S. physics; overview of post-World War II physics to 1951, and reasons for establishing own research group; establishment of the Radiation Lab, 1940; magnetron work; Bell Labs visits, 1941-1942 and 1943-1945. Planning of postwar development in MIT Physics Department; transition from Radiation Lab to Research Lab of Electronics; formation of laboratories of nuclear science, acoustics, and spectroscopy; the Lincoln Laboratory, the Instrumental Lab; growth of nuclear branch of Physics Department; physics activity in general in postwar years, Solid State and Molecular Theory Group; the Compton Lab.; Materials Science Center established ca. 1958; interdepartmental and interdisciplinary work; visits to Brookhaven National Laboratory; Slater and Per Olov Lowdin’s Florida Group. Also prominently mentioned are: John Bardeen, W. Buechner, Arthur Holly Compton, Edward Uhler Condon, Jens Dahl, Robley Dunglison Evans, James Brown Fisk, George Harrison, Douglas Rayner Hartree, Raymond George Herb, Milton Stanley Livingston, Millard Manning, Jacob Millman, Wayne B. Nottingham, Isidor Isaac Rabi, Schafer, William Shockley, R. A. Smith, Julius Stratton, Robert Jamison Van de Graaff, John Hasbrouck Van Vleck, Eugene Paul Wigner; American Physical Society, California Institute of Technology, Florida State University, Lawrence Radiation Laboratory, Princeton University, University of Bristol, University of California at Berkeley, and University of Chicago.