collaborators

6 papers

gr-qc2003

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

Luis Augusto Trevisan

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…

gr-qc2001

Amplification of Gravitational Waves During Inflation in Brans-Dicke Theory

Marcelo S. Berman, Luis A. Trevisan

We show that Gravitational Waves are exponetially amplified in the inflationary phase in Brans-Dicke theory, so that it would be possible to detect them and in this way verify seve…

gr-qc2001

Possible Cosmological Implications of Time Varying Fine Structure Constant

Marcelo S. Berman, Luis A. Trevisan

We make use of Dirac LNH and results for a time varying fine structure constant in order to derive possible laws of variation for speed of light, the number of nucleons in the Univ…

gr-qc2001

Static Generalized Brans-Dicke Universe and Gravitational Waves Amplification

Marcelo S. Berman, Luis A. Trevisan

We find a static solution for the scale-factor in a Brans-Dicke generalized theory where the scalar field and the coupling constant vary with time. We find also that in the early U…

gr-qc2001

On a time varying fine structure constant

Marcelo S. Berman, Luis A. Trevisan

By employing Dirac LNH, and a further generalization by Berman (GLNH), we estimate how should vary the total number of nucleons, the energy density, Newton Gravitational constant,…

gr-qc2001

Estimate on the deceleration parameter in a Universe with variable fine structure constant

Marcelo S. Berman, Luis A. Trevisan

We determine a cosmological model that include a positive acceleration of the Universe and a time decreasing fine structure constant. The present day deceleration parameter is esti…