Signatures of inhomogeneity in the early universe

Details Signatures of inhomogeneity in the early universe Signatures of inhomogeneity in the early universe

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...372....1k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 372, May 1, 1991, p. 1-7.

Astronomy and Astrophysics

Astrophysics

39

Evolution (Development), Nuclear Astrophysics, Nuclear Fusion, Universe, Astronomical Models, Carbon, Inhomogeneity, Nitrogen, Oxygen

Scientific paper

The production of elemental CNO in inhomogeneous nucleosynthesis is systematically studied for a much larger region of parameter space than ever before. The Li-7(n, gamma)Li-8(alpha, n)B-11 channel is shown to be the dominant path to CNO production in regions of parameter space in which there is significant CNO production. It is shown that this finding is a clear signal of an inhomogeneous Omega(b) = about 1 universe.

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