Black-hole nucleosynthesis and Omega(B) = 1

Details Black-hole nucleosynthesis and Omega(B) = 1 Black-hole nucleosynthesis and Omega(B) = 1

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvl..65.2225c&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 65, Oct. 29, 1990, p. 2225-2228. Research supported by the Miller Foundation for

Astronomy and Astrophysics

Astrophysics

8

Big Bang Cosmology, Black Holes (Astronomy), Nuclear Astrophysics, Nuclear Fusion, Abundance, Baryons, Computerized Simulation, Hadrons

Scientific paper

Black holes may be produced from false-vacuum bubble implosions at the end of the QCD phase transition. Evaporation of these black holes during the keV era readjusts the abundances of light nuclei. An appropriate mass distribution of black holes gives nuclear abundances broadly consistent with observations even for Omega(B) = 1, reconciling a critical baryonic universe with standard-model particle physics.

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