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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.
Childhood and major influences; college education at Harvard University; position at Edward C. Worden Co., position at Columbia University's chemistry department as a graduate student and instructor, as a professor, and as the department chairman; history of chemistry department's administration. Major emphasis on his research results and papers spanning his entire career; Hammett equation and acidity theory; his contact with students Henry P. Treffers, Martin Paul, Lois Zucker. Work during the World War I and World War II; consulting work; development of the field of physical organic chemistry and opinion of the future of chemistry. Philosophy of research; talk with Mrs. Hammett. Also prominently mentioned are: Roger Adams, Adkins, Bernard Auchincloss, Paul Doughty Bartlett, Hal Beans, Ernst Bodenstein, Marston Bogert, Branch, Breslow, Johannes Brn︣sted, Joseph Bunnett, Burkhardt, Mary Caldwell, Ray Christ, James Bryant Conant, Ralph Connor, Alder J. Deyrup, John R. Dunning, Henry Eyring, Leo Flexser, George S. Forbes, Ernie Grunwald, Janet Hammett, Arthur R. Hantzsch, Christopher Ingold, Iserman, James Kendall, Elmer Kohler, A. B. Lamb, Irving Langmuir, Jose Levy, Gilbert Newton Lewis, Willard Frank Libby, Bill McEwan, J. L. R. Morgan, Rosetta Natoli, J. M. Nelson, James Flack Norris, Louis Plack, Michael Polanyi, T. W. Richards, R. Robinson, Smith, Alexander Smith, E. F. Smith, Hermann Staudinger, Julius Stieglitz, Arthur Thomas, Harold Clayton Urey, George Walden, Chaim Weizmann, E. C. Worden, Theodore Zucker, Dick Zuemer; Alpha Chi Sigma Fraternity, American Chemical Society, Commercial Solvents Co., E. I. duPont de Nemours & Company, Inc., Eidgenössische Technische Hochschule at Zurich, Johns Hopkins University, Manhattan Project, Petroleum Research Fund, Rohm and Haas Co., United States President's Science Advisory Committee, Universal Oil Production Corporation, University of California at Los Angeles, University of Illinois, and University of Wisconsin.
Childhood and major influences; college education at Harvard University; position at Edward C. Worden Co., position at Columbia University's chemistry department as a graduate student and instructor, as a professor, and as the department chairman; history of chemistry department's administration. Major emphasis on his research results and papers spanning his entire career; Hammett equation and acidity theory; his contact with students Henry P. Treffers, Martin Paul, Lois Zucker. Work during the World War I and World War II; consulting work; development of the field of physical organic chemistry and opinion of the future of chemistry. Philosophy of research; talk with Mrs. Hammett. Also prominently mentioned are: Roger Adams, Adkins, Bernard Auchincloss, Paul Doughty Bartlett, Hal Beans, Ernst Bodenstein, Marston Bogert, Branch, Breslow, Johannes Brn︣sted, Joseph Bunnett, Burkhardt, Mary Caldwell, Ray Christ, James Bryant Conant, Ralph Connor, Alder J. Deyrup, John R. Dunning, Henry Eyring, Leo Flexser, George S. Forbes, Ernie Grunwald, Janet Hammett, Arthur R. Hantzsch, Christopher Ingold, Iserman, James Kendall, Elmer Kohler, A. B. Lamb, Irving Langmuir, Jose Levy, Gilbert Newton Lewis, Willard Frank Libby, Bill McEwan, J. L. R. Morgan, Rosetta Natoli, J. M. Nelson, James Flack Norris, Louis Plack, Michael Polanyi, T. W. Richards, R. Robinson, Smith, Alexander Smith, E. F. Smith, Hermann Staudinger, Julius Stieglitz, Arthur Thomas, Harold Clayton Urey, George Walden, Chaim Weizmann, E. C. Worden, Theodore Zucker, Dick Zuemer; Alpha Chi Sigma Fraternity, American Chemical Society, Commercial Solvents Co., E. I. duPont de Nemours & Company, Inc., Eidgenössische Technische Hochschule at Zurich, Johns Hopkins University, Manhattan Project, Petroleum Research Fund, Rohm and Haas Co., United States President's Science Advisory Committee, Universal Oil Production Corporation, University of California at Los Angeles, University of Illinois, and University of Wisconsin.
