Abstract
Field equations of Saez and Ballester (Phys. Lett. A 113:467, 1986) scalar-tensor theory are obtained in the presence of two minimally interacting fields; matter and holographic dark energy components in spatially homogeneous and anisotropic LRS Bianchi type-II space-time. An exact solution of the field equations is presented using linearly varying deceleration parameter proposed by Akarsu and Dereli (Int. J. Theor. Phys. 51:612, 2012) which represents a minimally interacting Bianchi type-II universe in Saez-Ballester theory of gravitation. Some physical and kinematical properties of the model are also studied.
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Ramesh, G., Umadevi, S. LRS Bianchi type-II minimally interacting holographic dark energy model in Saez-Ballester theory of gravitation. Astrophys Space Sci 361, 50 (2016). https://doi.org/10.1007/s10509-015-2645-4
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DOI: https://doi.org/10.1007/s10509-015-2645-4