Tidal effect on the gyroscopic precession around a compact star

General relativistic effects around massive astrophysical objects can be captured using a test gyro orbiting the object in circular geodesic. This paper discusses how tidal field due to companion affects spin precession frequency and orbital angular velocity of spinning compact object. The is studied region space central perturbative approach. either neutron star or white dwarf this study. any planetary asteroid-like dwarf. Moreover, that causes star, stellar black hole. It seen effect significantly spacetime object, which velocity. Slow rotation approximation has been considered for creates negligible deformation. change gyro’s increases with an increase object’s mass decreases as separation between increases. also varies stiffness equation state matter describing host star. lower compactness greater response; thus