wavefunction of universe according to $$\Psi (G^{(3)},\Phi (x\in G^{(3)}))=\int{e^{iS(G^{(4)},\phi(x\in G^{(4)}))}\delta \phi\delta G}.$$ Here $G^{(4)}$ represents the four geometry and the fields $\phi$ defined on this four geometry are non-singular. There are some technical difficulties in choosing the complex paths in $a$-space in (23). However no unique prescription still has emerged. The question is to choose or find ‘allowable’ and ‘good’ paths, that contribute in (23). Finally, once one has calculated the wavefunction, it is still unclear how it resolves the problem of time, settles between the Copenhagen and Everettian approaches and interpret the timeless version of the Euclidean path integration. The wormhole dominance proposal provides a prescription for that in evaluating $\psi$ within the framework of complex semiclassical WKB approximation. A more technical discussion relating the complex paths and the evaluation of Euclidean path integral is reserved for concluding discussion in order to not track away from the main content of the paper. Let us try to understand the complex solutions considering (19) and (22). An important boundary condition is that both the initial and final value of $a$ must be real, keeping option open to include the complex paths in evaluating (23). Let us investigate the nature of the 