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

dc.creatorTrevisan, Luis Augusto
dc.date2003-02-03
dc.date2003-02-04
dc.date.accessioned2026-07-07T03:27:36Z
dc.date.available2026-07-07T03:27:36Z
dc.descriptionWe 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.
dc.descriptionThe 4 figures (ps files) were included
dc.identifierhttps://arxiv.org/abs/gr-qc/0302002
dc.identifierhttp://arxiv.org/abs/gr-qc/0302002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34493
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA numerical analysis for G(t) in a scalar tensor theory
dc.typetext

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