Cosmological solution with matter in a new theory of gravitation

Details Cosmological solution with matter in a new theory of gravitation Cosmological solution with matter in a new theory of gravitation

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980cajph..58..729k&link_type=abstract

Canadian Journal of Physics, vol. 58, June 1980, p. 729-736. Research supported by the Natural Sciences and Engineering Researc

Physics

7

Big Bang Cosmology, Gravitation Theory, Matter (Physics), Background Radiation, Conservation Laws, Cosmic Dust, Curvature, Flux Density, Helium, Hermitian Polynomial, Stress Tensors, Temperature Dependence, Universe

Scientific paper

A plane-symmetric, homogeneous solution with matter in a theory of gravitation based on a non-symmetric Hermitian metric is presented. The solution describes a universe which begins with finite 4-curvature, energy density, and temperature. The initial temperature depends on a new parameter in the theory. An analysis of primordial helium abundance gives rise to a lower bound initial temperature greater than 10 to the 10th K. The resulting cosmology is consistent with all presently known observations.

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