Helium formation in a Bianchi type V cosmological model with tilt
- 11 July 1984
- journal article
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 1 (4) , 407-415
- https://doi.org/10.1088/0264-9381/1/4/014
Abstract
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.Keywords
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