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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.
Early years in Vienna; emigration to Sydney, Australia as refugee; training there in theoretical physics, to 1946. Quantum field theory and social interactions under Rudolf Peierls at University of Birmingham, to 1949, and Hans Bethe at Cornell University; relations among U.S. field theorists; nuclear theory applied to experiments. Discovery of triple-alpha process at Caltech, 1951; move into astrophysics and social relations in Cornell physics and astronomy departments. Work on increasing variety of astrophysics problems, some related to cosmology, and on ionosphere; Arecibo observatory.