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George Gamow

George Gamow, born Gyorgy Antonovich Gamow (March 4, 1904 - August 19, 1968) was a Ukrainian born physicist and cosmologist. He worked on subjects including the atomic nucleus, star formation, stellar nucleosynthesis, nucleocosmogenesis[?], and genetics.

Gamow was born in Odessa, Russia, now Ukraine. He was educated at the Novorossia University in Odessa (1922-23) and at the University of Leningrad (1923-1929). On graduation he studied quantum theory in Göttingen, where his research into the atomic nucleus provided the basis for his doctorate. He then worked at the Theoretical Physics Institute of the University of Copenhagen, from 1928 to 1931 with a break to work with Ernest Rutherford at the Cavendish Laboratory, Cambridge, he continued to study the atomic nucleus (proposing the "liquid drop" model) but also worked on stellar physics with Robert Atkinson[?] and Fritz Houtermans.

Gamow then worked at a number of establishments before fleeing the increased oppression in Russia and settling at George Washington University[?] in 1934, where he published with Edward Teller, Mario Schoenberg[?] and Ralph Alpher[?]

The cosmogenesis[?] paper with Alpher was published as the Alpher-Bethe-Gamow theory, Gamow had added the name of Hans Bethe to make a pun on the first three letters of the Greek alphabet, alpha beta gamma.

Gamow was a strong advocate of the Big Bang theory. He remained in Washington until 1954, then working at University of California, Berkeley (1954), University of Colorado (1956-1968). In 1956 he was awarded the Kalinga prize[?] by UNESCO for his work in popularizing science with his Mr. Tompkins... series of books (1939-1967), One Two Three ... Infinity, and other works.

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