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arXiv · 1201.0271

$γ$ Parameter and Solar System constraint in Chameleon Brans Dick Theory

Khaled Saaidi·Abolhassan Mohammadi·Haidar Sheikhahmadi
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Abstract

The post Newtonian parameter is considered in the Chameleon-Brans-Dicke frame. In the first step, the general form of this parameter and also effective gravitational constant is obtained. An arbitrary function for $f(Φ)$, which indicates the coupling between matter and scalar field, is introduced to investigate validity of solar system constraint. It is shown that Chameleon-Brans-Dicke model can satisfy the solar system constraint and gives us an $ω$ parameter of order $10^4$, which is in comparable to the constraint which has been indicated in {\cite{17-a}}.

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Khaled Saaidi, Abolhassan Mohammadi, Haidar Sheikhahmadi. 2011-12-31. $γ$ Parameter and Solar System constraint in Chameleon Brans Dick Theory. https://doi.org/10.1103/physrevd.83.104019

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