Stability analysis and Observational Measurement in Chameleonic Generalised Brans--Dicke Cosmology

We investigate the dynamics of the chameleonic Generalised Brans–Dicke model in flat FRW cosmology. In a new approach, a framework to study stability and attractor solutions in the phase space is developed for the model by simultaneously best fitting the stability and model parameters with the observational data. The results show that for an accelerating universe the phantom crossing does not occur in the past and near future.