Abstract
In the present study, we investigate the Bianchi type III cosmological model in the context of Brans–Dicke (BD) theory of gravitation. We assume viscous holographic dark energy as a matter source. Exact solutions of the field equations are obtained. Two different models based on parameter \(m\) are investigated. It is observed that the viscosity and BD coupling constant have a measurable effect on dynamical quantities. Some physical parameters are also discussed.
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Hatkar, S.P., Wadale, C.D. & Katore, S.D. Viscous holographic dark energy in Brans–Dicke theory of gravitation. Astrophys Space Sci 365, 7 (2020). https://doi.org/10.1007/s10509-020-3723-9
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DOI: https://doi.org/10.1007/s10509-020-3723-9