arXiv · 1711.05426
Cosmological Constant in Chameleon Brans-Dicke Theory
Abstract
We consider a generalized Brans-Dicke model in which the scalar field has a self-interacting potential function. The scalar field is also allowed to couple non-minimally with the matter part. We assume that it has a chameleon behavior in the sense that it acquires a density-dependent effective mass. We consider two different types of matter systems which couple with the chameleon, dust and vacuum. In the first case, we find a set of exact solutions when the potential has an exponential form. In the second case, we find a power-law exact solution for the scale factor. In this case, we will show that the vacuum density decays during expansion due to coupling with the chameleon.
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Yousef Bisabr. 2018-03-21. Cosmological Constant in Chameleon Brans-Dicke Theory. https://doi.org/10.1142/s0218271819500226
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