Displaying 1 - 10 of total 11 results:
Family background; early interest in mathematics; physics at University of Manchester; Ernest Rutherford's influence; early research under Rutherford at Manchester; examination by Joseph J. Thomson for degree; recollections of associates at Manchester, including Niels Bohr; scholarship to Universität Berlin and work there with Hans Geiger; internment during World War I; scientific work at internment camp; return to Manchester; move with Rutherford to University of Cambridge; appointment as Assistant Director of Research at Cavendish Laboratory (ca.
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.
Gamow's involvement with nuclear physics. His later work in astrophysics and his interest in biology. Personal anecdotes about Gamow's childhood in Odessa, student life with Lev Landau and Dmitriy Ivanenko at the University of Leningrad, his fellowship at Göttingen, work in Copenhagen with Niels Bohr, and at University of Cambridge with Ernest Rutherford. Emigration to America in 1934, subsequent work in the United States. Work on penetration barriers, saturation, the beta decay rule, and the nuclear droplet model.
Early education, Real-gymnasium; Universität Berlin, 1930; early interest in physics; courses, books studied, method of noting original ideas; University of Cambridge, 1933; first formal paper on nuclear physics; reaction in Berlin to discovery of neutron, colloquium of Lise Meitner; beta decay and the neutrino hypothesis; working habits at Cavendish Laboratory; collaboration with James Chadwick; photodisintegration of the deuteron; work with slow neutrons; circumstances of move to U.S., 1938; consequences of death of Ernest Rutherford on research at Cavendish Laboratory; use of proportiona
In this interview Fred Hoyle discusses his childhood and growing up in Yorkshire; parental background and influences; early reading in science; early experience with literature; influence of Eddington's books; education at Cambridge; interest in mathematics; early interest in exploring cosmology after World War II; history of development of steady state model; influence of Dirac and preference for understanding mathematics first; thesis work with Dirac; personality of Dirac; history of work on nucleosynthesis in stars: the Cavendish Laboratory, nucleosynthesis in supernovae, carbon producti
This interview was conducted as part of the Archives for the History of Quantum Physics project, which includes tapes and transcripts of oral history interviews conducted with circa 100 atomic and quantum physicists. Subjects discuss their family backgrounds, how they became interested in physics, their educations, people who influenced them, their careers including social influences on the conditions of research, and the state of atomic, nuclear, and quantum physics during the period in which they worked.
Discussion includes his background in wave mechanics; educational background; undergraduate work at the University of Cambridge (circa 1925-1930); Niels Bohr Institute, Copenhagen (1928-1929); University of Gottingen (1929); teaching mathematics at the University of Cambridge; Kapitza Club; work with George Gamow, Niels Bohr, Charlie Ellis, Harrie Massey.
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.
Family background; education at Tubigen Univ.; Schrodinger Theory thesis at Univ. of Munich (1927), influence of Sommerfeld, Heisenberg. Potsdam experiments inspired by K. Schwarzschild, Emden: Local thermodynamic equilibrium and curve of growth. Spent 1928 at Mt. Wilson. Return to Germany to teach physics during Depression; use of microphotometer, Coude spectrograph; analysis of Tau Scorpii. Pre-war professorship at Yerkes with Struve: line profile information, stellar composition. WWII return to Kiel, star temperature detection, solar spectrum analysis, elements/energy production.
Early life and family origins; Phillips Andover Academy; teachers; Andover and Max Millikan; early interest in astronomy; methodology of science; undergraduate years at Yale University; hobbies, teachers at Yale; physics and Alan Waterman; interest in particle accelerator; extracurricular study group at Yale; interest in economics; Henry Fellowship at University of Cambridge; concentration in theoretical physics; studies with Arthur Eddington.