What question did this study set out to answer?

The research aims to validate Higgs Quantum Gravity Theory by analyzing its application to Sagittarius A* and understanding spin interactions.

April 3, 2026Open Access

Validation of the Higgs Quantum Gravity Theory HQGFT under Extreme Gravitational Regimes A Case Study of Sagittarius A Spin and Accretion Anomalies

Key Points

The research aims to validate Higgs Quantum Gravity Theory by analyzing its application to Sagittarius A* and understanding spin interactions.
Employed a high-fidelity stochastic simulation framework with 10,000 iterations
Analyzed electron spin interactions with the local Higgs field density
Investigated gravitational effects within Kerr curvature
Identified optimal spin of a = 0.92 that minimizes residual error (χ2 ≈ 1.20)
Provided unprecedented precision in modeling extreme orbits around Sagittarius A*
Discussed HQGFT's solution to low-luminosity jet anomalies
Established predictions related to gravitational saturation with the Magellanic Cloud's interaction

Abstract

This scientific treatise presents a comprehensive validation of the Higgs QuantumGravity Theory (HQGFT) applied to the supermassive black hole Sagittarius A*(Sgr A*). Utilizing a high-fidelity stochastic simulation framework with 10,000iterations, we analyze the fundamental interaction between electron spin and thelocal Higgs field density within the Kerr curvature. Results derived from the analysisof the S2 star demonstrate that a spin of a = 0.92 minimizes residual error (χ2 ≈1.20), providing unprecedented precision in modeling extreme orbits. Furthermore,the HQGFT solution to the low-luminosity jet mystery is discussed, and a temporalprediction for gravitational saturation during the imminent interaction with theMagellanic Cloud is established.

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