superposition diffuses to the environment such that a ‘variable’ (position in ordinary quantum theory, scale factor in gravity) emerges nearest in sense to the classical counterpart. The above discussion refers to any system that deals with quantum to classical transition. For systems whose dynamics are described by any of the three fundamental interactions (electromagnetic, weak and strong) other than gravity, we have a time parameter with three characteristics. In the above three interactions the ‘time’ i.e., the time of everyday reality is considered (i) classical, (ii) non-dynamical and (iii) being the same in all models. But in quantum gravity the situation is rather obscure. We have here two broad problems: problem of time and the emergence of time. In classical general relativity the condition (i) is satisfied, whereas the conditions (ii) and (iii) are not so because the time enters into the Einstein equations dynamically just like other three position co-ordinates and different geometries (we understand here as different models) evolve with different facets of time. Thus for a given manifold with a spacetime structure we observe time as if having many fingures - called ‘many fingured’ time. This is briefly the problem of time. The problem with the ‘emergence 