William Alfred Fowler

He got married to Adriane Foy Olmsted on 24 August 1940. The couple had two daughters, named, Mary and Martha.

William Alfred Fowler died on 14 March 1995 due to kidney failure in Pasadena, California, at the age of 83.

William Alfred Fowler was born in Pittsburgh in Pennsylvania, United States on 9 August 1911, to John Macleod Fowler and his wife Jenni Summers Watson Fowler. His father was employed in the capacity of an accountant. William had a younger brother and a younger sister.

He grew up in the city of Lima in Ohio since the family had moved following his father’s transfer. Initially, he studied at the Horace Mann Grade School and later on went on to graduate from Lima Central High School in 1929. In school, he showed an early interest in the sciences and engineering.

After graduating from high school, he took admission to the Ohio State University to study ceramic engineering. However, his interest in physics made him switch to engineering physics. Following his graduation from Ohio State University in 1933, he went to California Institute of Technology for his post graduate education. He received his doctorate in 1936 from the same institute in nuclear physics.

After attaining his doctorate from the California Institute of Technology, William Alfred Fowler was appointed as an assistant professor at the institute in 1939 and during that period he was engaged in in studying the nuclear reactions of the protons of carbon and nitrogen isotopes. The experiments commence following the discovery of CN cycle by Hans Bethe.

When the Second World War was in full swing, the Kellogg Laboratory at the California Institute of Technology was given away for defence research. In fact, in 1944, Fowler was sent to the South Pacific to assist the American forces and he stayed there in a non military capacity for three months. Two years later, he was appointed as a full professor by the California Institute of Technology.

He spent the better part of the 1950s in research related to experimental physics and one of his most celebrated work was the paper ‘Synthesis of the Elements in Stars’ which he co-authored with Fred Hoyle, Margaret Burbidge and Geoffrey Burbidge. The paper was published in the year 1957 and suggested that the process of synthesis of elements in stars starts from lighter elements.

Subsequently, he became the director of the Kellogg Laboratory at the California Institute of Technology. Other than his work on element generation, he was also involved in research related to the field of radio astronomy, with Fred Hoyle at the Institute of Theoretical Physics, established in 1966, at the University of Cambridge. He continued to work at Kellogg Laboratory simultaneously.

The most important work in his life as a scientist was achieved when he conducted a long drawn out study on nuclear reactions and elemental generation at the Kellogg Laboratory at the California Institute of Technology. His theories on elemental generation won him the Nobel Prize in 1983, which he shared with Subrahmanyan Chandrashekhar who had conducted an independent study on the same subject.

His most significant work was his theoretical and experimental studies of the nuclear reactions of importance in the formation of the chemical elements in the universe"..