Periodic Orbits of Quantised Restricted Three-Body Problem

In this paper, perturbed third-body motion is considered under quantum corrections to analyse the existence of periodic orbits. These orbits are studied through two approaches identify first (second) periodic-orbit types. The essential conditions given in order prove that circular (elliptical) rotating Kepler problem (RKP) can continue third body where a massive primary has excessive gravitational force over smaller body. primaries moved around each other orbits, and mass ratio was assumed be sufficiently small. We types by using terminologies Poincaré for quantised motion.