On the gravitational instability in the Newtonian limit of MOG
arXiv:1704.04161 · doi:10.1016/j.physletb.2017.04.029
Abstract
We have found some analytical cosmological solutions to MOdified Gravity (MOG). These solutions describe different evolutionary epochs of an isotropic and homogeneous universe. During each epoch, the evolution of cosmological perturbation is studied in the Newtonian framework and compared with the corresponding results of GR.
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- Quasinormal Modes of Modified Gravity (MOG) Black Holes
- MOG cosmology without dark matter and the cosmological constant
- The Train Wreck Cluster Abell 520 and the Bullet Cluster 1E0657-558 in a Generalized Theory of Gravitation
- Effects of Scalar-Tensor-Vector Gravity on relativistic jets
- Stellar Bar evolution in the absence of dark matter halo
- Linear cosmological perturbations in Scalar-tensor-vector gravity
- Cosmology with Higher-Derivative Gravities
- The Weak Lensing Mass of Cosmic Web Filaments and Modified Gravity (MOG)