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Inflationary cosmology from STM theory of gravity

Mauricio Bellini
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Abstract

I study the power-law and de Sitter expansions for the universe during inflation from the STM theory of gravity. In a de Sitter expansion the additional dimension is related to the cosmological constant. I find from experimental data that the mass of the inflaton field is $m^2=2/(3Ψ^2)$. In power-law expansion, the fifth coordinate appears to be a dimensionless constant. The interesting here is that the $Ψ$-value depends on the initial conditions. I find the 5D line element for this inflationary expansion, which is a function of the classical component of the inflaton.

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Mauricio Bellini. 2003-08-15. Inflationary cosmology from STM theory of gravity. https://doi.org/10.1016/s0550-3213(03)00234-7

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