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In physical cosmology, the Alpher–Bethe–Gamow paper, or αβγ paper, was created by Ralph Alpher, then a physics PhD student, his advisor George Gamow, and Hans Bethe. The work, which would become the subject of Alpher's PhD dissertation, argued that the Big Bang would create hydrogen , helium and heavier elements in the correct ...
These results of Gamow and Alpher appeared in 1948 as the Alpher–Bethe–Gamow paper. [21] Before his interest turned to the question of the genetic code, Gamow published about twenty papers on cosmology. The earliest was in 1939 with Edward Teller on galaxy formation, [22] followed in 1946 by the first description of cosmic nucleosynthesis ...
It was created by George Gamow upon a suggestion by James Watson in 1954 [2] when the relationship between nucleic acids and amino acids in genetic information was unknown. The club consisted of 20 full members, each representing an amino acid, and four honorary members, representing the four nucleotides .
Coming across Gamow's paper, Crick immediately noticed some issues in the scheme. The first was that he and Watson never had before counted the 20 amino acids or the possible 20 nucleotide triplets [19] (although Gamow was subsequently proven to be correct and his model was the first prediction of the genetic code [17] [23]). The other issue ...
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The liquid-drop model was first proposed by George Gamow and further developed by Niels Bohr, John Archibald Wheeler and Lise Meitner. [3] It treats the nucleus as a drop of incompressible fluid of very high density, held together by the nuclear force (a residual effect of the strong force ), there is a similarity to the structure of a ...
The cosmic microwave background was first predicted in 1948 by Ralph Alpher and Robert Herman, in a correction [16] they prepared for a paper by Alpher's PhD advisor George Gamow. [17] Alpher and Herman were able to estimate the temperature of the cosmic microwave background to be 5 K. [18]
The Birth and Death of the Sun is a popular science book by theoretical physicist and cosmologist George Gamow, first published in 1940, exploring atomic chemistry, stellar evolution, and cosmology. [1] The book is illustrated by Gamow. It was revised in 1952.