Damghan University Press Iranian Journal of Astronomy and Astrophysics 2322-4924 8 2 2021 07 01 Bianchi I Cosmology and Scalar Vector Tensor Brans Dicke Gravity 91 121 266 10.22128/ijaa.2021.520.1116 EN Hossein Ghaffarnejad Faculty of Physics, Semnan Universiy, Semnan, Iran, 35131-19111 0000-0002-0438-6452 Hoda Gholipour Semnan university Journal Article 2022 03 22 We consider Brans Dicke scalar vector tensor gravity to study an inflationary scenario of the accelerating expansion of the<br />universe for which the anisotropy property occurs. We study both primordial inflation and late inflationary period of the universe.<br />To do so we use Bianchi I line element where spatial part has cylindrical symmetry along $x$ direction in the local Cartesian coordinates. To seek stabilization of our obtained metric solution we apply dynamical system approach to obtain critical manifolds in phase space and determine which of them confirms the inflation with stable nature in presence of the anisotropy property of spacetime. We solve dynamical equations for different directions of the timelike dynamical vector field. We obtain several critical manifolds whose nature of stable (sink) or quasi stable (saddle) are dependent to direction of the used vector field. At last we should point that observational constraint on the Brans Dicke parameter ω>40000 which satisfied by the well known Brans Dicke scalar tensor gravity is not valid for our modified scalar vector Brans Dicke gravity because of presence of timelike dynamical vector field. https://ijaa.du.ac.ir/article_266_11c993fd049eec71df2eb523318a77ac.pdf