

German-American nuclear physicist
German Reich
Pleasant Grove Cemetery
Hans Bethe (born 2 July 1906 in Strasbourg; died 6 March 2005 in Ithaca, New York) was a German-American theoretical physicist. He worked in nuclear physics, astrophysics, quantum physics and solid-state physics. In 1967 he received the Nobel Prize in Physics for his contributions to the theory of nuclear reactions, especially for explaining energy production in stars.
Bethe studied in Frankfurt and Munich and earned his doctorate at the University of Munich. Arnold Sommerfeld was among his formative scientific teachers. After posts in Europe, Bethe lost his academic future in Nazi Germany in 1933; his mother was of Jewish background. He first went to Britain and in 1935 came to Cornell University in Ithaca. Cornell remained his scientific home for decades.
In the 1930s Bethe became one of the leading experts in nuclear physics. His review articles helped organize the young field. In 1939 his paper Energy Production in Stars appeared. In it he described nuclear reactions through which stars can release energy over long periods of time. This research connected nuclear physics and astronomy and became a foundation of nuclear astrophysics.
During the Second World War Bethe worked on the Manhattan Project. At Los Alamos he led the Theoretical Division and took part in calculations important to the development of the first atomic bombs. After the war, the military use of physics remained a recurring subject of his public work. Bethe spoke about arms control, nuclear risk and the responsibility of scientists in political decisions.
After the war Bethe returned to Cornell. He continued to work in theoretical physics, including quantum electrodynamics, nuclear processes and later astrophysical questions. On 10 December 1967 he received the Nobel Prize in Physics in Stockholm. Even after retirement he remained scientifically active and spoke publicly on nuclear security issues, including missile defense policy in the 1980s.
Hans Bethe died in Ithaca on 6 March 2005. His biography connects basic research with one of the most consequential technical developments of the twentieth century. His scientific work explained how stars produce energy; his later public work shows how deeply the political consequences of modern physics occupied him.
until 1926
until 1928
until 1930
until 1931
until 1933
until 1975