Helium formation in a Bianchi type V cosmological model with tilt

Details Helium formation in a Bianchi type V cosmological model with tilt Helium formation in a Bianchi type V cosmological model with tilt

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984cqgra...1..407m&link_type=abstract

Classical and Quantum Gravity (ISSN 0264-9381), vol. 1, July 11, 1984, p. 407-415.

Mathematics

Logic

12

Abundance, Astronomical Models, Cosmology, Helium, Nuclear Fusion, Cauchy Problem, Deuterium, Neutron Distribution

Scientific paper

A formalism is developed for studying the evolution of Bianchi type V
cosmological models with tilt and a Cauchy horizon. Results are
presented on neutron fractions, predicted helium and deuterium
abundances and the effect of varying the photon to baryon ratio, in some
models. The constraint on the shear/expansion ratio is discussed.

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