Abstract
Within the framework of Relativistic Quantum Geometry, we explore a physical scenario involving the interaction of a gravitational wave with a Schwarzschild black hole. During this interaction, the black hole absorbs a fraction of the incoming energy, converting it into rotational and translational kinetic energies. The remaining energy is then carried away by the reflected gravitational wave. This article focuses on examining the characteristics of the reflected wave and analyzing the amount of energy absorbed by the black hole.
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