Conditions for when the future-distribution inner-product space is a Hilbert space
Determine the necessary and sufficient conditions under which the space of future distributions G, defined as the linear span of functions g_{\bar{a}} representing conditional future distributions for a discrete-time, stationary stochastic process with a countable observation set, becomes a Hilbert space when endowed with the inner product induced by the L^2(\mu_\epsilon) embedding via densities \gamma(g) constructed through the Radon–Nikodym theorem.
References
The second objective is to investigate under what conditions the space of future distributions together with the inner product constructed in [unpub-tutorial] is a Hilbert space. This is an open question and answering it is the first step towards developing an approximation theory for OOMs via the two outlined pathways.