Morphology-Dependent Gravitational Corrections from Integration-Limited Coherence

Key Points

• This research aims to explore how morphological structure affects gravitational corrections in systems influenced by dark matter.
• Analyzed deviations from Newtonian and General Relativistic predictions at galactic scales.
• Evaluated the relationship between baryonic mass and internal morphological structure.
• Utilized theoretical models to assess various galactic configurations.
• Identified significant deviations from expected gravitational behaviors at large scales.
• Found that gravitational correction magnitudes are influenced by the system's morphology and baryonic mass.