Displaying 1 - 10 of total 27 results:
Family background, early life in Brooklyn and Detroit, high school; undergraduate studies at University of Michigan, switch from mathematics to physics. Graduate work at Michigan, 1931-1933; thesis research combines quantum mechanics and infrared spectroscopy. Difficulty finding academic job during Depression; works for Lowell Observatory while at Michigan, 1933-1936; devises long-path absorption cell, research in infrared spectrum of earth's atmosphere. Joins faculty of Johns Hopkins University (Gerhard Dietz), 1935-1936. To Lowell Observatory (Roger Lowell Putnam, V. M. Slipher, E. C.
Includes information on his pre-Harvard education and postdoctoral experience; pre-World War II work at Harvard with students and in building of the cyclotron; wartime work on radar in U.S. and Britain; move to the Manhattan Project and responsibility for Trinity Test site; return to Harvard and start of new cyclotron building.
This interview describes Bainbridge’s return to Harvard after his time in Los Alamos. His first task was the construction of a new cyclotron. He also helped to get the Physics Department back into prominence, attracting and retaining (or not) colleagues who had been doing war work. Examples of the former are Purcell and Ramsey and of the latter, R. R. Wilson. Bainbridge describes his time as department chairman, setting up the Loeb Lectureship which persists to this day.
Recollections of physics community in 1920s and early 1930s; opportunities for physics work in Europe; awareness of political climate in Germany (1932); relationship with Werner Heisenberg at University of Leipzig; awarded Rockefeller Fellowship to study at University of Rome; contacts with physicists after Leipzig and before Rome; John Von Neumann's list of refugee physicists; offered appointment to position at Stanford University; visit to University of Copenhagen and Niels Bohr's advice to accept appointment; relinquishing of second half of fellowship; influenced by Bohr, Heisenberg and
Interview focusses on early life in Vienna, family and religion; atmosphere in Vienna in early 1930s; growth of interest in mathematical physics; anti-Semitism in Vienna; influence of history teacher and rejection of religion; influence of reading Eddington and Jeans in the mid-1930s; further study in England and contact with Eddington; Trinity College, 1937-1940; study with Besicovitch; collapse of plebiscite and family in Vienna; internment during World WarII; graduate study with Harold Jeffreys; naval radar, 1942; associates during war and circle at Cambridge; development of radar resear
Topics discussed include: his family history, his educational background, beginnings of nuclear physics and particle acceleration, Cockcroft-Walton generator, his fellowship at the Massachusetts Institute of Technology (MIT), his World War II research at the MIT radiation lab on radar systems, his time at the Brookhaven National Laboratory, his work with various accelerators including the Cosmotron, and his time with the Atomic Energy Commission and the National Science Foundation.
Childhood in Germany and family background — competitive spirit; war years — internment and radar work with Bondi and Hoyle (1942-1945) at Cambridge — development of theory of hearing and steady state theory; at Greenwich (1952-1956) — research on lunar surface and terrestrial dynamics; positions at Harvard and Cornell — involvement with Arecibo; involvement with governmental agencies including NSF and NASA — changes in government funding. A major part of the interview covers the development and reception of the steady date theory.