Matter, Antimatter, and the Origin of Galaxies

Details Matter, Antimatter, and the Origin of Galaxies Matter, Antimatter, and the Origin of Galaxies

Jun 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967phrvl..18.1011h&link_type=abstract

Physical Review Letters, vol. 18, Issue 23, pp. 1011-1013

Physics

59

Scientific paper

Baryon inhomogeneities in the early high-density universe may account for the origin of galaxies. Any such inhomogeneity is amplified by baryon-pair annihilation as the universe expands and can eventually result in the formation of galaxies and antigalaxies. This process is more efficient than the usual process which assumes that the initial conditions of a structured universe are density fluctuations.

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