2012/02/01 by M. Farasat Shamir, Akhlaq Ahmad Bhatti · 1 citation
Physics and Astronomy · #Advanced Differential Geometry Research #Anisotropy #Black Holes and Theoretical Physics #Brans–Dicke theory #Classical mechanics #Cosmological constant #Cosmology #Cosmology and Gravitation Theories #Dark energy #Deceleration parameter #Gravitation #Mathematical physics #Metric expansion of space #Physics #Quantum mechanics #Scalar field #Scalar–tensor theory #Scale factor (cosmology) #Theoretical physics #Type (biology) #gr-qc
paper · pdf · doi:10.1139/p2012-007
published as Can. J. Phys. 90: 193-198, 2012 · 14 pages, accepted for publication in Canadian Journal of Physics. arXiv admin note: substantial text overlap with arXiv:0910.5787
openalex publication_date 2012/02/01 · arxiv created 2012/06/02 · arxiv updated 2017/08/23 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The main purpose of this paper is to explore the solutions of Bianchi type III cosmological model in Brans–Dicke theory of gravity in the background of anisotropic dark energy. We use the assumption of constant deceleration parameter and power law relation between scalar field [Formula: see text] and scale factor a to find the solutions. The physical behavior of the solutions has been discussed using some physical quantities.