Bianchi type-VIo Holographic Dark Energy Cosmological Model in Brans-Dicke Theory of Gravitation

In this paper, we derive Brans-Dicke (Phys.Rev. 124 ; 925,1961) field equations in Bianchi type-VI 0 space time in the presence of minimally interacting fields; matter and holographic dark energy components. A determinate solution of the field equations is obtained using some physically plausible conditions. This solution represents an anistropic holographic dark energy model in Brans-Dicke theory of gravitation. Physical and kinematical parameters of the model are computed and physical aspects of the model are discussed.