Recently the Lorentz gauge theory of gravity has been introduced as a candidate for a quantum gravity theory. In the Lorentz gauge theory of gravity, by using the tetrads and changing the way of variation, the metric becomes a non dynamical variable. In this theory, in addition to mass of particles, the spin of quantum particles also act as source in interactions. In order to show that this theory is consistent with existing experimental observations, it is important to obtain exact solutions for black holes. In this thesis, we will consider some of the metric solutions of black holes such as Schwarzschild, Cylindrical black hole with toroid horizon, all in d-dimensions and rotating BTZ black hole in three dimensions and Kerr black hole in four demensions. We have shown that these space-time as well as the de-Sitter space are exact solutions for this theory. We study the experimental test about precession of gyroscope spin by helping the Kerr metric in terms of the theory. We also investigate the spin interaction of the quantum particles with the gravitational field’s