Born in Mexico; interested in geology at a young age. Attended Harvard University, majoring in geology; formal physics education limited to half a term; early contacts with Edward M. Purcell, Julian R. Schwinger, and Nicolaas Bloembergen; James Thomson, Albert F. Burch, and George Kennedy most influential teachers; early interest in science policy. Professor at Massachusetts Institute of Technology, exposure to computers; transition to University of California, Los Angeles, 1958; collaboration with Walter Munk on geophysics text; affiliations with NASA and Goddard Space Institute; director of Atmospheric Research Laboratory, 1960. Early JASON involvement after invitation from Murray Gell-Mann; hiatus from JASON, 1970-1977; concurrent involvement with PSAC; relations with fellow JASON members regarding ABM testimony and acid rain; JASON's transition from IDA to SRI and then to MITRE; technical advice and policy implications.
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.
This interview deals with Siegman's education, from 1949 to 1957, as an undergraduate at Harvard University, Hughes Aircraft Company work-study fellow at the University of California in Los Angeles, and a Ph.D. candidate at Stanford University. Also prominently mentioned are: Hubert Heffner, Rudolf Kompfner, Frederick Emmons Terman, Ping K. Tien, Dean A. Watkins, Joseph Weber, and John R. Whinnery.
In this interview, David Zierler, Oral Historian for AIP, interviews Robert Finkelstein, (deceased in August 2020) formerly professor emeritus, department of physics, University of California, Los Angeles (UCLA). Finkelstein describes his early interests in physics and his undergraduate education at Dartmouth College, and he describes his formative summer at Columbia University, where he studied under I.I. Rabi. He discusses he graduate work at Harvard University under the direction of John van Vleck, and he discusses van Vleck’s fundamental contributions to quantum mechanics. Finkelstein describes his postdoctoral work expanding on Niels Bohr’s capacity to deal with magnetism, and he discusses his work with Francis Bitter at Massachusetts Institute of Technology (MIT). He describes his conscription to the Navy during World War II, where he worked on mine warfare, and he explains his close relationship with George Gamow and his work on tunneling in quantum mechanics and general relativity. Finkelstein discusses his postwar work at Fermilab, where he became interested in meson physics, and he describes his position at the Institute for Advanced Study at Princeton as a postdoctoral researcher under Robert Oppenheimer, where he continued to work on mesons. He describes getting to know at the Institute, he discusses his first contact with the Feynman diagrams, and he recounts how Jack Steinberger used his calculations which were in agreement with the diagrams. Finkelstein discusses his decision to join the faculty at UCLA, and he explains his opinion that Julian Schwinger was a “deeper” thinker than Feynman. He explains the originals of his unitary field theory, and he describes his contributions to the concept of supergravity. At the end of the interview, Finkelstein explains his ongoing interest with improving upon the Standard Model, and he reflects on the incredible level of understanding about the cosmos that has been developed over the course of his career.
In this interview, Joanna Behrman, Assistant Public Historian for AIP, interviews Margaret Kivelson, Distinguished Professor Emerita of Space Physics at the University of California, Los Angeles. Kivelson recounts her childhood in New York City and her decision to attend Radcliffe College. She describes her experiences attending graduate school at Harvard University and working with Julian Schwinger. Kivelson explains her decision to move out to California, to work at the RAND Corporation, and her efforts to secure a position at UCLA. Kivelson describes how UCLA became a hub for space physics research and her work on the magnetometers for various projects including OGO-5, Pioneer 11, and Galileo. Kivelson also discusses her work to improve the status of women in academia on the Harvard Board of Overseers and at UCLA.