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2003•arXiv (Cornell University)Open access

A numerical analysis for G(t) in a scalar tensor theory

Luis A. Trevisan

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Abstract

We calculated the evolution of the Newton gravitational in a scalar tensor theory, using parameters that holds for the present Universe. We analised the evolution from one billion of years ago.

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We calculated the evolution of the Newton gravitational in a scalar tensor theory, using parameters that holds for the present Universe. We analised the evolution from one billion of years ago.

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Available abstract

We calculated the evolution of the Newton gravitational in a scalar tensor theory, using parameters that holds for the present Universe. We analised the evolution from one billion of years ago.

Key concepts: Scalar (mathematics), Mathematical physics, Tensor (intrinsic definition), Scalar–tensor theory, Mathematics, Physics, Pure mathematics, Geometry

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