作者: M. Mousavi , F. Darabi
DOI: 10.1088/1475-7516/2015/08/009
关键词: Mathematical physics 、 Kinetic energy 、 Tensor 、 Equations of motion 、 Einstein 、 Perturbation (astronomy) 、 Physics 、 Classical mechanics 、 Scalar field 、 Cosmology 、 Tensor contraction
摘要: We generalize the scalar tensor bigravity models to non-minimal kinetic coupling with two fields whose terms are non-minimally coupled Einstein tensors constructed by metrics. show that a broad class of expanding universes can be explained some solutions this model. Then, we study stability issue means imposing homogeneous perturbation on equations motion and extract stable solutions.