Can relativistic beaming of gravity explain the surprising results of the James Webb Space Telescope Deep Field regarding the early universe?

The hypothesis of gravitational beaming says that compact objects such as supermassive black holes, stellar mass black holes and neutron stars, if their cores are rotating near the speed of light, emit approximately 1/r gravitational force into their rotational plane. If SgrA* participates in this process, then it would be interesting to see what would be the long-term effects on the S stars orbiting SgrA*. I wrote a MATLAB program using the impulse approximation to calculate the change in the orbital elements that would result from each crossing of the orbital plane. Then I examined the expected change in the orbits of various S stars. Some S stars orbits degraded, indicating that supermassive black holes may be active feeders. Other S stars orbits gained energy and became more radial, ultimately reaching escape velocity. These S stars would apparently then enter radial orbits of the center of mass of the bulge. These results suggest that in the early universe, supermassive black holes, as active eaters, would grow faster that predicted by ΛCDM theory, and that they would actively form bulges or elipticals around themselves, leading to early formation of mature galaxies. Additionally, since the S stars escaping SgrA* would do so at the escape velocity of the black hole, this could lead to a solution of the enigmatic M_bh -σ relation.