“…One advantage of that step is that we can define S(t) by an explicit formula that depends on the coefficients of the operator H. Another advantage is that for each t the operator S(t) is a linear bounded operator, which allows us to define analytic functions of argument S(t) via power series (see examples [40,39,37,41,36]) to obtain a semigroup e −itH t≥0 that solves Schrödinger equation with Hamiltonian H. This idea was introduced in [40] where we defined R(t) = exp − i(S(t) − I) and proved that e −itH = lim n→∞ R(t/n) n . Members of O.G.Smolyanov's group employed Chernoff's theorem using integral operators as Chernoff functions to find solutions to parabolic equations in many cases during the last 15 years: see the pioneering papers [46,45], overview [44], several examples [43,11,38,16,47,42,12] to see the diversity of applications, and recent papers [39,13,41,9,5,29,8,36,27,22,24,48,21,7,35]. The solutions obtained were represented in the form of a Feynman formula, i.e.…”