A Modified Holographic Ricci Dark Energy Model in a Lyra Manifold &Bianchi Type-V Spacetime

The main motive of this investigation is to study the behavior of cosmological model in the presence of matter and a modified holographic Ricci dark energy in the anisotropic Bianchi type-V space time. We have used a modified theory of gravitation formulated in the frame work of Lyra (Math.Z.54, 52: 1951 ) manifold for this purpose. Modified field equations of this theory are solved using physically viable conditions to obtain a deterministic cosmological model. Using this model the dynamical cosmological parameters have been computed and their detailed physical discussion is presented.