Displaying 1 - 10 of total 16 results:
Discusses his childhood and education in Illinois, undergrad and graduate work at Harvard; writing his thesis with Van Vleck; working at Bell Laboratoreis and the scientists there including William Shockley; the rise of interest in solid state physics in the early 1950s; research in superconductivity; the creation of theory groups at Bell Labs in 1956 and the relationship between theorists and experimenters in the lab; decisions on research topics at Bell; his year in Japan with Kubo; security restrictions at Bell and military research; collaborations with John Galt; experiments leading to
Family background; undergraduate and graduate studies at Princeton University: electrical engineering 1921, graduate research on ionization of argon and HC1, spectroscopic interests, (MA 1924, PhD 1925); developmental research as engineer for American Telephone and Telegraph Laboratories (1921–23); National Research Council Fellow at Harvard University (1925–27); Bartol Research Foundation Fellow (1927–29), research on “impact of protons on atoms and molecules.” Assistant professor at Cornell University (1929–31), high voltage x-ray research, visit to Cavendish Laboratory, associations (193
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
In this interview, Geoffrey Burbidge discusses the history of physics over the course of his career. Topics discussed include: Astronomical Society of the Pacific; E. Margaret Burbridge; American Astronomical Society; Hale Observatory; Lick Observatory; radio astronomy; Naval Research Laboratory; x-ray astronomy; Bruno Rossi; optical astronomy; Kitt Peak National Observatory; air and light pollution; Allan Sandage; Harvard University; Princeton University; Lord Kelvin; S.
A thorough, reflective survey of the life and work of this theoretical astrophysicist. Early life and education in India, 1910-1930, and experiences at Trinity College, University of Cambridge, 1930-1937, with comments on Edward A. Milne and Arthur S. Eddington; debate with the latter over collapse of white dwarf stars. Move to U.S. in 1937, with comments on the situation at Harvard and Princeton Universities since the 1930s, and especially on Henry N. Russell, John Von Neumann, and Martin Schwarzschild.
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.
Life and career to 1965.
This interview was conducted for McCrosky's biographical profile and especially to gain insight into his work and training at Harvard in the 1940s and his professional career at the Smithsonian Astrophysical Observatory from the 1950s through the 1980s.It includes commentary on family background, early schooling, development of interests, jobs as a child and as a student, work with brother at MIT, courses at Akron University in chemistry, wartime training in meteorology at Denison University, colleagues during wartime including Harlan Smith, duty in Hawaii, return to MIT in physics with Har
Developments of the technique of separated oscillating fields and the atomic clock. Move to Harvard University from Columbia University and Brookhaven National Laboratory; work at Harvard concentrating on the first molecular beam magnetic resonance apparatus, doctoral thesis of Harwood Kolsky; Jerrold Zacharias and the cesium beam clock; Brookhaven Molecular Beam Conferences (beginning 1947), significant developments in resonance. Also prominently mentioned are: P. I. Dee, Harwood Kolsky, Polykarp Kusch, William Aaron Nierenberg, Pendulchron, Ken Smith, John Hasbrouck Van Vleck, Robert F.
Student years at University of Cambridge, 1919-1923; move to Harvard University in 1923, and subsequent career. Comments on being a woman studying physics at Cambridge in the 1920s; influences of Ernest Rutherford, Arthur Eddington and Edward Milne on her career choice; some of her early research. Move to Harvard (inspired by lecture by Harlow Shapley). At Harvard, work (virtually alone) on stellar spectra; encouragement of Shapley and Annie J. Cannon. Publications on stellar atmospheres and variable stars; anecdotes about including E.C. Pickering, Henry N. Russell, Raymond S.