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Berman M.S.,Instituto Albert Einstein Latinamerica
Astrophysics and Space Science | Year: 2011

We consider a General Relativistic RW's metric, with variable speed of light, and find a field of Universal acceleration, numerically coincident with the value of the Pioneers anomalous one. This deceleration may decrease with time, as we calculated. This is relevant to understand the Physics that may be involved in the Cosmological approach to the Pioneers anomaly. © 2011 Springer Science+Business Media B.V. Source


Berman M.S.,Instituto Albert Einstein Latinamerica
Astrophysics and Space Science | Year: 2012

In a previous paper (Berman, in Astrophys. Space Sci., 2011), we showed how to prove the two Pioneers Anomalies, and now we add the fly-bys, by means of a rotating Universe. We discuss Einstein's Machian program, which we find as being fullfilled. Godlowski et al. (Los Alamos Archives, 2003) idea for a rotating General Relativistic Universe, led us to the adopted model. Updated evidence on rotation is cited (Godlowski, in Los Alamos Archives, 2011; Ni in Phys. Rev. Lett. 107(5):051103, 2011). We conclude that a rotating and expanding Universe may be the unique solution to the apparent divergences between Einstein and Mach. This is cosmologically important. © 2011 Springer Science+Business Media B.V. Source


Berman M.S.,Instituto Albert Einstein Latinamerica
Astrophysics and Space Science | Year: 2011

We show how to prove the two Pioneers Anomalies by means of the Godlowski et al. (arXiv:astro-ph/0404329, 2004) idea for a rotating General Relativistic Universe. The so-called clock effect is calculated. © 2011 Springer Science+Business Media B.V. Source


Berman M.S.,Instituto Albert Einstein Latinamerica
Astrophysics and Space Science | Year: 2010

After reviewing the scalar-tensor lambda-accelerating power-law solutions by Berman (Astrophys. Space Sci. 323:103, 2009a), we obtain solutions for the amplification of gravitational waves in the models. The solutions consider a perfect gas equation of state, with cosmic pressure proportional to the energy density, the proportionality constant being smaller than -2/3. © Springer Science+Business Media B.V. 2009. Source


Berman M.S.,Instituto Albert Einstein Latinamerica
International Journal of Theoretical Physics | Year: 2010

After reviewing the scalar-tensor inflationary solutions by Berman and Trevisan (Int. J. Theor. Phys. 29, 1411-1414, 2009), we obtain solutions for the amplification of gravitational waves in the models. The solutions consider a perfect gas equation of state, with cosmic pressure proportional to the energy density, the proportionality constant being smaller than -2/3, and a cosmological term. © Springer Science+Business Media, LLC 2009. Source

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