“…Upon setting c 2 = 0, c 1 = 1/R 0 and expanding around χ = 0 we obtain V (χ) = 1/(R 0 χ), that is V (r) = 1/r, which is of course the Newtonian potential in flat space R 3 . The cosmological constant is represented quantum-mechanically as an operator that, in flat space, is proportional to the inverse of the squared radial distance ρ [7]. In R 3 , the standard choice is of course the centrifugal potential energy,…”