Dynamical and static solutions to $R=0$-scalar-tensor theory. (arXiv:2007.11023v1 [gr-qc])
<a href="http://arxiv.org/find/gr-qc/1/au:+Azreg_Ainou_M/0/1/0/all/0/1">Mustapha Azreg-Aïnou</a>
We consider the most cosmologically interesting and relevant case of
scalar-tensor theory (STT) and derive new normal and phantom, dynamical and
static, solutions. We determine the Bianchi I Kasner exponents and show that
the dynamical solutions are heteroclinic orbits connecting two singularities.
Approaching the singularities, a purely transverse expansion (no radial
expansion or collapse) may occur.
We consider the most cosmologically interesting and relevant case of
scalar-tensor theory (STT) and derive new normal and phantom, dynamical and
static, solutions. We determine the Bianchi I Kasner exponents and show that
the dynamical solutions are heteroclinic orbits connecting two singularities.
Approaching the singularities, a purely transverse expansion (no radial
expansion or collapse) may occur.
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