Bondi lectured in mathematics in the University of Cambridge from 1945 to 1954. He was a fellow of Trinity College from 1943 to 1949 and from 1952 to 1954. In 1948, Hermann Bondi,
Fred Hoyle and
Thomas Gold formulated the
Steady State theory, which holds that the universe is constantly expanding but matter is constantly created to form new stars and galaxies to maintain a constant average density. Steady State theory was eclipsed by the rival Big Bang theory with the discovery of the
cosmic microwave background (CMB). Bondi was one of the first to correctly appreciate the nature of
gravitational radiation, introducing Bondi radiation coordinates, the
Bondi k-calculus, the notions of
Bondi mass and
Bondi news, and writing review articles. He popularized the
sticky bead argument which was said to be originally due, anonymously, to
Richard Feynman, for the claim that physically meaningful gravitational radiation is indeed predicted by general relativity, an assertion which was controversial up until about 1955. A 1947 paper revived interest in the
Lemaître–Tolman metric, He was secretary of the
Royal Astronomical Society from 1956 to 1964. == Other work ==