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A diagram, produced by NASA and the WMAP Science Team, showing a posited history of the cosmos: shortly after the Big Bang (marked “dawn of time”), the universe was made up of ylem(first oval shape). Recombination of the ylem into neutral atoms 380,000 years after the Big Bang entailed the release of radiation (photons) forming the cosmic microwave background(second oval shape), recorded by the WMAP satellite. The last oval shape shows the universe as it exists today.An all-sky image of the cosmic microwave background, based on nine years' worth of data gathered by WMAP, representing the universe at the time of the phase transition of ylem to atomic matter. The colour differences in the image represent temperaturefluctuations corresponding to the ‘seeds’ that grew into galaxies.
The term ylem was first used in modern English in the paper “The Origin of Chemical Elements”, coauthored by Russian-American theoreticalphysicist and cosmologistGeorge Gamow (1904–1968), American cosmologist Ralph Asher Alpher (1921–2007) and German-American nuclear physicist Hans Bethe (1906–2005), published 1 April 1948 in Physical Review. Alpher claimed to have found the word “in a large dictionary”, perhaps Webster’s New International Dictionary (2nd ed., 1934), which he referred to in a second 1948 paper (cited below). In a 1968 interview, Gamow also associated ylem with a Hebrew word he did not name; it remains unclear which word he was referring to.
The word ylem reappeared in popular books on science following the discovery in 1964–1965 of the cosmic microwave background, which had been predicted in 1948 by Alpher and Robert Herman (1914–1997), and again after the publication of images of the radiation composed from measurements by two satellites, the Cosmic Background Explorer (COBE) in 1992 and the Wilkinson Microwave Anisotropy Probe (WMAP) in 2003.
Let us now consider the state of matter during the first minutes of the expansion process, when the temperature of the universe was many billions of degrees high. he state of matter must be visualized as a hot gas formed entirely by nuclear particles; that is, protons, neutrons, and electrons. We will call this primordial mixture of nuclear particles "Ylem," reviving an obsolete noun which, according to Webster's Dictionary, means "the first substance from which the elements were supposed to be formed." Next we can ask what happened to the Ylem when its density and temperature began to drop as the result of the rapid expansion taking place in the young universe.
He surmised that that the universe began as a super-condensed raging inferno of protons, neutrons and electrons, which he and his colleagues called the ylem The internal pressures of the ylem caused it to expand outward extremely rapidly. After a few minutes the ylem cooled down sufficiently to allow the strong force to bind neutrons and protons together into deuterium nuclei. Then there was just enough time for some of the deuterium to fuse into helium before temperatures and pressures of the ylem became too diffuse to allow more fusions.
^ George Gamow, Charles Weiner, interviewer (1968 April 25) “Oral Histories: George Gamow”, in Niels Bohr Library & Archives, American Institute of Physics, archived from the original on 2 June 2016:
Gamow: You can look in the Webster dictionary. This is a word—I think it’s an old Hebrew word, but Aristotle was using it—in Webster dictionary it says “material from which elements were formed.” / Weiner: The primordial substance? / Gamow: The primordial substance, yes—ylem. I mean this is the old Hebrew word meaning something like “space between heaven and earth.”
^ R A Alpher, R C. Herman (1948 December 15) “On the Relative Abundance of the Elements”, in Physical Review, volume 74, number 12, College Park, Md.: American Physical Society, →DOI, →OCLC, pages 1737–1742.