Cosmic scenario of early universe in context of Euclidean wormhole in dilatonic Einstein–Gauss–Bonnet gravity

We present some wormhole configurations using analytic and numerical solutions of the Euclidean field equations considering Einstein Gauss Bonnet dilaton coupled interaction in Robertson Walker metric. Analytic invoking slow-roll type approximation for potentials yield identical wormholes early era. Eventually, a later era, universe enters to an expanding era much faster than usual inflation accompanied by oscillations with continuation \tau=it. The terms scale factor a(\tau) are almost standard field, except evolution potentials. Hubble parameter deceleration obtained curve fit solution inflationary away from throat A sharp decay potential is also observed.