A documentary about George Gamow's Life is now available on Youtube.
|1904||Born, March 4, Odessa, Russia|
|In his school days Gamow became very much interested in astronomy, examining the starry sky through a little telescope, his father's present on the thirteenth birthday of his son. Gamow then decided to become a scientist and began his study of mathematics, physics, and astronomy.|
|1922||-1923||Student at Novorossia University, Odessa|
|1923||-1929||Student at University of Leningrad|
|After graduation from the University of Leningrad in 1926, he attended summer school in Gottingen and decided to see if the newly-formulated quantum theory, so successful in explaining the structure of the atom, could also be applied to the atomic nucleus. Through research he was able to explain the then-mysterious phenomenon of natural radioactivity as well as the experiments of Lord Rutherford on the induced transformation of light elements. On the basis of this research, Gamow received his Ph.D. degree from the University of Leningrad.|
|1928||-1929||Fellow of Theoretical Physics Institute of the University of Copenhagen|
Later, in Copenhagen, when he told Niels Bohr of his work, Bohr offered him a year at the Institute of Theoretical Physics on a stipend from the Royal Danish Academy. There Gamow proposed a hypothesis that atomic nuclei can be treated as little droplets of so-called "nuclear fluid." These views led ultimately to the present theory of nuclear fission and fusion.
At this period Gamow also collaborated with F. Houtermans and R. Atkinson in attempts to apply his formula for calculating the rate of induced nuclear transformations to the so-called thermonuclear reaction in the interior of the Sun and other stars. This formula, originally applied only to astronomical topics, is now successfully used for designing H-bombs, as well as for studying the possibility of controlled thermonuclear reactions.
|1929||-1930||Rockefeller Fellow, Cambridge University|
|1930||-1931||Fellow of Theoretical Physics Institute of the University of Copenhagen|
|1931||Married Lyubov Vokhminzeva; divorced 1956|
|1931||-1933||Professor, University of Leningrad|
|Gamow spent a year working with Lord Rutherford at Cambridge, a second year in Copenhagen, and later became a professor at the University of Leningrad.|
|1933||-1934||Fellow of Pierre Curie Institute, Paris
Visiting Professor, University of London
|1934||Lecturer, University of Michigan|
|While attending the International Solvay Congress in Brussels, he was invited, in the summer of 1934, to lecture at the University of Michigan.|
|1934||-1956||Professor, George Washington University, Washington, D.C.|
During the early years in Washington he collaboratedwith Edward Teller on the theory of beta-decay, and formulated the so-called "Gamow-Teller Selection Rule for Beta Emission."
While Gamow was in Washington he developed the theory of the internal structure of red giant stars. With Mario Schoenberg he developed the theory of the so-called Urca process; and, with Ralph Alpher, the theory of the origin of chemical elements by the process of successive neutron capture.
|1935||Son, Rustem Igor, born|
|1954||Visiting Professor, University of California, Berkeley|
|In 1954 Gamow developed an interest in biological phenomena and published papers on the information storage and transfer in a living cell. In these papers he proposed the so-called "genetic code," an idea later completely confirmed by experimental studies in laboratories.|
|1956||-1968||Professor, University Of Colorado|
|1956||Awarded Kalinga Prize by UNESCO for popularization of science|
|1958||Married Barbara Perkins ("Perky")|
|1965||Overseas Fellow, Churchill College, Cambridge University|
|1968||George Gamow Passed Away at Age 64|
|The George Gamow Memorial Lectures were initiated by the Department of Physics and Mrs. Barbara Gamow after the death of her husband. The lecture series began in 1971 and is now maintained by a bequest to the Regents of the University of Colorado from the Will of Mrs. Barbara Gamow, who died in December 1975.|
George Gamow's fame as a physicist began with his theory that explained the radioactive alpha particle decay of atomic nuclei. In his cosmological studies, he is known for the "big bang" theory of the origin of the universe, and in 1954 his studies in biology led him to suggest that the genetic code was a triplet code. This concept is fundamental to modern biology. He was perhaps most widely known for his popular writings on science that introduced millions of readers to the concepts of relativity and atomic and nuclear physics. These writings have been translated into several dozen languages. In recognition of the global impact of his popular scientific writings, the United National awarded him with the Kalinga Prize in 1956.
|1928||Explained nuclear alpha decay by quantum mechanical tunneling;|
|1928||Pioneered the liquid-drop model in nuclear physics;|
|1936||Described, with Edward Teller, spin-induced nuclear beta decay;|
|1938||Introduced the "Gamow" factor in stellar reaction rates and element formation;|
|1939||Modeled red giants, supernovae, and neutron stars;|
|1954||First suggested how the genetic code might be transcribed;|
|Wrote the popular science fiction series, the "Adventures of Mr. Tompkins"
(most recently reprinted in 2001).
"It was a bank holiday, and Mr. Tompkins, the little clerk of a big city bank, slept late and had a leisurely breakfast. Trying to plan his day, he first thought about going to some afternoon movie and, opening the morning paper, turned to the entertainment page. But none of the films looked attractive to him. He detested all this Hollywood stuff, with infinite romances between popular stars.
"If only there were at least one film with some real adventure, something unusual and maybe even fantastic about it. But there was none. Unexpectedly, his eye fell on a little notice in the corner of the page. The local university was announcing a series of lectures on the problems of modern physics, and this afternoon's lecture was to be about Einstein's Theory of Relativity. Well, that might be something!"
So begins the first chapter of "Mr. Tompkins in Wonderland."
George Gamow was perhaps most widely known for his popular writings on science that introduced millions of readers to concepts of relativity and atomic and nuclear physics. These writings have been translated into several dozen languages. In recognition of the global impact of his popular scientific writings, he was awarded the Kalinga Prize by the United Nations in 1956.
The Mr. Tompkins Series
|1939||Mr. Tompkins in Wonderland|
|1944||Mr. Tompkins Explores the Atom|
|1953||Mr. Tompkins Learns the Facts of Life|
|1967||Mr. Tompkins Inside Himself|
Other Popular Writing
|1940||The Birth and Death of the Sun|
|1941||Biography of the Earth|
|1947||One, Two, Three. . . Infinity: Facts and Speculations of Science|
|1961||Biography of Physics|
|1963||A Planet Called Earth|
|1964||A Star Called the Sun|
|1966||Thirty Years that Shook Physics: The Story of Quantum Theory|
Science Text Books
|1931||The Constitution of Atomic Nuclei and Radioactivity|
|1937||Structure of Atomic Nuclei and Nuclear Transformations|
|1947||Atomic Energy in Cosmic and Human Life|
|1949||Theory of Atomic Nucleus and Nuclear Energy Sources, with C.L. Critchfield|
|1952||The Creation of the Universe|
|1958||Matter, Earth & Sky, with John M. Cleveland|
|1960||Physics: Foundations & Frontiers|
|1961||The Atom and its Nucleus|