Constraining hybrid potential scalar field cosmological model in Lyra's geometry with recent observational data

In this study, we investigate a scalar field cosmological model with Lyra's geometry to explain the present cosmic expansion in a homogeneous and isotropic flat FRW universe. In Einstein's field equations, we presupposed a variable displacement vector as an element of Lyra's geometry. In the context of the conventional theory of gravity, we suggest a suitable parametrization of the scalar field's dark energy density in the hybrid function of redshift z, confirming the essential transition behavior of the universe from a decelerating era to the present accelerated scenario. We present constraints on model parameters using the most recent observational datasets from OHD, BAO/CMB and Pantheon, taking Markov Chain Monte Carlo (MCMC) analysis into account. For the proposed model, the best estimated values of parameters for the combined dataset (OHD, BAO/CMB and Pantheon) are H-0 = 71.15 +/- 0.26km/s/Mpc, Omega(m0) = 0.2625 +/- 0.0024, Omega(phi 0) = 0.676 +/- 0.038, alpha = -0.22 +/- 0.13, n = 0.096 +/- 0.079 and k = 0.38 +/- 0.32. The model exhibits a flipping nature, and the redshift transition occurs at z(t) = 0.756(-0.015)(+0.005). The current value of the decelerated parameter for the proposed model is calculated as q(0) = -0.625(-0.085)(+0.067) for the combined dataset. Some dynamical properties of the model like energy density (rho(phi)), scalar field pressure (p(phi)), EoS parameter of scalar field (omega(phi)), and effective EoS parameter (omega(eff)) are analyzed and presented. Further, we have also examined the statefinder diagnosis and jerk parameters of the derived model. The total density parameter for the derived model is found to be unity which is in nice agreement with recent standard findings.