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Gamow, George
(redirected from Gamow)

   Also found in: Dictionary/thesaurus, Acronyms, Wikipedia, Hutchinson 0.04 sec.
Gamow, George (găm`ŏf), 1904–68, Russian-American theoretical physicist and author, b. Odessa. A nuclear physicist, Gamow is better known to the public for his excellent books popularizing abstract physical theories. He did his earlier research at the Univ. of Copenhagen, Cambridge Univ., and the Univ. of Leningrad, where he was professor (1931–33). He then came to the United States, where he taught at George Washington Univ. (1934–56) and the Univ. of Colorado (from 1956) and served with U.S. government agencies. He formulated (1928) a theory of radioactive decay and worked on the application of nuclear physics to problems of stellar evolution. He was one of the first proponents of the "big bang" theory of cosmology cosmology, area of science that aims at a comprehensive theory of the structure and evolution of the entire physical universe .

Modern Cosmological Theories


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. In 1954 he proposed an important theory concerning the organization of genetic information in the living cell. His writings include Constitution of Atomic Nuclei (1931; 3d ed., with C. L. Critchfield, Theory of Atomic Nucleus, 1949), Mr. Tompkins in Wonderland (1939), One, Two, Three … Infinity (1947, rev. ed. 1961), The Creation of the Universe (1952, rev. ed. 1961), Mr. Tompkins Learns the Facts of Life (1953), The Atom and Its Nucleus (1961), and Gravity (1962).

Bibliography

See his autobiography, My World Line (1970).


Gamow, George

 orig. Georgy Antonovich Gamov

(born March 4, 1904, Odessa, Russian Empire—died Aug. 19, 1968, Boulder, Colo., U.S.) Russian-born U.S. nuclear physicist and cosmologist. After studying at Leningrad University with Aleksandr Friedmann (1888–1925), he subsequently developed his quantum theory of radioactivity, the first successful explanation of the behaviour of radioactive elements. His “liquid drop” model of atomic nuclei served as the basis for modern theories of nuclear fission and fusion. After immigrating to the U.S. in 1934, he collaborated with Edward Teller in researching beta decay (1936) and developing a theory of the internal structures of red giant stars (1942). In the 1950s he became interested in biochemistry, proposing theories of genetic code structure that were later found to be true. Throughout his career he also wrote popular works on such difficult subjects as relativity and cosmology.


Gamow, George (1904–68) physicist; born in Odessa, Russia. His European research on radioactivity and atomic fission gained him an international reputation that preceded his arrival at George Washington University (1934–56). He and Edward Teller formulated their rule for beta decay in 1936. He postulated that primordial matter existed prior to the origin of the universe (1948), he developed the theory of red giant stars, and he was a major proponent of the "big bang" theory of the origin of the universe. He correctly theorized that DNA structure forms a code that directs protein synthesis. He became a professor at Colorado (1956–68), where he wrote and illustrated most of his many books for nonscientists.


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These years were marked by frequent contact and collaboration with other great physicists who had emigrated from Europe to escape Hitler and the coming war, including Fermi, Bohr, Szilard, Wigner, George Gamow and Hans Bethe.
Stories of his encounters and work with some of the leading scientists of the 20th century include Linus Pauling, Richard Feynman, and especially George Gamow, the Russian physicist with whom Watson founded the legendary RNA-Tie Club.
and building on the ideas of George Gamow - offered an elaboration of some of the Big Bang ideas that had been around since well before 1920.
 
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