Forcefield Analysis in Sagittarius A* and Hypothetical Second Black Hole

This paper presents a theoretical forcefield analysis of Sagittarius A*, the supermassive black hole at the center of the Milky Way, and a hypothetical secondary black hole. Recent observations suggest that Sagittarius A* may exhibit an elongated structure rather than a purely spherical shape. We hypothesize that this elongation could be due to gravitational interactions with an unseen second black hole. To investigate this possibility, we calculated gravitational forces, graviton corrections, centrifugal forces, and gravitational wave strengths within this system, using distances ranging from to meters between Sagittarius A* and the hypothetical companion. Our approach incorporates the mass of Sagittarius A* () and the hypothetical second black hole (), along with their Schwarzschild radii and gravitational constants. Notably, we considered the accretion disk’s rotation at 60% of the speed of light around Sagittarius A*, which adds a significant centrifugal force component. This setup allows us to simulate the gravitational field and assess its elongation effects, illustrating potential asymmetries in the gravitational structure that may align with observational data. Our findings include visualized gravitational force fields for both objects and the elongation axis’s directional bias. This analysis aims to support the scientific community in exploring the hypothesis of an additional black hole within the vicinity of Sagittarius A*, as well as further validating the elongated structure. The visualizations provided could serve as a basis for additional studies using instruments such as the Event Horizon Telescope to confirm or refute these findings.